A |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
a |
twomass_psc |
TWOMASS |
Catalog identifier of an optical source from either the Tycho 2 or USNO-A2.0 catalog that falls within ~5" of the TWOMASS source position. |
varchar |
1 |
|
|
meta.id |
A1 |
mgcGalaxyStruct |
MGC |
Asymmetry index (background corrected) alpha=1 |
real |
4 |
|
99.99 |
|
A2 |
mgcGalaxyStruct |
MGC |
Asymmetry index (background corrected) alpha=2 |
real |
4 |
|
99.99 |
|
A3 |
mgcGalaxyStruct |
MGC |
Asymmetry index (background corrected) alpha=3 |
real |
4 |
|
99.99 |
|
A4 |
mgcGalaxyStruct |
MGC |
Asymmetry index (background corrected) alpha=4 |
real |
4 |
|
99.99 |
|
A_B |
twomass |
SIXDF |
minor/major axis ratio fit to 3-sig. super-coadd isophote |
real |
4 |
|
|
|
a_g_percentile_lower |
gaia_source |
GAIADR2 |
Lower uncertainty on A_G |
real |
4 |
mag |
|
phys.absorption.gal;stat.min |
a_g_percentile_upper |
gaia_source |
GAIADR2 |
Upper uncertainty on A_G |
real |
4 |
mag |
|
phys.absorption.gal;stat.max |
a_g_val |
gaia_source |
GAIADR2 |
Line-of-sight extinction in the G band, A_G |
real |
4 |
mag |
|
phys.absorption.gal |
A_IMAGE |
mgcDetection |
MGC |
Flux rms along major axis |
real |
4 |
pixel |
|
|
A_V |
target |
SIXDF |
Schlegel V extinction |
real |
4 |
|
|
|
ab_flags |
catwise_2020, catwise_prelim |
WISE |
Two character (W1 W2) artifact flag |
varchar |
9 |
|
|
|
abbe |
phot_variable_time_series_g_fov_statistical_parameters |
GAIADR1 |
Abbe value of the G-band time series values |
float |
8 |
|
|
stat.value |
ABEMMA |
spectra |
SIXDF |
redshift type: abs=1,emi=2,man=3 |
int |
4 |
|
|
|
abMagLim |
MultiframeDetector |
SHARKSv20210222 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
SHARKSv20210421 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
ULTRAVISTADR4 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSDR1 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSDR2 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSDR3 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSDR4 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSDR5 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSDR6 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20120926 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20130417 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20140409 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20150108 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20160114 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20160507 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20170630 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20180419 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20201209 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20231101 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VHSv20240731 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIDEODR2 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIDEODR3 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIDEODR4 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIDEODR5 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIDEOv20111208 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGDR2 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGDR3 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGDR4 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGv20110714 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGv20111019 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGv20130417 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGv20140402 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGv20150421 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGv20151230 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGv20160406 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGv20161202 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VIKINGv20170715 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCDEEPv20230713 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCDEEPv20240506 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCDR1 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCDR2 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCDR3 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCDR4 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCDR5 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20110816 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20110909 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20120126 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20121128 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20130304 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20130805 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20140428 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20140903 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20150309 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20151218 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20160311 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20160822 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20170109 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20170411 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20171101 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20180702 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20181120 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20191212 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20210708 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20230816 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VMCv20240226 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VVVDR1 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VVVDR2 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VVVDR5 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VVVXDR1 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VVVv20110718 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
5-sigma limiting AB magnitude for point sources |
real |
4 |
mag |
-0.9999995e9 |
|
ABS_CSB_BULGE |
mgcGalaxyStruct |
MGC |
Absolute Central Surface Brightness of Bulge |
real |
4 |
Vega mag/sq arcsec |
99.99 |
|
ABS_CSB_DISK |
mgcGalaxyStruct |
MGC |
Absolute Central Surface Brightness of Disk |
real |
4 |
Vega mag/sq arcsec |
99.99 |
|
ABS_ESB_BULGE |
mgcGalaxyStruct |
MGC |
Absolute Effective Surface Brightness of Bulge |
real |
4 |
Vega mag/sq arcsec |
99.99 |
|
ABS_ESB_DISK |
mgcGalaxyStruct |
MGC |
Absolute Effective Surface Brightness of Disk |
real |
4 |
Vega mag/sq arcsec |
99.99 |
|
ABS_HLRSB_BULG |
mgcGalaxyStruct |
MGC |
Absolute Surface Brightness at Re |
real |
4 |
Vega mag/sq arcsec |
99.99 |
|
ABS_HLRSB_DISK |
mgcGalaxyStruct |
MGC |
Absolute Surface Brightness at 1.678alpha |
real |
4 |
Vega mag/sq arcsec |
99.99 |
|
ABS_MAG_GIM2D |
mgcGalaxyStruct |
MGC |
GIM2D B Absolute Disk mag, dust and K & E-corrected |
real |
4 |
Vega mag |
99.99 |
|
ABS_MAG_GIM2DB |
mgcGalaxyStruct |
MGC |
GIM2D B Absolute mag, dust and K & E-corrected |
real |
4 |
Vega mag |
99.99 |
|
ABS_MAG_GIM2DD |
mgcGalaxyStruct |
MGC |
GIM2D B Absolute Bulge mag, dust and K & E-corrected |
real |
4 |
Vega mag |
99.99 |
|
ABS_SB_B |
mgcGalaxyStruct |
MGC |
MGC B Absolute KRON SB, dust K & E-corrected |
real |
4 |
Vega mag |
-99.000 |
|
ABS_SB_g |
mgcGalaxyStruct |
MGC |
SDSS g Absolute PET SB, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
ABS_SB_i |
mgcGalaxyStruct |
MGC |
SDSS i Absolute PET SB, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
ABS_SB_r |
mgcGalaxyStruct |
MGC |
SDSS r Absolute PET SB, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
ABS_SB_u |
mgcGalaxyStruct |
MGC |
SDSS u Absolute PET SB, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
ABS_SB_z |
mgcGalaxyStruct |
MGC |
SDSS z Absolute PET SB, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
abSatMag |
MultiframeDetector |
SHARKSv20210222 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
SHARKSv20210421 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
ULTRAVISTADR4 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSDR1 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSDR2 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSDR3 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSDR4 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSDR5 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSDR6 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20120926 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20130417 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20140409 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20150108 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20160114 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20160507 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20170630 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20180419 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20201209 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20231101 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VHSv20240731 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIDEODR2 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIDEODR3 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIDEODR4 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIDEODR5 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIDEOv20111208 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGDR2 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGDR3 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGDR4 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGv20110714 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGv20111019 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGv20130417 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGv20140402 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGv20150421 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGv20151230 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGv20160406 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGv20161202 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VIKINGv20170715 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCDEEPv20230713 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCDEEPv20240506 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCDR1 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCDR2 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCDR3 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCDR4 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCDR5 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20110816 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20110909 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20120126 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20121128 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20130304 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20130805 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20140428 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20140903 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20150309 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20151218 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20160311 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20160822 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20170109 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20170411 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20171101 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20180702 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20181120 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20191212 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20210708 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20230816 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VMCv20240226 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VVVDR1 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VVVDR2 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VVVDR5 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VVVXDR1 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VVVv20110718 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Saturation limit for point sources (AB magnitude) |
real |
4 |
mag |
-0.9999995e9 |
|
absMagPsf_g |
mgcGalaxyStruct |
MGC |
SDSS g Absolute PSF mag, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
absMagPsf_i |
mgcGalaxyStruct |
MGC |
SDSS i Absolute PSF mag, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
absMagPsf_r |
mgcGalaxyStruct |
MGC |
SDSS r Absolute PSF mag, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
absMagPsf_u |
mgcGalaxyStruct |
MGC |
SDSS u Absolute PSF mag, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
absMagPsf_z |
mgcGalaxyStruct |
MGC |
SDSS z Absolute PSF mag, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
absMagPt_B |
mgcGalaxyStruct |
MGC |
MGC B Absolute KRON mag, dust K & E-corrected |
real |
4 |
Vega mag |
-99.000 |
|
absMagPt_g |
mgcGalaxyStruct |
MGC |
SDSS g Absolute PET mag, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
absMagPt_i |
mgcGalaxyStruct |
MGC |
SDSS i Absolute PET mag, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
absMagPt_r |
mgcGalaxyStruct |
MGC |
SDSS r Absolute PET mag, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
absMagPt_u |
mgcGalaxyStruct |
MGC |
SDSS u Absolute PET mag, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
absMagPt_z |
mgcGalaxyStruct |
MGC |
SDSS z Absolute PET mag, dust K & E-corrected |
real |
4 |
AB mag |
-99.000 |
|
ACTMJD_R |
spectra |
SIXDF |
the time the field was actually configured |
float |
8 |
Julian days |
|
|
ACTMJD_V |
spectra |
SIXDF |
the time the field was actually configured |
float |
8 |
Julian days |
|
|
addSurveyList |
RequiredMatchedApertureProduct |
SHARKSv20210222 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
SHARKSv20210421 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
ULTRAVISTADR4 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VHSv20201209 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VHSv20231101 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VHSv20240731 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VMCDEEPv20230713 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VMCDEEPv20240506 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VMCDR5 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VMCv20191212 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VMCv20210708 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VMCv20230816 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VMCv20240226 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VVVDR5 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
addSurveyList |
RequiredMatchedApertureProduct |
VVVXDR1 |
List of external surveys that are included in the matched aperture tables |
varchar |
256 |
|
NONE |
|
adjacentFrameTolerance |
Programme |
SHARKSv20210222 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
SHARKSv20210421 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
ULTRAVISTADR4 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSDR1 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSDR2 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSDR3 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSDR4 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSDR5 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSDR6 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSv20120926 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSv20130417 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSv20150108 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSv20160114 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSv20160507 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSv20170630 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSv20180419 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSv20201209 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSv20231101 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VHSv20240731 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIDEODR2 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIDEODR3 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIDEODR4 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIDEODR5 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIDEOv20100513 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIDEOv20111208 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGDR2 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGDR3 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGDR4 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGv20110714 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGv20111019 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGv20130417 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGv20150421 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGv20151230 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGv20160406 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGv20161202 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VIKINGv20170715 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCDEEPv20230713 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCDEEPv20240506 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCDR1 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCDR3 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCDR4 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCDR5 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20110816 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20110909 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20120126 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20121128 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20130304 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20130805 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20140428 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20140903 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20150309 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20151218 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20160311 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20160822 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20170109 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20170411 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20171101 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20180702 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20181120 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20191212 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20210708 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20230816 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VMCv20240226 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VSAQC |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VVVDR1 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VVVDR2 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VVVDR5 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VVVXDR1 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VVVv20100531 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VVVv20110718 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
aebv |
Filter |
SHARKSv20210421 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
ULTRAVISTADR4 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSDR1 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSDR2 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSDR3 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSDR4 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSDR5 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSDR6 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSv20120926 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSv20130417 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSv20150108 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSv20160114 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSv20160507 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSv20170630 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSv20180419 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSv20201209 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSv20231101 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VHSv20240731 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIDEODR2 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIDEODR3 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIDEODR4 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIDEODR5 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIDEOv20100513 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIDEOv20111208 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGDR2 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGDR3 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGDR4 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGv20110714 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGv20111019 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGv20130417 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGv20150421 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGv20151230 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGv20160406 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGv20161202 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VIKINGv20170715 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCDEEPv20230713 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCDEEPv20240506 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCDR1 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCDR3 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCDR4 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCDR5 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20110816 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20110909 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20120126 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20121128 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20130304 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20130805 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20140428 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20140903 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20150309 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20151218 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20160311 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20160822 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20170109 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20170411 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20171101 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20180702 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20181120 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20191212 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20210708 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20230816 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VMCv20240226 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VSAQC |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VVVDR1 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VVVDR2 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VVVDR5 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VVVXDR1 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VVVv20100531 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VVVv20110718 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter, FilterSections |
SHARKSv20210222 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aEBVCard |
FilterExtinctionCoefficients |
EXTINCT |
The constant to multiply the E(B-V) value by to get the extinction in the Cardelli et al. (1989) system. |
real |
4 |
|
-0.9999995e9 |
|
aEHKsCard |
FilterExtinctionCoefficients |
EXTINCT |
The constant to multiply the E(H-Ks) value by to get the extinction in the Cardelli et al. (1989) system. |
real |
4 |
|
-0.9999995e9 |
|
aEHKsNish |
FilterExtinctionCoefficients |
EXTINCT |
The constant to multiply the E(H-Ks) value by to get the extinction in the Nishiyama et al. (2009) system. |
real |
4 |
|
-0.9999995e9 |
|
aEJKsCard |
FilterExtinctionCoefficients |
EXTINCT |
The constant to multiply the E(J-Ks) value by to get the extinction in the Cardelli et al. (1989) system. |
real |
4 |
|
-0.9999995e9 |
|
aEJKsNish |
FilterExtinctionCoefficients |
EXTINCT |
The constant to multiply the E(J-Ks) value by to get the extinction in the Nishiyama et al. (2009) system. |
real |
4 |
|
-0.9999995e9 |
|
aH |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSDR1 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aH |
vhsSource |
VHSDR2 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aH |
vhsSource |
VHSDR3 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSDR4 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSDR5 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSDR6 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20120926 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20130417 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20140409 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20150108 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20160114 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20160507 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20170630 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20180419 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20201209 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20231101 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vhsSource |
VHSv20240731 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
videoSource |
VIDEODR2 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aH |
videoSource |
VIDEODR3 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
videoSource |
VIDEODR4 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
videoSource |
VIDEODR5 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
videoSource |
VIDEOv20100513 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aH |
videoSource |
VIDEOv20111208 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aH |
vikingSource |
VIKINGDR2 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aH |
vikingSource |
VIKINGDR3 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vikingSource |
VIKINGDR4 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vikingSource |
VIKINGv20110714 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aH |
vikingSource |
VIKINGv20111019 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aH |
vikingSource |
VIKINGv20130417 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vikingSource |
VIKINGv20140402 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vikingSource |
VIKINGv20150421 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vikingSource |
VIKINGv20151230 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vikingSource |
VIKINGv20160406 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vikingSource |
VIKINGv20161202 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vikingSource |
VIKINGv20170715 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aH |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
air_temp |
twomass_scn |
TWOMASS |
Air temperature at beginning of scan. |
real |
4 |
degC |
|
phys.temperature |
air_temp |
twomass_sixx2_scn |
TWOMASS |
air temperature (deg C) at beginning of scan |
real |
4 |
degC |
|
|
airm |
twomass_scn |
TWOMASS |
Airmass at beginning of scan. |
real |
4 |
|
|
obs.airMass |
airm |
twomass_sixx2_scn |
TWOMASS |
beginning airmass of scan |
real |
4 |
|
|
|
airMass |
Detection |
PS1DR2 |
Airmass at midpoint of the exposure. Necessary for converting listed fluxes and magnitudes back to measured ADU counts. |
real |
4 |
|
0 |
|
aJ |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSDR1 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aJ |
vhsSource |
VHSDR2 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aJ |
vhsSource |
VHSDR3 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSDR4 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSDR5 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSDR6 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20120926 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20130417 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20140409 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20150108 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20160114 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20160507 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20170630 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20180419 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20201209 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20231101 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vhsSource |
VHSv20240731 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
videoSource |
VIDEODR2 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aJ |
videoSource |
VIDEODR3 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
videoSource |
VIDEODR4 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
videoSource |
VIDEODR5 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
videoSource |
VIDEOv20100513 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aJ |
videoSource |
VIDEOv20111208 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aJ |
vikingSource |
VIKINGDR2 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aJ |
vikingSource |
VIKINGDR3 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vikingSource |
VIKINGDR4 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vikingSource |
VIKINGv20110714 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aJ |
vikingSource |
VIKINGv20111019 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aJ |
vikingSource |
VIKINGv20130417 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vikingSource |
VIKINGv20140402 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vikingSource |
VIKINGv20150421 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vikingSource |
VIKINGv20151230 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vikingSource |
VIKINGv20160406 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vikingSource |
VIKINGv20161202 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vikingSource |
VIKINGv20170715 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aJ |
vvvPsfDaophotJKsSource |
VVVDR5 |
The galactic extinction correction in the J band for objects at the distance of the Galactic Centre {catalogue TType keyword: aj} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
sharksSource |
SHARKSv20210222 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
sharksSource |
SHARKSv20210421 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSDR1 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
vhsSource |
VHSDR2 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
vhsSource |
VHSDR3 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSDR4 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSDR5 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSDR6 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20120926 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20130417 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20140409 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20150108 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20160114 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20160507 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20170630 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20180419 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20201209 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20231101 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vhsSource |
VHSv20240731 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
videoSource |
VIDEODR2 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
videoSource |
VIDEODR3 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
videoSource |
VIDEODR4 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
videoSource |
VIDEODR5 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
videoSource |
VIDEOv20100513 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
videoSource |
VIDEOv20111208 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
vikingSource |
VIKINGDR2 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
vikingSource |
VIKINGDR3 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vikingSource |
VIKINGDR4 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vikingSource |
VIKINGv20110714 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
vikingSource |
VIKINGv20111019 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
vikingSource |
VIKINGv20130417 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vikingSource |
VIKINGv20140402 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vikingSource |
VIKINGv20150421 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vikingSource |
VIKINGv20151230 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vikingSource |
VIKINGv20160406 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vikingSource |
VIKINGv20161202 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vikingSource |
VIKINGv20170715 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aKs |
vvvPsfDaophotJKsSource |
VVVDR5 |
The galactic extinction correction in the Ks band for objects at the distance of the Galactic Centre {catalogue TType keyword: ak} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aks |
vmcRRLyraeVariables |
VMCv20240226 |
The dust absorption in the Ks-band {catalogue TType keyword: AKs} |
real |
4 |
mag |
99.0 |
phys.absorption.gal |
Al |
ravedr5Source |
RAVE |
[Al/H] abundance of Al |
real |
4 |
dex |
|
phys.abund.Z |
Al_N |
ravedr5Source |
RAVE |
Number of used spectral lines in calc. of [Al/H] |
smallint |
2 |
|
|
meta.number |
Algo_Conv_K |
ravedr5Source |
RAVE |
Quality Flag for Stellar Parameter pipeline,[0..4] |
int |
4 |
|
|
meta.code.qual |
allwise_cntr |
masterDR2 |
SKYMAPPER |
Unique identifier (cntr) of closest AllWISE source |
bigint |
8 |
|
|
meta.id.cross |
allwise_dist |
masterDR2 |
SKYMAPPER |
Distance on sky to closest AllWISE source |
real |
4 |
arcsec |
|
pos.angDistance |
Alpha_c |
ravedr5Source |
RAVE |
[Alpha/Fe] [Chemical pipeline] (Note 2) |
real |
4 |
dex |
|
phys.abund |
amEnd |
Multiframe |
SHARKSv20210222 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
SHARKSv20210421 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
ULTRAVISTADR4 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSDR1 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSDR2 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSDR3 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSDR4 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSDR5 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSDR6 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20120926 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20130417 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20140409 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20150108 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20160114 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20160507 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20170630 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20180419 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20201209 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20231101 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VHSv20240731 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIDEODR2 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIDEODR3 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIDEODR4 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIDEODR5 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIDEOv20100513 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIDEOv20111208 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGDR2 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGDR3 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGDR4 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGv20110714 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGv20111019 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGv20130417 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGv20140402 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGv20150421 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGv20151230 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGv20160406 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGv20161202 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VIKINGv20170715 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCDEEPv20230713 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCDEEPv20240506 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCDR1 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCDR2 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCDR3 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCDR4 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCDR5 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20110816 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20110909 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20120126 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20121128 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20130304 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20130805 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20140428 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20140903 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20150309 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20151218 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20160311 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20160822 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20170109 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20170411 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20171101 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20180702 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20181120 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20191212 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20210708 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20230816 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VMCv20240226 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VVVDR1 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VVVDR2 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VVVDR5 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VVVXDR1 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VVVv20100531 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
Multiframe |
VVVv20110718 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amEnd |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Airmass at end of observation |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
ampI |
ogle4CepLmcSource, ogle4CepSmcSource, ogle4RRLyrLmcSource, ogle4RRLyrSmcSource |
OGLE |
I-band amplitude (maximum-minimum) |
real |
4 |
mag |
|
src.var.amplitude |
ampI1 |
ogle3LpvLmcSource, ogle3LpvSmcSource |
OGLE |
I-band amplitude of the primary period |
real |
4 |
mag |
|
src.var.amplitude |
ampI2 |
ogle3LpvLmcSource, ogle3LpvSmcSource |
OGLE |
I-band amplitude of the secondary period |
real |
4 |
mag |
|
src.var.amplitude |
ampI3 |
ogle3LpvLmcSource, ogle3LpvSmcSource |
OGLE |
I-band amplitude of the tertiary period |
real |
4 |
mag |
|
src.var.amplitude |
amStart |
Multiframe |
SHARKSv20210222 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
SHARKSv20210421 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
ULTRAVISTADR4 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSDR1 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSDR2 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSDR3 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSDR4 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSDR5 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSDR6 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20120926 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20130417 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20140409 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20150108 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20160114 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20160507 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20170630 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20180419 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20201209 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20231101 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VHSv20240731 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIDEODR2 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIDEODR3 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIDEODR4 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIDEODR5 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIDEOv20100513 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIDEOv20111208 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGDR2 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGDR3 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGDR4 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGv20110714 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGv20111019 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGv20130417 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGv20140402 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGv20150421 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGv20151230 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGv20160406 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGv20161202 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VIKINGv20170715 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCDEEPv20230713 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCDEEPv20240506 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCDR1 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCDR2 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCDR3 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCDR4 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCDR5 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20110816 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20110909 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20120126 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20121128 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20130304 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20130805 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20140428 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20140903 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20150309 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20151218 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20160311 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20160822 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20170109 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20170411 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20171101 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20180702 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20181120 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20191212 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20210708 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20230816 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VMCv20240226 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VVVDR1 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VVVDR2 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VVVDR5 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VVVXDR1 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VVVv20100531 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
Multiframe |
VVVv20110718 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
amStart |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Airmass at start of observation |
real |
4 |
|
-0.9999995e9 |
obs.airMass |
aNb118 |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
The galactic extinction correction in the Nb118 band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
ANCHOR_PARITY |
mgcGalaxyStruct |
MGC |
0=OK, 1=Inverted, 2=LSB BULGE |
tinyint |
1 |
|
9 (FIX) |
|
ANCHOR_POINT |
mgcGalaxyStruct |
MGC |
Radius at which MU_BULGE=MU_DISK |
real |
4 |
kpc |
9 |
|
ANCHOR_SB |
mgcGalaxyStruct |
MGC |
Surface brightness at Anchor Point |
real |
4 |
Vega mag/sq arcsec |
99.99 |
|
anom |
twomass_scn |
TWOMASS |
Special flag indicating whether or not an unusual problem was found in the Atlas Images for this scan. |
smallint |
2 |
|
|
meta.code |
anom |
twomass_sixx2_scn |
TWOMASS |
entry in coadd anomaly table (0:not found|1:found) |
smallint |
2 |
|
|
|
AORNumber24 |
sage_lmcMips24Source |
SPITZER |
Request key for the 1st AOR within which the source appears |
int |
4 |
|
|
|
Ap35mag_I |
denisDR3Source |
DENIS |
Magnitude in I band from 3.5" aperture |
float |
8 |
mag |
|
|
Ap35mag_J |
denisDR3Source |
DENIS |
Magnitude in J band from 3.5" aperture |
float |
8 |
mag |
|
|
Ap35mag_K |
denisDR3Source |
DENIS |
Magnitude in K band from 3.5" aperture |
float |
8 |
mag |
|
|
Ap45mag_I |
denisDR3Source |
DENIS |
Magnitude in I band from 4.5" aperture |
float |
8 |
mag |
|
|
Ap45mag_J |
denisDR3Source |
DENIS |
Magnitude in J band from 4.5" aperture |
float |
8 |
mag |
|
|
Ap45mag_K |
denisDR3Source |
DENIS |
Magnitude in K band from 4.5" aperture |
float |
8 |
mag |
|
|
Ap55mag_I |
denisDR3Source |
DENIS |
Magnitude in I band from 5.5" aperture |
float |
8 |
mag |
|
|
Ap55mag_J |
denisDR3Source |
DENIS |
Magnitude in J band from 5.5" aperture |
float |
8 |
mag |
|
|
Ap55mag_K |
denisDR3Source |
DENIS |
Magnitude in K band from 5.5" aperture |
float |
8 |
mag |
|
|
Ap_Rmag |
combo17CDFSSource |
COMBO17 |
aperture magnitude in R |
real |
4 |
mag |
|
|
Apc15mag_I |
denisDR3Source |
DENIS |
I band Magnitude in 1.5" corr. aperture |
float |
8 |
mag |
|
|
Apc15mag_J |
denisDR3Source |
DENIS |
J band Magnitude in 1.5" corr. aperture |
float |
8 |
mag |
|
|
Apc15mag_K |
denisDR3Source |
DENIS |
K band Magnitude in 1.5" corr. aperture |
float |
8 |
mag |
|
|
Apc25mag_I |
denisDR3Source |
DENIS |
I band Magnitude in 2.5" corr. aperture |
float |
8 |
mag |
|
|
Apc25mag_J |
denisDR3Source |
DENIS |
J band Magnitude in 2.5" corr. aperture |
float |
8 |
mag |
|
|
Apc25mag_K |
denisDR3Source |
DENIS |
K band Magnitude in 2.5" corr. aperture |
float |
8 |
mag |
|
|
Apc35mag_I |
denisDR3Source |
DENIS |
I band Magnitude in 3.5" corr. aperture |
float |
8 |
mag |
|
|
Apc35mag_J |
denisDR3Source |
DENIS |
J band Magnitude in 3.5" corr. aperture |
float |
8 |
mag |
|
|
Apc35mag_K |
denisDR3Source |
DENIS |
K band Magnitude in 3.5" corr. aperture |
float |
8 |
mag |
|
|
ApD_Rmag |
combo17CDFSSource |
COMBO17 |
aperture difference of Rmag (=Rmag-Ap_Rmag, zero for point sources) |
real |
4 |
mag |
|
|
aperCor1 |
MultiframeDetector |
SHARKSv20210222 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
SHARKSv20210421 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
ULTRAVISTADR4 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSDR1 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSDR2 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSDR3 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSDR4 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSDR5 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSDR6 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20120926 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20130417 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20140409 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20150108 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20160114 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20160507 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20170630 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20180419 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20201209 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20231101 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VHSv20240731 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIDEODR2 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIDEODR3 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIDEODR4 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIDEODR5 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIDEOv20100513 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIDEOv20111208 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGDR2 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGDR3 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGDR4 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGv20110714 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGv20111019 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGv20130417 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGv20140402 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGv20150421 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGv20151230 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGv20160406 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGv20161202 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VIKINGv20170715 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCDEEPv20230713 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCDEEPv20240506 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCDR1 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCDR2 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCDR3 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCDR4 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCDR5 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20110816 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20110909 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20120126 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20121128 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20130304 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20130805 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20140428 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20140903 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20150309 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20151218 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20160311 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20160822 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20170109 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20170411 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20171101 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20180702 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20181120 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20191212 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20210708 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20230816 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VMCv20240226 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VVVDR1 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VVVDR2 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VVVDR5 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VVVXDR1 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VVVv20100531 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
MultiframeDetector |
VVVv20110718 |
Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor1 |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Stellar aperture correction: 1⁄2 × core flux |
real |
4 |
|
-0.9999995e9 |
?? |
aperCor2 |
MultiframeDetector |
SHARKSv20210222 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
SHARKSv20210421 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
ULTRAVISTADR4 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSDR1 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSDR2 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSDR3 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSDR4 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSDR5 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSDR6 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20120926 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20130417 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20140409 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20150108 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20160114 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20160507 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20170630 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20180419 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20201209 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20231101 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VHSv20240731 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIDEODR2 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIDEODR3 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIDEODR4 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIDEODR5 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIDEOv20100513 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIDEOv20111208 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGDR2 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGDR3 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGDR4 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGv20110714 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGv20111019 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGv20130417 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGv20140402 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGv20150421 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGv20151230 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGv20160406 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGv20161202 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VIKINGv20170715 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCDEEPv20230713 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCDEEPv20240506 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCDR1 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCDR2 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCDR3 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCDR4 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCDR5 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20110816 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20110909 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20120126 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20121128 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20130304 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20130805 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20140428 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20140903 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20150309 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20151218 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20160311 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20160822 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20170109 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20170411 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20171101 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20180702 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20181120 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20191212 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20210708 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20230816 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VMCv20240226 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VVVDR1 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VVVDR2 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VVVDR5 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VVVXDR1 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VVVv20100531 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
MultiframeDetector |
VVVv20110718 |
Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor2 |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Stellar aperture correction: 1⁄√2 core flux |
real |
4 |
|
-0.9999995e9 |
?? |
aperCor3 |
MultiframeDetector |
SHARKSv20210222 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
SHARKSv20210421 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
ULTRAVISTADR4 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSDR1 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSDR2 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSDR3 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSDR4 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSDR5 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSDR6 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20120926 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20130417 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20140409 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20150108 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20160114 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20160507 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20170630 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20180419 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20201209 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20231101 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VHSv20240731 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIDEODR2 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIDEODR3 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIDEODR4 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIDEODR5 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIDEOv20100513 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIDEOv20111208 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGDR2 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGDR3 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGDR4 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGv20110714 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGv20111019 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGv20130417 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGv20140402 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGv20150421 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGv20151230 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGv20160406 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGv20161202 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VIKINGv20170715 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCDEEPv20230713 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCDEEPv20240506 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCDR1 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCDR2 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCDR3 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCDR4 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCDR5 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20110816 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20110909 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20120126 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20121128 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20130304 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20130805 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20140428 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20140903 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20150309 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20151218 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20160311 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20160822 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20170109 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20170411 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20171101 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20180702 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20181120 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20191212 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20210708 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20230816 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VMCv20240226 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VVVDR1 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VVVDR2 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VVVDR5 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VVVXDR1 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VVVv20100531 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
MultiframeDetector |
VVVv20110718 |
Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor3 |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Stellar aperture correction: core flux |
real |
4 |
|
-0.9999995e9 |
?? |
aperCor4 |
MultiframeDetector |
SHARKSv20210222 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
SHARKSv20210421 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
ULTRAVISTADR4 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSDR1 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSDR2 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSDR3 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSDR4 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSDR5 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSDR6 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20120926 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20130417 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20140409 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20150108 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20160114 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20160507 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20170630 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20180419 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20201209 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20231101 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VHSv20240731 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIDEODR2 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIDEODR3 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIDEODR4 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIDEODR5 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIDEOv20100513 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIDEOv20111208 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGDR2 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGDR3 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGDR4 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGv20110714 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGv20111019 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGv20130417 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGv20140402 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGv20150421 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGv20151230 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGv20160406 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGv20161202 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VIKINGv20170715 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCDEEPv20230713 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCDEEPv20240506 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCDR1 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCDR2 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCDR3 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCDR4 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCDR5 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20110816 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20110909 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20120126 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20121128 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20130304 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20130805 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20140428 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20140903 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20150309 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20151218 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20160311 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20160822 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20170109 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20170411 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20171101 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20180702 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20181120 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20191212 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20210708 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20230816 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VMCv20240226 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VVVDR1 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VVVDR2 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VVVDR5 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VVVXDR1 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VVVv20100531 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
MultiframeDetector |
VVVv20110718 |
Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor4 |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Stellar aperture correction: √2 × core flux |
real |
4 |
|
-0.9999995e9 |
?? |
aperCor5 |
MultiframeDetector |
SHARKSv20210222 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
SHARKSv20210421 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
ULTRAVISTADR4 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSDR1 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSDR2 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSDR3 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSDR4 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSDR5 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSDR6 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20120926 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20130417 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20140409 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20150108 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20160114 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20160507 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20170630 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20180419 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20201209 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20231101 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VHSv20240731 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIDEODR2 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIDEODR3 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIDEODR4 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIDEODR5 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIDEOv20100513 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIDEOv20111208 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGDR2 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGDR3 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGDR4 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGv20110714 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGv20111019 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGv20130417 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGv20140402 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGv20150421 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGv20151230 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGv20160406 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGv20161202 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VIKINGv20170715 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCDEEPv20230713 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCDEEPv20240506 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCDR1 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCDR2 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCDR3 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCDR4 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCDR5 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20110816 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20110909 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20120126 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20121128 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20130304 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20130805 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20140428 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20140903 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20150309 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20151218 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20160311 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20160822 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20170109 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20170411 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20171101 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20180702 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20181120 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20191212 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20210708 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20230816 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VMCv20240226 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VVVDR1 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VVVDR2 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VVVDR5 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VVVXDR1 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VVVv20100531 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
MultiframeDetector |
VVVv20110718 |
Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor5 |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Stellar aperture correction: 2 × core flux |
real |
4 |
|
-0.9999995e9 |
?? |
aperCor6 |
MultiframeDetector |
SHARKSv20210222 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
SHARKSv20210421 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
ULTRAVISTADR4 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSDR1 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSDR2 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSDR3 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSDR4 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSDR5 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSDR6 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20120926 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20130417 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20140409 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20150108 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20160114 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20160507 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20170630 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20180419 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20201209 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20231101 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VHSv20240731 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIDEODR2 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIDEODR3 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIDEODR4 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIDEODR5 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIDEOv20100513 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIDEOv20111208 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGDR2 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGDR3 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGDR4 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGv20110714 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGv20111019 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGv20130417 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGv20140402 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGv20150421 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGv20151230 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGv20160406 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGv20161202 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VIKINGv20170715 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCDEEPv20230713 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCDEEPv20240506 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCDR1 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCDR2 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCDR3 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCDR4 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCDR5 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20110816 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20110909 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20120126 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20121128 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20130304 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20130805 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20140428 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20140903 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20150309 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20151218 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20160311 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20160822 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20170109 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20170411 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20171101 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20180702 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20181120 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20191212 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20210708 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20230816 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VMCv20240226 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VVVDR1 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VVVDR2 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VVVDR5 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VVVXDR1 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VVVv20100531 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
MultiframeDetector |
VVVv20110718 |
Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor6 |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Stellar aperture correction: 2√2 × core flux |
real |
4 |
|
-0.9999995e9 |
?? |
aperCor7 |
MultiframeDetector |
SHARKSv20210222 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
SHARKSv20210421 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
ULTRAVISTADR4 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSDR1 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSDR2 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSDR3 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSDR4 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSDR5 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSDR6 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20120926 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20130417 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20140409 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20150108 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20160114 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20160507 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20170630 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20180419 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20201209 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20231101 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VHSv20240731 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIDEODR2 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIDEODR3 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIDEODR4 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIDEODR5 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIDEOv20100513 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIDEOv20111208 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGDR2 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGDR3 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGDR4 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGv20110714 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGv20111019 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGv20130417 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGv20140402 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGv20150421 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGv20151230 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGv20160406 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGv20161202 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VIKINGv20170715 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCDEEPv20230713 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCDEEPv20240506 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCDR1 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCDR2 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCDR3 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCDR4 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCDR5 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20110816 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20110909 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20120126 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20121128 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20130304 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20130805 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20140428 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20140903 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20150309 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20151218 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20160311 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20160822 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20170109 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20170411 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20171101 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20180702 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20181120 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20191212 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20210708 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20230816 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VMCv20240226 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VVVDR1 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VVVDR2 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VVVDR5 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VVVXDR1 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VVVv20100531 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
MultiframeDetector |
VVVv20110718 |
Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCor7 |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Stellar aperture correction: 4 × core flux |
real |
4 |
|
-0.9999995e9 |
?? |
aperCorPeak |
MultiframeDetector |
SHARKSv20210222 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
SHARKSv20210421 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
ULTRAVISTADR4 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSDR1 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSDR2 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSDR3 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSDR4 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSDR5 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSDR6 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20120926 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20130417 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20140409 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20150108 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20160114 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20160507 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20170630 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20180419 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20201209 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20231101 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VHSv20240731 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIDEODR2 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIDEODR3 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIDEODR4 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIDEODR5 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIDEOv20100513 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIDEOv20111208 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGDR2 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGDR3 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGDR4 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGv20110714 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGv20111019 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGv20130417 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGv20140402 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGv20150421 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGv20151230 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGv20160406 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGv20161202 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VIKINGv20170715 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCDEEPv20230713 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCDEEPv20240506 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCDR1 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCDR2 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCDR3 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCDR4 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCDR5 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20110816 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20110909 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20120126 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20121128 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20130304 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20130805 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20140428 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20140903 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20150309 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20151218 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20160311 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20160822 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20170109 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20170411 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20171101 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20180702 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20181120 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20191212 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20210708 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20230816 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VMCv20240226 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VVVDR1 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VVVDR2 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VVVDR5 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VVVXDR1 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VVVv20100531 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
MultiframeDetector |
VVVv20110718 |
Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real |
4 |
|
-0.9999995e9 |
?? |
Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. |
aperCorPeak |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Stellar aperture correction: peak height |
real |
4 |
|
-0.9999995e9 |
?? |
aperFlux1 |
sharksDetection |
SHARKSv20210222 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
sharksDetection |
SHARKSv20210421 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
ultravistaDetection |
ULTRAVISTADR4 |
Default aperture flux counts 1, no aperture correction applied (SE: FLUX_APER1) {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
Flux vector within fixed circular aperture, but no aperture correction. |
aperFlux1 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 1 (SE: FLUX_APER1) {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux1 |
vhsDetection |
VHSDR1 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSDR2 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSDR3 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSDR4 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSDR5 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSDR6 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20120926 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20130417 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20140409 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20150108 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20160114 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20160507 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20170630 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20180419 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20201209 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20231101 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsDetection |
VHSv20240731 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vhsListRemeasurement |
VHSDR1 |
default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
videoDetection |
VIDEODR2 |
Default aperture flux counts 1, no aperture correction applied (SE: FLUX_APER1) {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
Flux vector within fixed circular aperture, but no aperture correction. |
aperFlux1 |
videoDetection |
VIDEODR3 |
Default aperture flux counts 1, no aperture correction applied (SE: FLUX_APER1) {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
Flux vector within fixed circular aperture, but no aperture correction. |
aperFlux1 |
videoDetection |
VIDEODR4 |
Default aperture flux counts 1, no aperture correction applied (SE: FLUX_APER1) {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
Flux vector within fixed circular aperture, but no aperture correction. |
aperFlux1 |
videoDetection |
VIDEODR5 |
Default aperture flux counts 1, no aperture correction applied (SE: FLUX_APER1) {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
Flux vector within fixed circular aperture, but no aperture correction. |
aperFlux1 |
videoDetection |
VIDEOv20100513 |
Default aperture flux counts 1, no aperture correction applied (SE: FLUX_APER1) {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
Flux vector within fixed circular aperture, but no aperture correction. |
aperFlux1 |
videoDetection |
VIDEOv20111208 |
Default aperture flux counts 1, no aperture correction applied (SE: FLUX_APER1) {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
Flux vector within fixed circular aperture, but no aperture correction. |
aperFlux1 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGDR2 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGDR3 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGDR4 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGv20110714 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGv20111019 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGv20130417 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGv20140402 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGv20150421 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGv20151230 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGv20160406 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGv20161202 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingDetection |
VIKINGv20170715 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingListRemeasurement |
VIKINGv20111019 |
default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 1 (SE: FLUX_APER1) {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux1 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 1 (SE: FLUX_APER1) {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux1 |
vmcDetection |
VMCDR1 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCDR2 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCDR3 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCDR4 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCDR5 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20110816 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20110909 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20120126 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20121128 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20130304 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20130805 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20140428 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20140903 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20150309 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20151218 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20160311 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20160822 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20170109 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20170411 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20171101 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20180702 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20181120 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20191212 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20210708 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20230816 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcDetection |
VMCv20240226 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcListRemeasurement |
VMCv20110816 |
default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcListRemeasurement |
VMCv20110909 |
default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcdeepDetection |
VMCDEEPv20230713 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vmcdeepDetection |
VMCDEEPv20240506 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vvvDetection |
VVVDR1 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vvvDetection |
VVVDR2 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vvvDetection |
VVVv20100531 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
phot.count |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vvvListRemeasurement |
VVVv20100531 |
default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux1 |
vvvListRemeasurement |
VVVv20110718 |
default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. |
aperFlux10 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 10, no aperture correction applied (SE: FLUX_APER10) {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 10 (SE: FLUX_APER10) {catalogue TType keyword: Aper_flux_10} 7 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux10 |
vhsDetection |
VHSDR2 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
vhsDetection |
VHSDR3 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSDR4 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSDR5 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSDR6 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20120926 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20130417 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20140409 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20150108 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20160114 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20160507 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20170630 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20180419 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20201209 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20231101 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection |
VHSv20240731 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
videoDetection |
VIDEODR2 |
default aperture flux 10, no aperture correction applied (SE: FLUX_APER10) {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
videoDetection |
VIDEODR3 |
default aperture flux 10, no aperture correction applied (SE: FLUX_APER10) {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
videoDetection |
VIDEODR4 |
default aperture flux 10, no aperture correction applied (SE: FLUX_APER10) {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
videoDetection |
VIDEODR5 |
default aperture flux 10, no aperture correction applied (SE: FLUX_APER10) {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
videoDetection |
VIDEOv20100513 |
default aperture flux 10, no aperture correction applied (SE: FLUX_APER10) {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
videoDetection |
VIDEOv20111208 |
default aperture flux 10, no aperture correction applied (SE: FLUX_APER10) {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
vikingDetection |
VIKINGDR2 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
vikingDetection |
VIKINGDR3 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vikingDetection |
VIKINGDR4 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 10 (SE: FLUX_APER10) {catalogue TType keyword: Aper_flux_10} 7 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux10 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 10 (SE: FLUX_APER10) {catalogue TType keyword: Aper_flux_10} 7 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux10 |
vmcDetection |
VMCDR1 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
vmcDetection |
VMCDR2 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCDR3 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCDR4 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCDR5 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20110909 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
vmcDetection |
VMCv20120126 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
vmcDetection |
VMCv20121128 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20130304 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20130805 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20140428 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20140903 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20150309 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20151218 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20160311 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20160822 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20170109 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20170411 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20171101 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20180702 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20181120 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20191212 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20210708 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20230816 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection |
VMCv20240226 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vvvDetection |
VVVDR1 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vvvDetection |
VVVDR2 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux10 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux10err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 10 (SE: FLUXERR_APER10) {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux10err |
vhsDetection |
VHSDR2 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSDR3 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSDR4 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSDR5 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSDR6 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
videoDetection |
VIDEODR2 |
Error in aperture flux 10 (SE: FLUXERR_APER10) {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
videoDetection |
VIDEODR3 |
Error in aperture flux 10 (SE: FLUXERR_APER10) {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
videoDetection |
VIDEODR4 |
Error in aperture flux 10 (SE: FLUXERR_APER10) {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
videoDetection |
VIDEODR5 |
Error in aperture flux 10 (SE: FLUXERR_APER10) {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 10 (SE: FLUXERR_APER10) {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 10 (SE: FLUXERR_APER10) {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux10err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux10err |
vmcDetection |
VMCDR1 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCDR2 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCDR3 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCDR4 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCDR5 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vvvDetection |
VVVDR1 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vvvDetection |
VVVDR2 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux10err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 11, no aperture correction applied (SE: FLUX_APER11) {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 11 (SE: FLUX_APER11) {catalogue TType keyword: Aper_flux_11} 8 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux11 |
vhsDetection |
VHSDR2 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
vhsDetection |
VHSDR3 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSDR4 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSDR5 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSDR6 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20120926 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20130417 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20140409 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20150108 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20160114 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20160507 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20170630 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20180419 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20201209 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20231101 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection |
VHSv20240731 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
videoDetection |
VIDEODR2 |
default aperture flux 11, no aperture correction applied (SE: FLUX_APER11) {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
videoDetection |
VIDEODR3 |
default aperture flux 11, no aperture correction applied (SE: FLUX_APER11) {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
videoDetection |
VIDEODR4 |
default aperture flux 11, no aperture correction applied (SE: FLUX_APER11) {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
videoDetection |
VIDEODR5 |
default aperture flux 11, no aperture correction applied (SE: FLUX_APER11) {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
videoDetection |
VIDEOv20100513 |
default aperture flux 11, no aperture correction applied (SE: FLUX_APER11) {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
videoDetection |
VIDEOv20111208 |
default aperture flux 11, no aperture correction applied (SE: FLUX_APER11) {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
vikingDetection |
VIKINGDR2 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
vikingDetection |
VIKINGDR3 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vikingDetection |
VIKINGDR4 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 11 (SE: FLUX_APER11) {catalogue TType keyword: Aper_flux_11} 8 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux11 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 11 (SE: FLUX_APER11) {catalogue TType keyword: Aper_flux_11} 8 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux11 |
vmcDetection |
VMCDR1 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
vmcDetection |
VMCDR2 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCDR3 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCDR4 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCDR5 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20110909 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
vmcDetection |
VMCv20120126 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
vmcDetection |
VMCv20121128 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20130304 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20130805 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20140428 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20140903 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20150309 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20151218 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20160311 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20160822 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20170109 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20170411 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20171101 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20180702 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20181120 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20191212 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20210708 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20230816 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection |
VMCv20240226 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vvvDetection |
VVVDR1 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vvvDetection |
VVVDR2 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux11 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux11err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux11err |
vhsDetection |
VHSDR2 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSDR3 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSDR4 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSDR5 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSDR6 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
videoDetection |
VIDEODR2 |
Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
videoDetection |
VIDEODR3 |
Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
videoDetection |
VIDEODR4 |
Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
videoDetection |
VIDEODR5 |
Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux11err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux11err |
vmcDetection |
VMCDR1 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCDR2 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCDR3 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCDR4 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCDR5 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vvvDetection |
VVVDR1 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vvvDetection |
VVVDR2 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux11err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 12 (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12} 10 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux12 |
vhsDetection |
VHSDR2 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
vhsDetection |
VHSDR3 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSDR4 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSDR5 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSDR6 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20120926 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20130417 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20140409 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20150108 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20160114 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20160507 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20170630 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20180419 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20201209 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20231101 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection |
VHSv20240731 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
videoDetection |
VIDEODR2 |
default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
videoDetection |
VIDEODR3 |
default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
videoDetection |
VIDEODR4 |
default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
videoDetection |
VIDEODR5 |
default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
videoDetection |
VIDEOv20100513 |
default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
videoDetection |
VIDEOv20111208 |
default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
vikingDetection |
VIKINGDR2 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
vikingDetection |
VIKINGDR3 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vikingDetection |
VIKINGDR4 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 12 (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12} 10 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux12 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 12 (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12} 10 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux12 |
vmcDetection |
VMCDR1 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
vmcDetection |
VMCDR2 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCDR3 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCDR4 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCDR5 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20110909 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
vmcDetection |
VMCv20120126 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
vmcDetection |
VMCv20121128 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20130304 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20130805 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20140428 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20140903 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20150309 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20151218 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20160311 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20160822 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20170109 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20170411 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20171101 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20180702 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20181120 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20191212 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20210708 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20230816 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection |
VMCv20240226 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vvvDetection |
VVVDR1 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vvvDetection |
VVVDR2 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux12 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux12err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux12err |
vhsDetection |
VHSDR2 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSDR3 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSDR4 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSDR5 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSDR6 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
videoDetection |
VIDEODR2 |
Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
videoDetection |
VIDEODR3 |
Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
videoDetection |
VIDEODR4 |
Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
videoDetection |
VIDEODR5 |
Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux12err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux12err |
vmcDetection |
VMCDR1 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCDR2 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCDR3 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCDR4 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCDR5 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vvvDetection |
VVVDR1 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vvvDetection |
VVVDR2 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux12err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 13 (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13} 12 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux13 |
vhsDetection |
VHSDR2 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
vhsDetection |
VHSDR3 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSDR4 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSDR5 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSDR6 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20120926 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20130417 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20140409 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20150108 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20160114 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20160507 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20170630 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20180419 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20201209 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20231101 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection |
VHSv20240731 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
videoDetection |
VIDEODR2 |
default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
videoDetection |
VIDEODR3 |
default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
videoDetection |
VIDEODR4 |
default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
videoDetection |
VIDEODR5 |
default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
videoDetection |
VIDEOv20100513 |
default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
videoDetection |
VIDEOv20111208 |
default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
vikingDetection |
VIKINGDR2 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
vikingDetection |
VIKINGDR3 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vikingDetection |
VIKINGDR4 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 13 (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13} 12 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux13 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 13 (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13} 12 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux13 |
vmcDetection |
VMCDR1 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
vmcDetection |
VMCDR2 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCDR3 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCDR4 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCDR5 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20110909 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
vmcDetection |
VMCv20120126 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
vmcDetection |
VMCv20121128 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20130304 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20130805 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20140428 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20140903 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20150309 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20151218 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20160311 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20160822 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20170109 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20170411 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20171101 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20180702 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20181120 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20191212 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20210708 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20230816 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection |
VMCv20240226 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vvvDetection |
VVVDR1 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vvvDetection |
VVVDR2 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux13 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux13err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux13err |
vhsDetection |
VHSDR2 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSDR3 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSDR4 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSDR5 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSDR6 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
videoDetection |
VIDEODR2 |
Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
videoDetection |
VIDEODR3 |
Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
videoDetection |
VIDEODR4 |
Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
videoDetection |
VIDEODR5 |
Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux13err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux13err |
vmcDetection |
VMCDR1 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCDR2 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCDR3 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCDR4 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCDR5 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vvvDetection |
VVVDR1 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vvvDetection |
VVVDR2 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux13err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux1err |
vhsDetection |
VHSDR2 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSDR3 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSDR4 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSDR5 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSDR6 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20120926 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20130417 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20140409 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20150108 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20160114 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20160507 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20170630 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20180419 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20201209 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20231101 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection |
VHSv20240731 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
videoDetection |
VIDEODR2 |
Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
videoDetection |
VIDEODR3 |
Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
videoDetection |
VIDEODR4 |
Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
videoDetection |
VIDEODR5 |
Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux1err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux1err |
vmcDetection |
VMCDR1 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCDR2 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCDR3 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCDR4 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCDR5 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20110909 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20120126 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20121128 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20130304 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20130805 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20140428 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20140903 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20150309 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20151218 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20160311 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20160822 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20170109 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20170411 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20171101 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20180702 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20181120 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20191212 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20210708 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20230816 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection |
VMCv20240226 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vvvDetection |
VVVDR1 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vvvDetection |
VVVDR2 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux1err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2 |
sharksDetection |
SHARKSv20210222 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
sharksDetection |
SHARKSv20210421 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
ultravistaDetection |
ULTRAVISTADR4 |
Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 2 (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSDR1 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
vhsDetection |
VHSDR2 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
vhsDetection |
VHSDR3 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSDR4 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSDR5 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSDR6 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20120926 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20130417 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20140409 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20150108 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20160114 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20160507 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20170630 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20180419 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20201209 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20231101 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsDetection |
VHSv20240731 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vhsListRemeasurement |
VHSDR1 |
default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux2 |
videoDetection |
VIDEODR2 |
Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
videoDetection |
VIDEODR3 |
Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
videoDetection |
VIDEODR4 |
Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
videoDetection |
VIDEODR5 |
Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
videoDetection |
VIDEOv20100513 |
Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
videoDetection |
VIDEOv20111208 |
Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux2 |
vikingDetection |
VIKINGDR2 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
vikingDetection |
VIKINGDR3 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vikingDetection |
VIKINGDR4 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vikingDetection |
VIKINGv20110714 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
vikingDetection |
VIKINGv20111019 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
vikingDetection |
VIKINGv20130417 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vikingDetection |
VIKINGv20140402 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vikingDetection |
VIKINGv20150421 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vikingDetection |
VIKINGv20151230 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vikingDetection |
VIKINGv20160406 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vikingDetection |
VIKINGv20161202 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vikingDetection |
VIKINGv20170715 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux2 |
vikingListRemeasurement |
VIKINGv20111019 |
default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux2 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 2 (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 2 (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCDR1 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
vmcDetection |
VMCDR2 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCDR3 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCDR4 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCDR5 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20110816 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
vmcDetection |
VMCv20110909 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
vmcDetection |
VMCv20120126 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
vmcDetection |
VMCv20121128 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20130304 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20130805 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20140428 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20140903 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20150309 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20151218 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20160311 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20160822 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20170109 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20170411 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20171101 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20180702 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20181120 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20191212 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20210708 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20230816 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcDetection |
VMCv20240226 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcListRemeasurement |
VMCv20110816 |
default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux2 |
vmcListRemeasurement |
VMCv20110909 |
default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux2 |
vmcdeepDetection |
VMCDEEPv20230713 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vmcdeepDetection |
VMCDEEPv20240506 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vvvDetection |
VVVDR1 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vvvDetection |
VVVDR2 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vvvDetection |
VVVv20100531 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count;em.opt |
aperFlux2 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
phot.count |
aperFlux2 |
vvvListRemeasurement |
VVVv20100531 |
default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux2 |
vvvListRemeasurement |
VVVv20110718 |
default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux2err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux2err |
vhsDetection |
VHSDR2 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSDR3 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSDR4 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSDR5 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSDR6 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
videoDetection |
VIDEODR2 |
Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
videoDetection |
VIDEODR3 |
Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
videoDetection |
VIDEODR4 |
Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
videoDetection |
VIDEODR5 |
Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux2err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux2err |
vmcDetection |
VMCDR1 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCDR2 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCDR3 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCDR4 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCDR5 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vvvDetection |
VVVDR1 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vvvDetection |
VVVDR2 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux2err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 3 (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. |
real |
4 |
ADU |
|
phot.count |
aperFlux3 |
vhsDetection |
VHSDR2 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
vhsDetection |
VHSDR3 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSDR4 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSDR5 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSDR6 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20120926 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20130417 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20140409 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20150108 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20160114 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20160507 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20170630 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20180419 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20201209 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20231101 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection |
VHSv20240731 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
videoDetection |
VIDEODR2 |
default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
videoDetection |
VIDEODR3 |
default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
videoDetection |
VIDEODR4 |
default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
videoDetection |
VIDEODR5 |
default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
videoDetection |
VIDEOv20100513 |
default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
videoDetection |
VIDEOv20111208 |
default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
vikingDetection |
VIKINGDR2 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
vikingDetection |
VIKINGDR3 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vikingDetection |
VIKINGDR4 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 3 (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. |
real |
4 |
ADU |
|
phot.count |
aperFlux3 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 3 (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. |
real |
4 |
ADU |
|
phot.count |
aperFlux3 |
vmcDetection |
VMCDR1 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
vmcDetection |
VMCDR2 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCDR3 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCDR4 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCDR5 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20110909 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
vmcDetection |
VMCv20120126 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
vmcDetection |
VMCv20121128 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20130304 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20130805 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20140428 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20140903 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20150309 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20151218 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20160311 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20160822 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20170109 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20170411 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20171101 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20180702 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20181120 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20191212 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20210708 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20230816 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection |
VMCv20240226 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vvvDetection |
VVVDR1 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vvvDetection |
VVVDR2 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux3 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux3err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux3err |
vhsDetection |
VHSDR2 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSDR3 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSDR4 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSDR5 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSDR6 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
videoDetection |
VIDEODR2 |
Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
videoDetection |
VIDEODR3 |
Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
videoDetection |
VIDEODR4 |
Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
videoDetection |
VIDEODR5 |
Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux3err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux3err |
vmcDetection |
VMCDR1 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCDR2 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCDR3 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCDR4 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCDR5 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vvvDetection |
VVVDR1 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vvvDetection |
VVVDR2 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux3err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 4 (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. |
real |
4 |
ADU |
|
phot.count |
aperFlux4 |
vhsDetection |
VHSDR2 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
vhsDetection |
VHSDR3 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSDR4 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSDR5 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSDR6 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20120926 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20130417 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20140409 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20150108 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20160114 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20160507 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20170630 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20180419 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20201209 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20231101 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection |
VHSv20240731 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
videoDetection |
VIDEODR2 |
default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
videoDetection |
VIDEODR3 |
default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
videoDetection |
VIDEODR4 |
default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
videoDetection |
VIDEODR5 |
default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
videoDetection |
VIDEOv20100513 |
default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
videoDetection |
VIDEOv20111208 |
default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
vikingDetection |
VIKINGDR2 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
vikingDetection |
VIKINGDR3 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vikingDetection |
VIKINGDR4 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 4 (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. |
real |
4 |
ADU |
|
phot.count |
aperFlux4 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 4 (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. |
real |
4 |
ADU |
|
phot.count |
aperFlux4 |
vmcDetection |
VMCDR1 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
vmcDetection |
VMCDR2 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCDR3 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCDR4 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCDR5 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20110909 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
vmcDetection |
VMCv20120126 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
vmcDetection |
VMCv20121128 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20130304 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20130805 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20140428 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20140903 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20150309 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20151218 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20160311 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20160822 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20170109 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20170411 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20171101 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20180702 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20181120 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20191212 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20210708 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20230816 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection |
VMCv20240226 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vvvDetection |
VVVDR1 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vvvDetection |
VVVDR2 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux4 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux4err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux4err |
vhsDetection |
VHSDR2 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSDR3 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSDR4 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSDR5 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSDR6 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
videoDetection |
VIDEODR2 |
Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
videoDetection |
VIDEODR3 |
Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
videoDetection |
VIDEODR4 |
Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
videoDetection |
VIDEODR5 |
Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux4err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux4err |
vmcDetection |
VMCDR1 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCDR2 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCDR3 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCDR4 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCDR5 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vvvDetection |
VVVDR1 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vvvDetection |
VVVDR2 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux4err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 5 (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5} 2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux5 |
vhsDetection |
VHSDR2 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
vhsDetection |
VHSDR3 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSDR4 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSDR5 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSDR6 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20120926 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20130417 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20140409 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20150108 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20160114 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20160507 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20170630 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20180419 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20201209 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20231101 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection |
VHSv20240731 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
videoDetection |
VIDEODR2 |
default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
videoDetection |
VIDEODR3 |
default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
videoDetection |
VIDEODR4 |
default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
videoDetection |
VIDEODR5 |
default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
videoDetection |
VIDEOv20100513 |
default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
videoDetection |
VIDEOv20111208 |
default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
vikingDetection |
VIKINGDR2 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
vikingDetection |
VIKINGDR3 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vikingDetection |
VIKINGDR4 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 5 (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5} 2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux5 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 5 (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5} 2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux5 |
vmcDetection |
VMCDR1 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
vmcDetection |
VMCDR2 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCDR3 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCDR4 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCDR5 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20110909 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
vmcDetection |
VMCv20120126 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
vmcDetection |
VMCv20121128 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20130304 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20130805 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20140428 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20140903 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20150309 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20151218 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20160311 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20160822 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20170109 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20170411 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20171101 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20180702 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20181120 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20191212 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20210708 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20230816 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection |
VMCv20240226 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vvvDetection |
VVVDR1 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vvvDetection |
VVVDR2 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux5 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux5err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux5err |
vhsDetection |
VHSDR2 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSDR3 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSDR4 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSDR5 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSDR6 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
videoDetection |
VIDEODR2 |
Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
videoDetection |
VIDEODR3 |
Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
videoDetection |
VIDEODR4 |
Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
videoDetection |
VIDEODR5 |
Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux5err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux5err |
vmcDetection |
VMCDR1 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCDR2 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCDR3 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCDR4 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCDR5 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vvvDetection |
VVVDR1 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vvvDetection |
VVVDR2 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux5err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 6 (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6} 2√2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux6 |
vhsDetection |
VHSDR2 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
vhsDetection |
VHSDR3 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSDR4 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSDR5 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSDR6 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20120926 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20130417 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20140409 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20150108 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20160114 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20160507 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20170630 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20180419 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20201209 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20231101 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection |
VHSv20240731 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
videoDetection |
VIDEODR2 |
default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
videoDetection |
VIDEODR3 |
default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
videoDetection |
VIDEODR4 |
default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
videoDetection |
VIDEODR5 |
default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
videoDetection |
VIDEOv20100513 |
default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
videoDetection |
VIDEOv20111208 |
default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
vikingDetection |
VIKINGDR2 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
vikingDetection |
VIKINGDR3 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vikingDetection |
VIKINGDR4 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 6 (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6} 2√2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux6 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 6 (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6} 2√2 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux6 |
vmcDetection |
VMCDR1 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
vmcDetection |
VMCDR2 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCDR3 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCDR4 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCDR5 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20110909 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
vmcDetection |
VMCv20120126 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
vmcDetection |
VMCv20121128 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20130304 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20130805 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20140428 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20140903 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20150309 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20151218 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20160311 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20160822 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20170109 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20170411 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20171101 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20180702 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20181120 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20191212 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20210708 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20230816 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection |
VMCv20240226 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vvvDetection |
VVVDR1 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vvvDetection |
VVVDR2 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux6 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux6err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux6err |
vhsDetection |
VHSDR2 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSDR3 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSDR4 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSDR5 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSDR6 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
videoDetection |
VIDEODR2 |
Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
videoDetection |
VIDEODR3 |
Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
videoDetection |
VIDEODR4 |
Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
videoDetection |
VIDEODR5 |
Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux6err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux6err |
vmcDetection |
VMCDR1 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCDR2 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCDR3 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCDR4 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCDR5 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vvvDetection |
VVVDR1 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vvvDetection |
VVVDR2 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux6err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 7 (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7} 4 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux7 |
vhsDetection |
VHSDR2 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
vhsDetection |
VHSDR3 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSDR4 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSDR5 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSDR6 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20120926 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20130417 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20140409 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20150108 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20160114 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20160507 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20170630 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20180419 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20201209 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20231101 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection |
VHSv20240731 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
videoDetection |
VIDEODR2 |
default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
videoDetection |
VIDEODR3 |
default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
videoDetection |
VIDEODR4 |
default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
videoDetection |
VIDEODR5 |
default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
videoDetection |
VIDEOv20100513 |
default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
videoDetection |
VIDEOv20111208 |
default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
vikingDetection |
VIKINGDR2 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
vikingDetection |
VIKINGDR3 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vikingDetection |
VIKINGDR4 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 7 (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7} 4 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux7 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 7 (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7} 4 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux7 |
vmcDetection |
VMCDR1 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
vmcDetection |
VMCDR2 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCDR3 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCDR4 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCDR5 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20110909 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
vmcDetection |
VMCv20120126 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
vmcDetection |
VMCv20121128 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20130304 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20130805 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20140428 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20140903 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20150309 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20151218 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20160311 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20160822 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20170109 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20170411 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20171101 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20180702 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20181120 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20191212 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20210708 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20230816 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection |
VMCv20240226 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vvvDetection |
VVVDR1 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vvvDetection |
VVVDR2 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux7 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux7err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux7err |
vhsDetection |
VHSDR2 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSDR3 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSDR4 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSDR5 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSDR6 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
videoDetection |
VIDEODR2 |
Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
videoDetection |
VIDEODR3 |
Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
videoDetection |
VIDEODR4 |
Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
videoDetection |
VIDEODR5 |
Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux7err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux7err |
vmcDetection |
VMCDR1 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCDR2 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCDR3 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCDR4 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCDR5 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vvvDetection |
VVVDR1 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vvvDetection |
VVVDR2 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux7err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 8 (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8} 5 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux8 |
vhsDetection |
VHSDR2 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
vhsDetection |
VHSDR3 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSDR4 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSDR5 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSDR6 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20120926 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20130417 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20140409 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20150108 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20160114 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20160507 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20170630 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20180419 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20201209 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20231101 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection |
VHSv20240731 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
videoDetection |
VIDEODR2 |
default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
videoDetection |
VIDEODR3 |
default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
videoDetection |
VIDEODR4 |
default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
videoDetection |
VIDEODR5 |
default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
videoDetection |
VIDEOv20100513 |
default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
videoDetection |
VIDEOv20111208 |
default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
vikingDetection |
VIKINGDR2 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
vikingDetection |
VIKINGDR3 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vikingDetection |
VIKINGDR4 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 8 (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8} 5 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux8 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 8 (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8} 5 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux8 |
vmcDetection |
VMCDR1 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
vmcDetection |
VMCDR2 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCDR3 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCDR4 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCDR5 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20110909 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
vmcDetection |
VMCv20120126 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
vmcDetection |
VMCv20121128 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20130304 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20130805 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20140428 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20140903 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20150309 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20151218 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20160311 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20160822 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20170109 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20170411 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20171101 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20180702 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20181120 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20191212 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20210708 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20230816 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection |
VMCv20240226 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vvvDetection |
VVVDR1 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vvvDetection |
VVVDR2 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux8 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux8err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux8err |
vhsDetection |
VHSDR2 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSDR3 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSDR4 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSDR5 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSDR6 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
videoDetection |
VIDEODR2 |
Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
videoDetection |
VIDEODR3 |
Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
videoDetection |
VIDEODR4 |
Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
videoDetection |
VIDEODR5 |
Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux8err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux8err |
vmcDetection |
VMCDR1 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCDR2 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCDR3 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCDR4 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCDR5 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vvvDetection |
VVVDR1 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vvvDetection |
VVVDR2 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux8err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9 |
sharksDetection |
SHARKSv20210222 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
sharksDetection |
SHARKSv20210421 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
ultravistaDetection |
ULTRAVISTADR4 |
default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Default aperture flux 9 (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9} 6 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux9 |
vhsDetection |
VHSDR2 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
vhsDetection |
VHSDR3 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSDR4 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSDR5 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSDR6 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20120926 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20130417 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20140409 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20150108 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20160114 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20160507 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20170630 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20180419 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20201209 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20231101 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection |
VHSv20240731 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
videoDetection |
VIDEODR2 |
default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
videoDetection |
VIDEODR3 |
default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
videoDetection |
VIDEODR4 |
default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
videoDetection |
VIDEODR5 |
default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
videoDetection |
VIDEOv20100513 |
default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
videoDetection |
VIDEOv20111208 |
default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
videoListRemeasurement |
VIDEOv20100513 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
vikingDetection |
VIKINGDR2 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
vikingDetection |
VIKINGDR3 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vikingDetection |
VIKINGDR4 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vikingDetection |
VIKINGv20111019 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
vikingDetection |
VIKINGv20130417 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vikingDetection |
VIKINGv20140402 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vikingDetection |
VIKINGv20150421 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vikingDetection |
VIKINGv20151230 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vikingDetection |
VIKINGv20160406 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vikingDetection |
VIKINGv20161202 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vikingDetection |
VIKINGv20170715 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Default aperture flux 9 (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9} 6 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux9 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Default aperture flux 9 (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9} 6 × rcore |
real |
4 |
ADU |
|
phot.count |
aperFlux9 |
vmcDetection |
VMCDR1 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
vmcDetection |
VMCDR2 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCDR3 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCDR4 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCDR5 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20110909 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
vmcDetection |
VMCv20120126 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
vmcDetection |
VMCv20121128 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20130304 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20130805 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20140428 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20140903 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20150309 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20151218 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20160311 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20160822 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20170109 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20170411 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20171101 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20180702 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20181120 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20191212 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20210708 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20230816 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection |
VMCv20240226 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9 |
vmcdeepDetection |
VMCDEEPv20230713 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vmcdeepDetection |
VMCDEEPv20240506 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vvvDetection |
VVVDR1 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vvvDetection |
VVVDR2 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count |
aperFlux9 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
aperture |
phot.count;em.opt |
aperFlux9err |
sharksDetection |
SHARKSv20210222 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
sharksDetection |
SHARKSv20210421 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux9err |
vhsDetection |
VHSDR2 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSDR3 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSDR4 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSDR5 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSDR6 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20120926 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20130417 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20140409 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20150108 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20160114 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20160507 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20170630 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20180419 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20201209 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20231101 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection |
VHSv20240731 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
videoDetection |
VIDEODR2 |
Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
videoDetection |
VIDEODR3 |
Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
videoDetection |
VIDEODR4 |
Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
videoDetection |
VIDEODR5 |
Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
videoDetection |
VIDEOv20100513 |
Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
videoDetection |
VIDEOv20111208 |
Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
videoListRemeasurement |
VIDEOv20100513 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGDR2 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGDR3 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGDR4 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGv20111019 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGv20130417 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGv20140402 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGv20150421 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGv20151230 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGv20160406 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGv20161202 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection |
VIKINGv20170715 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux9err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error;phot.count |
aperFlux9err |
vmcDetection |
VMCDR1 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCDR2 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCDR3 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCDR4 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCDR5 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20110909 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20120126 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20121128 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20130304 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20130805 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20140428 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20140903 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20150309 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20151218 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20160311 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20160822 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20170109 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20170411 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20171101 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20180702 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20181120 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20191212 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20210708 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20230816 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection |
VMCv20240226 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vvvDetection |
VVVDR1 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vvvDetection |
VVVDR2 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperFlux9err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
stat.error |
aperJky1 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 1 |
real |
4 |
jansky |
|
phot.jansky |
aperJky1 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 1 |
real |
4 |
jansky |
|
phot.flux |
aperJky1 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 1 |
real |
4 |
jansky |
|
phot.mag |
aperJky1 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 1 |
real |
4 |
jansky |
|
phot.mag |
aperJky1 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 1 |
real |
4 |
jansky |
|
phot.mag |
aperJky1 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 1 |
real |
4 |
jansky |
|
phot.mag |
aperJky10 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 10 |
real |
4 |
jansky |
|
phot.jansky |
aperJky10 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 10 |
real |
4 |
jansky |
|
phot.flux |
aperJky10 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 10 |
real |
4 |
jansky |
|
phot.mag |
aperJky10 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 10 |
real |
4 |
jansky |
|
phot.mag |
aperJky10 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 10 |
real |
4 |
jansky |
|
phot.mag |
aperJky10 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 10 |
real |
4 |
jansky |
|
phot.mag |
aperJky10err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 10 |
real |
4 |
jansky |
|
stat.error |
aperJky10err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 10 |
real |
4 |
jansky |
|
stat.error |
aperJky10err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 10 |
real |
4 |
jansky |
|
stat.error |
aperJky10err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 10 |
real |
4 |
jansky |
|
stat.error |
aperJky10err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 10 |
real |
4 |
jansky |
|
stat.error |
aperJky10err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 10 |
real |
4 |
jansky |
|
stat.error |
aperJky11 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 11 |
real |
4 |
jansky |
|
phot.jansky |
aperJky11 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 11 |
real |
4 |
jansky |
|
phot.flux |
aperJky11 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 11 |
real |
4 |
jansky |
|
phot.mag |
aperJky11 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 11 |
real |
4 |
jansky |
|
phot.mag |
aperJky11 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 11 |
real |
4 |
jansky |
|
phot.mag |
aperJky11 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 11 |
real |
4 |
jansky |
|
phot.mag |
aperJky11err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 11 |
real |
4 |
jansky |
|
stat.error |
aperJky11err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 11 |
real |
4 |
jansky |
|
stat.error |
aperJky11err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 11 |
real |
4 |
jansky |
|
stat.error |
aperJky11err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 11 |
real |
4 |
jansky |
|
stat.error |
aperJky11err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 11 |
real |
4 |
jansky |
|
stat.error |
aperJky11err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 11 |
real |
4 |
jansky |
|
stat.error |
aperJky12 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 12 |
real |
4 |
jansky |
|
phot.jansky |
aperJky12 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 12 |
real |
4 |
jansky |
|
phot.flux |
aperJky12 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 12 |
real |
4 |
jansky |
|
phot.mag |
aperJky12 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 12 |
real |
4 |
jansky |
|
phot.mag |
aperJky12 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 12 |
real |
4 |
jansky |
|
phot.mag |
aperJky12 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 12 |
real |
4 |
jansky |
|
phot.mag |
aperJky12err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 12 |
real |
4 |
jansky |
|
stat.error |
aperJky12err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 12 |
real |
4 |
jansky |
|
stat.error |
aperJky12err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 12 |
real |
4 |
jansky |
|
stat.error |
aperJky12err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 12 |
real |
4 |
jansky |
|
stat.error |
aperJky12err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 12 |
real |
4 |
jansky |
|
stat.error |
aperJky12err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 12 |
real |
4 |
jansky |
|
stat.error |
aperJky13 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 13 |
real |
4 |
jansky |
|
phot.jansky |
aperJky13 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 13 |
real |
4 |
jansky |
|
phot.flux |
aperJky13 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 13 |
real |
4 |
jansky |
|
phot.mag |
aperJky13 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 13 |
real |
4 |
jansky |
|
phot.mag |
aperJky13 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 13 |
real |
4 |
jansky |
|
phot.mag |
aperJky13 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 13 |
real |
4 |
jansky |
|
phot.mag |
aperJky13err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 13 |
real |
4 |
jansky |
|
stat.error |
aperJky13err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 13 |
real |
4 |
jansky |
|
stat.error |
aperJky13err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 13 |
real |
4 |
jansky |
|
stat.error |
aperJky13err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 13 |
real |
4 |
jansky |
|
stat.error |
aperJky13err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 13 |
real |
4 |
jansky |
|
stat.error |
aperJky13err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 13 |
real |
4 |
jansky |
|
stat.error |
aperJky1err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 1 |
real |
4 |
jansky |
|
stat.error |
aperJky1err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 1 |
real |
4 |
jansky |
|
stat.error |
aperJky1err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 1 |
real |
4 |
jansky |
|
stat.error |
aperJky1err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 1 |
real |
4 |
jansky |
|
stat.error |
aperJky1err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 1 |
real |
4 |
jansky |
|
stat.error |
aperJky1err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 1 |
real |
4 |
jansky |
|
stat.error |
aperJky2 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 2 |
real |
4 |
jansky |
|
phot.jansky |
aperJky2 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 2 |
real |
4 |
jansky |
|
phot.flux |
aperJky2 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 2 |
real |
4 |
jansky |
|
phot.mag |
aperJky2 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 2 |
real |
4 |
jansky |
|
phot.mag |
aperJky2 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 2 |
real |
4 |
jansky |
|
phot.mag |
aperJky2 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 2 |
real |
4 |
jansky |
|
phot.mag |
aperJky2err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 2 |
real |
4 |
jansky |
|
stat.error |
aperJky2err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 2 |
real |
4 |
jansky |
|
stat.error |
aperJky2err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 2 |
real |
4 |
jansky |
|
stat.error |
aperJky2err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 2 |
real |
4 |
jansky |
|
stat.error |
aperJky2err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 2 |
real |
4 |
jansky |
|
stat.error |
aperJky2err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 2 |
real |
4 |
jansky |
|
stat.error |
aperJky3 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 3 |
real |
4 |
jansky |
|
phot.jansky |
aperJky3 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 3 |
real |
4 |
jansky |
|
phot.flux |
aperJky3 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 3 |
real |
4 |
jansky |
|
phot.mag |
aperJky3 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 3 |
real |
4 |
jansky |
|
phot.mag |
aperJky3 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 3 |
real |
4 |
jansky |
|
phot.mag |
aperJky3 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 3 |
real |
4 |
jansky |
|
phot.mag |
aperJky3err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 3 |
real |
4 |
jansky |
|
stat.error |
aperJky3err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 3 |
real |
4 |
jansky |
|
stat.error |
aperJky3err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 3 |
real |
4 |
jansky |
|
stat.error |
aperJky3err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 3 |
real |
4 |
jansky |
|
stat.error |
aperJky3err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 3 |
real |
4 |
jansky |
|
stat.error |
aperJky3err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 3 |
real |
4 |
jansky |
|
stat.error |
aperJky4 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 4 |
real |
4 |
jansky |
|
phot.jansky |
aperJky4 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 4 |
real |
4 |
jansky |
|
phot.flux |
aperJky4 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 4 |
real |
4 |
jansky |
|
phot.mag |
aperJky4 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 4 |
real |
4 |
jansky |
|
phot.mag |
aperJky4 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 4 |
real |
4 |
jansky |
|
phot.mag |
aperJky4 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 4 |
real |
4 |
jansky |
|
phot.mag |
aperJky4err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 4 |
real |
4 |
jansky |
|
stat.error |
aperJky4err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 4 |
real |
4 |
jansky |
|
stat.error |
aperJky4err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 4 |
real |
4 |
jansky |
|
stat.error |
aperJky4err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 4 |
real |
4 |
jansky |
|
stat.error |
aperJky4err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 4 |
real |
4 |
jansky |
|
stat.error |
aperJky4err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 4 |
real |
4 |
jansky |
|
stat.error |
aperJky5 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 5 |
real |
4 |
jansky |
|
phot.jansky |
aperJky5 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 5 |
real |
4 |
jansky |
|
phot.flux |
aperJky5 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 5 |
real |
4 |
jansky |
|
phot.mag |
aperJky5 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 5 |
real |
4 |
jansky |
|
phot.mag |
aperJky5 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 5 |
real |
4 |
jansky |
|
phot.mag |
aperJky5 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 5 |
real |
4 |
jansky |
|
phot.mag |
aperJky5err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 5 |
real |
4 |
jansky |
|
stat.error |
aperJky5err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 5 |
real |
4 |
jansky |
|
stat.error |
aperJky5err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 5 |
real |
4 |
jansky |
|
stat.error |
aperJky5err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 5 |
real |
4 |
jansky |
|
stat.error |
aperJky5err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 5 |
real |
4 |
jansky |
|
stat.error |
aperJky5err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 5 |
real |
4 |
jansky |
|
stat.error |
aperJky6 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 6 |
real |
4 |
jansky |
|
phot.jansky |
aperJky6 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 6 |
real |
4 |
jansky |
|
phot.flux |
aperJky6 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 6 |
real |
4 |
jansky |
|
phot.mag |
aperJky6 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 6 |
real |
4 |
jansky |
|
phot.mag |
aperJky6 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 6 |
real |
4 |
jansky |
|
phot.mag |
aperJky6 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 6 |
real |
4 |
jansky |
|
phot.mag |
aperJky6err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 6 |
real |
4 |
jansky |
|
stat.error |
aperJky6err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 6 |
real |
4 |
jansky |
|
stat.error |
aperJky6err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 6 |
real |
4 |
jansky |
|
stat.error |
aperJky6err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 6 |
real |
4 |
jansky |
|
stat.error |
aperJky6err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 6 |
real |
4 |
jansky |
|
stat.error |
aperJky6err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 6 |
real |
4 |
jansky |
|
stat.error |
aperJky7 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 7 |
real |
4 |
jansky |
|
phot.jansky |
aperJky7 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 7 |
real |
4 |
jansky |
|
phot.flux |
aperJky7 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 7 |
real |
4 |
jansky |
|
phot.mag |
aperJky7 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 7 |
real |
4 |
jansky |
|
phot.mag |
aperJky7 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 7 |
real |
4 |
jansky |
|
phot.mag |
aperJky7 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 7 |
real |
4 |
jansky |
|
phot.mag |
aperJky7err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 7 |
real |
4 |
jansky |
|
stat.error |
aperJky7err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 7 |
real |
4 |
jansky |
|
stat.error |
aperJky7err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 7 |
real |
4 |
jansky |
|
stat.error |
aperJky7err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 7 |
real |
4 |
jansky |
|
stat.error |
aperJky7err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 7 |
real |
4 |
jansky |
|
stat.error |
aperJky7err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 7 |
real |
4 |
jansky |
|
stat.error |
aperJky8 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 8 |
real |
4 |
jansky |
|
phot.jansky |
aperJky8 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 8 |
real |
4 |
jansky |
|
phot.flux |
aperJky8 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 8 |
real |
4 |
jansky |
|
phot.mag |
aperJky8 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 8 |
real |
4 |
jansky |
|
phot.mag |
aperJky8 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 8 |
real |
4 |
jansky |
|
phot.mag |
aperJky8 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 8 |
real |
4 |
jansky |
|
phot.mag |
aperJky8err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 8 |
real |
4 |
jansky |
|
stat.error |
aperJky8err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 8 |
real |
4 |
jansky |
|
stat.error |
aperJky8err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 8 |
real |
4 |
jansky |
|
stat.error |
aperJky8err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 8 |
real |
4 |
jansky |
|
stat.error |
aperJky8err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 8 |
real |
4 |
jansky |
|
stat.error |
aperJky8err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 8 |
real |
4 |
jansky |
|
stat.error |
aperJky9 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and corrected aperture flux 9 |
real |
4 |
jansky |
|
phot.jansky |
aperJky9 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture flux 9 |
real |
4 |
jansky |
|
phot.flux |
aperJky9 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and corrected aperture flux 9 |
real |
4 |
jansky |
|
phot.mag |
aperJky9 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and corrected aperture flux 9 |
real |
4 |
jansky |
|
phot.mag |
aperJky9 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture flux 9 |
real |
4 |
jansky |
|
phot.mag |
aperJky9 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture flux 9 |
real |
4 |
jansky |
|
phot.mag |
aperJky9err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged calibrated aperture flux 9 |
real |
4 |
jansky |
|
stat.error |
aperJky9err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture flux 9 |
real |
4 |
jansky |
|
stat.error |
aperJky9err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged calibrated aperture flux 9 |
real |
4 |
jansky |
|
stat.error |
aperJky9err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged calibrated aperture flux 9 |
real |
4 |
jansky |
|
stat.error |
aperJky9err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture flux 9 |
real |
4 |
jansky |
|
stat.error |
aperJky9err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture flux 9 |
real |
4 |
jansky |
|
stat.error |
aperJkyNoAperCorr1 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 1 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr1 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 1 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr1 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 1 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr1 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 1 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr1 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 1 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr1 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 1 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr2 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 2 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr2 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 2 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr2 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 2 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr2 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 2 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr2 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 2 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr2 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 2 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr3 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 3 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr3 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 3 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr3 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 3 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr3 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 3 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr3 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 3 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr3 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 3 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr4 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 4 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr4 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 4 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr4 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 4 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr4 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 4 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr4 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 4 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr4 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 4 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr5 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 5 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr5 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 5 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr5 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 5 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr5 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 5 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr5 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 5 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr5 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 5 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr6 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 6 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr6 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 6 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr6 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 6 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr6 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 6 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr6 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 6 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr6 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 6 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr7 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 7 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr7 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 7 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr7 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 7 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr7 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Calibrated and standard corrected (but no aperture correction applied) aperture flux 7 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr7 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 7 |
real |
4 |
jansky |
|
phot.mag |
aperJkyNoAperCorr7 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture flux 7 |
real |
4 |
jansky |
|
phot.mag |
aperLup1 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLup1 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLup1 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLup1 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLup1 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLup1 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLup10 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 10 |
real |
4 |
lup |
|
phot.mag |
aperLup10 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 10 |
real |
4 |
lup |
|
phot.mag |
aperLup10 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 10 |
real |
4 |
lup |
|
phot.mag |
aperLup10 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 10 |
real |
4 |
lup |
|
phot.mag |
aperLup10 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 10 |
real |
4 |
lup |
|
phot.mag |
aperLup10 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 10 |
real |
4 |
lup |
|
phot.mag |
aperLup10err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 10 |
real |
4 |
lup |
|
stat.error |
aperLup10err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 10 |
real |
4 |
lup |
|
stat.error |
aperLup10err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 10 |
real |
4 |
lup |
|
stat.error |
aperLup10err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 10 |
real |
4 |
lup |
|
stat.error |
aperLup10err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 10 |
real |
4 |
lup |
|
stat.error |
aperLup10err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 10 |
real |
4 |
lup |
|
stat.error |
aperLup11 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 11 |
real |
4 |
lup |
|
phot.mag |
aperLup11 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 11 |
real |
4 |
lup |
|
phot.mag |
aperLup11 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 11 |
real |
4 |
lup |
|
phot.mag |
aperLup11 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 11 |
real |
4 |
lup |
|
phot.mag |
aperLup11 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 11 |
real |
4 |
lup |
|
phot.mag |
aperLup11 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 11 |
real |
4 |
lup |
|
phot.mag |
aperLup11err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 11 |
real |
4 |
lup |
|
stat.error |
aperLup11err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 11 |
real |
4 |
lup |
|
stat.error |
aperLup11err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 11 |
real |
4 |
lup |
|
stat.error |
aperLup11err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 11 |
real |
4 |
lup |
|
stat.error |
aperLup11err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 11 |
real |
4 |
lup |
|
stat.error |
aperLup11err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 11 |
real |
4 |
lup |
|
stat.error |
aperLup12 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 12 |
real |
4 |
lup |
|
phot.mag |
aperLup12 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 12 |
real |
4 |
lup |
|
phot.mag |
aperLup12 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 12 |
real |
4 |
lup |
|
phot.mag |
aperLup12 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 12 |
real |
4 |
lup |
|
phot.mag |
aperLup12 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 12 |
real |
4 |
lup |
|
phot.mag |
aperLup12 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 12 |
real |
4 |
lup |
|
phot.mag |
aperLup12err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 12 |
real |
4 |
lup |
|
stat.error |
aperLup12err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 12 |
real |
4 |
lup |
|
stat.error |
aperLup12err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 12 |
real |
4 |
lup |
|
stat.error |
aperLup12err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 12 |
real |
4 |
lup |
|
stat.error |
aperLup12err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 12 |
real |
4 |
lup |
|
stat.error |
aperLup12err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 12 |
real |
4 |
lup |
|
stat.error |
aperLup13 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 13 |
real |
4 |
lup |
|
phot.mag |
aperLup13 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 13 |
real |
4 |
lup |
|
phot.mag |
aperLup13 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 13 |
real |
4 |
lup |
|
phot.mag |
aperLup13 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 13 |
real |
4 |
lup |
|
phot.mag |
aperLup13 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 13 |
real |
4 |
lup |
|
phot.mag |
aperLup13 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 13 |
real |
4 |
lup |
|
phot.mag |
aperLup13err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 13 |
real |
4 |
lup |
|
stat.error |
aperLup13err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 13 |
real |
4 |
lup |
|
stat.error |
aperLup13err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 13 |
real |
4 |
lup |
|
stat.error |
aperLup13err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 13 |
real |
4 |
lup |
|
stat.error |
aperLup13err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 13 |
real |
4 |
lup |
|
stat.error |
aperLup13err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 13 |
real |
4 |
lup |
|
stat.error |
aperLup1err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 1 |
real |
4 |
lup |
|
stat.error |
aperLup1err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 1 |
real |
4 |
lup |
|
stat.error |
aperLup1err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 1 |
real |
4 |
lup |
|
stat.error |
aperLup1err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 1 |
real |
4 |
lup |
|
stat.error |
aperLup1err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 1 |
real |
4 |
lup |
|
stat.error |
aperLup1err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 1 |
real |
4 |
lup |
|
stat.error |
aperLup2 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLup2 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLup2 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLup2 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLup2 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLup2 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLup2err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 2 |
real |
4 |
lup |
|
stat.error |
aperLup2err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 2 |
real |
4 |
lup |
|
stat.error |
aperLup2err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 2 |
real |
4 |
lup |
|
stat.error |
aperLup2err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 2 |
real |
4 |
lup |
|
stat.error |
aperLup2err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 2 |
real |
4 |
lup |
|
stat.error |
aperLup2err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 2 |
real |
4 |
lup |
|
stat.error |
aperLup3 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLup3 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLup3 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLup3 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLup3 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLup3 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLup3err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 3 |
real |
4 |
lup |
|
stat.error |
aperLup3err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 3 |
real |
4 |
lup |
|
stat.error |
aperLup3err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 3 |
real |
4 |
lup |
|
stat.error |
aperLup3err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 3 |
real |
4 |
lup |
|
stat.error |
aperLup3err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 3 |
real |
4 |
lup |
|
stat.error |
aperLup3err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 3 |
real |
4 |
lup |
|
stat.error |
aperLup4 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLup4 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLup4 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLup4 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLup4 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLup4 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLup4err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 4 |
real |
4 |
lup |
|
stat.error |
aperLup4err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 4 |
real |
4 |
lup |
|
stat.error |
aperLup4err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 4 |
real |
4 |
lup |
|
stat.error |
aperLup4err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 4 |
real |
4 |
lup |
|
stat.error |
aperLup4err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 4 |
real |
4 |
lup |
|
stat.error |
aperLup4err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 4 |
real |
4 |
lup |
|
stat.error |
aperLup5 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLup5 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLup5 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLup5 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLup5 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLup5 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLup5err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 5 |
real |
4 |
lup |
|
stat.error |
aperLup5err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 5 |
real |
4 |
lup |
|
stat.error |
aperLup5err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 5 |
real |
4 |
lup |
|
stat.error |
aperLup5err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 5 |
real |
4 |
lup |
|
stat.error |
aperLup5err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 5 |
real |
4 |
lup |
|
stat.error |
aperLup5err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 5 |
real |
4 |
lup |
|
stat.error |
aperLup6 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLup6 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLup6 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLup6 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLup6 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLup6 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLup6err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 6 |
real |
4 |
lup |
|
stat.error |
aperLup6err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 6 |
real |
4 |
lup |
|
stat.error |
aperLup6err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 6 |
real |
4 |
lup |
|
stat.error |
aperLup6err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 6 |
real |
4 |
lup |
|
stat.error |
aperLup6err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 6 |
real |
4 |
lup |
|
stat.error |
aperLup6err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 6 |
real |
4 |
lup |
|
stat.error |
aperLup7 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLup7 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLup7 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLup7 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLup7 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLup7 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLup7err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 7 |
real |
4 |
lup |
|
stat.error |
aperLup7err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 7 |
real |
4 |
lup |
|
stat.error |
aperLup7err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 7 |
real |
4 |
lup |
|
stat.error |
aperLup7err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 7 |
real |
4 |
lup |
|
stat.error |
aperLup7err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 7 |
real |
4 |
lup |
|
stat.error |
aperLup7err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 7 |
real |
4 |
lup |
|
stat.error |
aperLup8 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 8 |
real |
4 |
lup |
|
phot.mag |
aperLup8 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 8 |
real |
4 |
lup |
|
phot.mag |
aperLup8 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 8 |
real |
4 |
lup |
|
phot.mag |
aperLup8 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 8 |
real |
4 |
lup |
|
phot.mag |
aperLup8 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 8 |
real |
4 |
lup |
|
phot.mag |
aperLup8 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 8 |
real |
4 |
lup |
|
phot.mag |
aperLup8err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 8 |
real |
4 |
lup |
|
stat.error |
aperLup8err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 8 |
real |
4 |
lup |
|
stat.error |
aperLup8err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 8 |
real |
4 |
lup |
|
stat.error |
aperLup8err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 8 |
real |
4 |
lup |
|
stat.error |
aperLup8err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 8 |
real |
4 |
lup |
|
stat.error |
aperLup8err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 8 |
real |
4 |
lup |
|
stat.error |
aperLup9 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture luptitude 9 |
real |
4 |
lup |
|
phot.mag |
aperLup9 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture luptitude 9 |
real |
4 |
lup |
|
phot.mag |
aperLup9 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture luptitude 9 |
real |
4 |
lup |
|
phot.mag |
aperLup9 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture luptitude 9 |
real |
4 |
lup |
|
phot.mag |
aperLup9 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture luptitude 9 |
real |
4 |
lup |
|
phot.mag |
aperLup9 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture luptitude 9 |
real |
4 |
lup |
|
phot.mag |
aperLup9err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture luptitude 9 |
real |
4 |
lup |
|
stat.error |
aperLup9err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture luptitude 9 |
real |
4 |
lup |
|
stat.error |
aperLup9err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture luptitude 9 |
real |
4 |
lup |
|
stat.error |
aperLup9err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture luptitude 9 |
real |
4 |
lup |
|
stat.error |
aperLup9err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture luptitude 9 |
real |
4 |
lup |
|
stat.error |
aperLup9err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture luptitude 9 |
real |
4 |
lup |
|
stat.error |
aperLupNoAperCorr1 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr1 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr1 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr1 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr1 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr1 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 1 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr2 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr2 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr2 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr2 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr2 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr2 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 2 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr3 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr3 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr3 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr3 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr3 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr3 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 3 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr4 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr4 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr4 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr4 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr4 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr4 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 4 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr5 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr5 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr5 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr5 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr5 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr5 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 5 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr6 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr6 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr6 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr6 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr6 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr6 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 6 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr7 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr7 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr7 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr7 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr7 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperLupNoAperCorr7 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture luptitude 7 |
real |
4 |
lup |
|
phot.mag |
aperMag1 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag1 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag1 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
phot.mag |
aperMag10err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag10err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag10err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
stat.error |
aperMag11 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
phot.mag |
aperMag11err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag11err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag11err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
stat.error |
aperMag12 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
phot.mag |
aperMag12err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag12err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag12err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
stat.error |
aperMag13 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
phot.mag |
aperMag13err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag13err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag13err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag1err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag1err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
stat.error |
aperMag2 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
aperMag2err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag2err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag2err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
stat.error |
aperMag3 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
aperMag3err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag3err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag3err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
stat.error |
aperMag4 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
aperMag4err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag4err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag4err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
stat.error |
aperMag5 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
aperMag5err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag5err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag5err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
stat.error |
aperMag6 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
aperMag6err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag6err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag6err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
stat.error |
aperMag7 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
aperMag7err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag7err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag7err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
stat.error |
aperMag8 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
phot.mag |
aperMag8err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag8err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag8err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
stat.error |
aperMag9 |
sharksDetection |
SHARKSv20210222 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
sharksDetection |
SHARKSv20210421 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
vhsDetection |
VHSDR1 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSDR2 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSDR3 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSDR4 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSDR5 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSDR6 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20120926 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20130417 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20140409 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20150108 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20160114 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20160507 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20170630 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20180419 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20201209 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20231101 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection |
VHSv20240731 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsListRemeasurement |
VHSDR1 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
videoDetection |
VIDEODR2 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
videoDetection |
VIDEODR3 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
videoDetection |
VIDEODR4 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
videoDetection |
VIDEODR5 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
videoDetection |
VIDEOv20111208 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
vikingDetection |
VIKINGDR2 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGDR3 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGDR4 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGv20130417 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGv20140402 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGv20150421 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGv20151230 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGv20160406 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGv20161202 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingDetection |
VIKINGv20170715 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vikingListRemeasurement |
VIKINGv20110714 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
vikingListRemeasurement |
VIKINGv20111019 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
vmcDetection |
VMCDR1 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCDR2 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCDR3 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCDR4 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCDR5 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20110816 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20110909 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20120126 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20121128 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20130304 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20130805 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20140428 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20140903 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20150309 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20151218 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20160311 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20160822 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20170109 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20170411 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20171101 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20180702 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20181120 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20191212 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20210708 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20230816 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcDetection |
VMCv20240226 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcListRemeasurement |
VMCv20110816 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
vmcListRemeasurement |
VMCv20110909 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vvvDetection |
VVVDR1 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vvvDetection |
VVVDR2 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
phot.mag |
aperMag9err |
sharksDetection |
SHARKSv20210222 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
sharksDetection |
SHARKSv20210421 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
ultravistaDetection |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived Error in averaged calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vhsDetection |
VHSDR2 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vhsDetection |
VHSDR3 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vhsDetection |
VHSDR4 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection |
VHSDR5 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection |
VHSDR6 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection |
VHSv20120926 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vhsDetection |
VHSv20130417 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vhsDetection |
VHSv20140409 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vhsDetection |
VHSv20150108 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection |
VHSv20160114 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection |
VHSv20160507 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection |
VHSv20170630 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection |
VHSv20180419 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection |
VHSv20201209 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection |
VHSv20231101 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection |
VHSv20240731 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
videoDetection |
VIDEODR2 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
videoDetection |
VIDEODR3 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
videoDetection |
VIDEODR4 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
videoDetection |
VIDEODR5 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
videoDetection |
VIDEOv20111208 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingDetection |
VIKINGDR2 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingDetection |
VIKINGDR3 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingDetection |
VIKINGDR4 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingDetection |
VIKINGv20111019 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingDetection |
VIKINGv20130417 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingDetection |
VIKINGv20140402 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingDetection |
VIKINGv20150421 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vikingDetection |
VIKINGv20151230 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vikingDetection |
VIKINGv20160406 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vikingDetection |
VIKINGv20161202 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vikingDetection |
VIKINGv20170715 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived Error in averaged calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived Error in averaged calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vmcDetection |
VMCDR1 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vmcDetection |
VMCDR2 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vmcDetection |
VMCDR3 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCDR4 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCDR5 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20110909 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vmcDetection |
VMCv20120126 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vmcDetection |
VMCv20121128 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vmcDetection |
VMCv20130304 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vmcDetection |
VMCv20130805 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vmcDetection |
VMCv20140428 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vmcDetection |
VMCv20140903 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20150309 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20151218 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20160311 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20160822 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20170109 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20170411 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20171101 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20180702 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20181120 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20191212 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20210708 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20230816 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection |
VMCv20240226 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vvvDetection |
VVVDR1 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vvvDetection |
VVVDR2 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMag9err |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error;phot.mag |
aperMag9err |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
stat.error |
aperMagNoAperCorr1 |
sharksDetection |
SHARKSv20210222 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
sharksDetection |
SHARKSv20210421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
ultravistaDetection |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1, calculated from aperJkyNoAperCorr1 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr1 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr1 |
vhsDetection |
VHSDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSDR6 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20120926 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20140409 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20150108 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20160114 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20160507 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20170630 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20180419 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20201209 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20231101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection |
VHSv20240731 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
videoDetection |
VIDEODR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
videoDetection |
VIDEODR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
videoDetection |
VIDEODR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
videoDetection |
VIDEODR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
videoDetection |
VIDEOv20111208 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGv20110714 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGv20111019 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGv20140402 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGv20150421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGv20151230 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGv20160406 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGv20161202 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingDetection |
VIKINGv20170715 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1, calculated from aperJkyNoAperCorr1 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr1 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1, calculated from aperJkyNoAperCorr1 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr1 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr1 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr1 |
vmcDetection |
VMCDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20110816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20110909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20120126 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20121128 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20130304 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20130805 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20140428 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20140903 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20150309 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20151218 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20160311 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20160822 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20170109 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20170411 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20171101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20180702 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20181120 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20191212 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20210708 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20230816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcDetection |
VMCv20240226 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vvvDetection |
VVVDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vvvDetection |
VVVDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
sharksDetection |
SHARKSv20210222 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
sharksDetection |
SHARKSv20210421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
ultravistaDetection |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2, calculated from aperJkyNoAperCorr2 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr2 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr2 |
vhsDetection |
VHSDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSDR6 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20120926 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20140409 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20150108 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20160114 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20160507 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20170630 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20180419 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20201209 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20231101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VHSv20240731 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
videoDetection |
VIDEODR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
videoDetection |
VIDEODR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
videoDetection |
VIDEODR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
videoDetection |
VIDEODR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
videoDetection |
VIDEOv20111208 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGv20110714 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGv20111019 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGv20140402 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGv20150421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGv20151230 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGv20160406 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGv20161202 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingDetection |
VIKINGv20170715 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2, calculated from aperJkyNoAperCorr2 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr2 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2, calculated from aperJkyNoAperCorr2 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr2 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr2 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 2 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr2 |
vmcDetection |
VMCDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20110816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20110909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20120126 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20121128 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20130304 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20130805 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20140428 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20140903 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20150309 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20151218 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20160311 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20160822 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20170109 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20170411 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20171101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20180702 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20181120 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20191212 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20210708 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20230816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcDetection |
VMCv20240226 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vvvDetection |
VVVDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vvvDetection |
VVVDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
sharksDetection |
SHARKSv20210222 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
sharksDetection |
SHARKSv20210421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
ultravistaDetection |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3, calculated from aperJkyNoAperCorr3 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr3 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr3 |
vhsDetection |
VHSDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSDR6 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20120926 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20140409 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20150108 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20160114 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20160507 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20170630 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20180419 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20201209 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20231101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VHSv20240731 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
videoDetection |
VIDEODR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
videoDetection |
VIDEODR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
videoDetection |
VIDEODR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
videoDetection |
VIDEODR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
videoDetection |
VIDEOv20111208 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGv20110714 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGv20111019 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGv20140402 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGv20150421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGv20151230 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGv20160406 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGv20161202 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingDetection |
VIKINGv20170715 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3, calculated from aperJkyNoAperCorr3 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr3 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3, calculated from aperJkyNoAperCorr3 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr3 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr3 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 3 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr3 |
vmcDetection |
VMCDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20110816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20110909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20120126 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20121128 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20130304 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20130805 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20140428 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20140903 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20150309 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20151218 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20160311 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20160822 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20170109 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20170411 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20171101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20180702 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20181120 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20191212 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20210708 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20230816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcDetection |
VMCv20240226 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vvvDetection |
VVVDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vvvDetection |
VVVDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
sharksDetection |
SHARKSv20210222 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
sharksDetection |
SHARKSv20210421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
ultravistaDetection |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4, calculated from aperJkyNoAperCorr4 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr4 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr4 |
vhsDetection |
VHSDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSDR6 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20120926 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20140409 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20150108 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20160114 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20160507 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20170630 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20180419 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20201209 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20231101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VHSv20240731 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
videoDetection |
VIDEODR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
videoDetection |
VIDEODR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
videoDetection |
VIDEODR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
videoDetection |
VIDEODR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
videoDetection |
VIDEOv20111208 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGv20110714 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGv20111019 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGv20140402 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGv20150421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGv20151230 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGv20160406 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGv20161202 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingDetection |
VIKINGv20170715 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4, calculated from aperJkyNoAperCorr4 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr4 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4, calculated from aperJkyNoAperCorr4 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr4 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr4 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 4 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr4 |
vmcDetection |
VMCDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20110816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20110909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20120126 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20121128 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20130304 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20130805 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20140428 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20140903 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20150309 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20151218 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20160311 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20160822 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20170109 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20170411 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20171101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20180702 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20181120 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20191212 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20210708 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20230816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcDetection |
VMCv20240226 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vvvDetection |
VVVDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vvvDetection |
VVVDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
sharksDetection |
SHARKSv20210222 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
sharksDetection |
SHARKSv20210421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
ultravistaDetection |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5, calculated from aperJkyNoAperCorr5 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr5 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr5 |
vhsDetection |
VHSDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSDR6 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20120926 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20140409 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20150108 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20160114 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20160507 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20170630 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20180419 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20201209 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20231101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VHSv20240731 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
videoDetection |
VIDEODR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
videoDetection |
VIDEODR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
videoDetection |
VIDEODR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
videoDetection |
VIDEODR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
videoDetection |
VIDEOv20111208 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGv20110714 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGv20111019 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGv20140402 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGv20150421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGv20151230 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGv20160406 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGv20161202 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingDetection |
VIKINGv20170715 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5, calculated from aperJkyNoAperCorr5 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr5 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5, calculated from aperJkyNoAperCorr5 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr5 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr5 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 5 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr5 |
vmcDetection |
VMCDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20110816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20110909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20120126 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20121128 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20130304 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20130805 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20140428 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20140903 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20150309 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20151218 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20160311 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20160822 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20170109 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20170411 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20171101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20180702 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20181120 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20191212 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20210708 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20230816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcDetection |
VMCv20240226 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vvvDetection |
VVVDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vvvDetection |
VVVDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
sharksDetection |
SHARKSv20210222 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
sharksDetection |
SHARKSv20210421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
ultravistaDetection |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6, calculated from aperJkyNoAperCorr6 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr6 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr6 |
vhsDetection |
VHSDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSDR6 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20120926 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20140409 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20150108 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20160114 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20160507 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20170630 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20180419 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20201209 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20231101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VHSv20240731 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
videoDetection |
VIDEODR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
videoDetection |
VIDEODR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
videoDetection |
VIDEODR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
videoDetection |
VIDEODR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
videoDetection |
VIDEOv20111208 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGv20110714 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGv20111019 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGv20140402 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGv20150421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGv20151230 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGv20160406 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGv20161202 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingDetection |
VIKINGv20170715 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6, calculated from aperJkyNoAperCorr6 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr6 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6, calculated from aperJkyNoAperCorr6 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr6 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr6 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 6 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr6 |
vmcDetection |
VMCDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20110816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20110909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20120126 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20121128 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20130304 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20130805 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20140428 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20140903 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20150309 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20151218 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20160311 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20160822 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20170109 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20170411 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20171101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20180702 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20181120 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20191212 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20210708 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20230816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcDetection |
VMCv20240226 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vvvDetection |
VVVDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vvvDetection |
VVVDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
sharksDetection |
SHARKSv20210222 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
sharksDetection |
SHARKSv20210421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
ultravistaDetection |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7, calculated from aperJkyNoAperCorr7 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr7 |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr7 |
vhsDetection |
VHSDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSDR6 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20120926 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20140409 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20150108 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20160114 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20160507 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20170630 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20180419 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20201209 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20231101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VHSv20240731 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
videoDetection |
VIDEODR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
videoDetection |
VIDEODR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
videoDetection |
VIDEODR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
videoDetection |
VIDEODR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
videoDetection |
VIDEOv20111208 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGv20110714 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGv20111019 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGv20130417 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGv20140402 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGv20150421 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGv20151230 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGv20160406 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGv20161202 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingDetection |
VIKINGv20170715 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7, calculated from aperJkyNoAperCorr7 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr7 |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Derived averaged Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7, calculated from aperJkyNoAperCorr7 |
real |
4 |
mag |
|
phot.mag |
aperMagNoAperCorr7 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr7 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 7 |
real |
4 |
mag |
|
phot.lup |
aperMagNoAperCorr7 |
vmcDetection |
VMCDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCDR3 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCDR4 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20110816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20110909 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20120126 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20121128 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20130304 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20130805 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20140428 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20140903 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20150309 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20151218 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20160311 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20160822 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20170109 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20170411 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20171101 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20180702 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20181120 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20191212 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20210708 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20230816 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcDetection |
VMCv20240226 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vvvDetection |
VVVDR1 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vvvDetection |
VVVDR2 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
phot.mag |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperture |
RequiredListDrivenProduct |
VHSDR1 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VHSDR2 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VHSv20120926 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VIDEODR2 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VIDEODR3 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VIDEOv20100513 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VIDEOv20111208 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VIKINGDR2 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VIKINGDR3 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VIKINGv20110714 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VIKINGv20111019 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VMCDR1 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VMCv20110816 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VMCv20110909 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VMCv20120126 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VMCv20121128 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VMCv20130304 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VVVDR1 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VVVv20100531 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VVVv20110718 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
apertureID |
MapApertureIDsultraVistaMapLc, MapApertureIDsultravistaDual |
ULTRAVISTADR4 |
UID of aperture unique over the MAP |
bigint |
8 |
|
|
meta.id;meta.main |
apertureID |
MapApertureIDsvikingZY_selJ |
VIKINGZYSELJv20160909 |
UID of aperture unique over the MAP |
bigint |
8 |
|
|
meta.id;meta.main |
apertureID |
MapApertureIDsvikingZY_selJ |
VIKINGZYSELJv20170124 |
UID of aperture unique over the MAP |
bigint |
8 |
|
|
meta.id;meta.main |
apertureID |
ultravistaMapAverageWeights, ultravistaMapRemeasAver |
ULTRAVISTADR4 |
UID of this aperture as assigned by MAP selection, see RequiredMatchedApertureProduct |
bigint |
8 |
|
|
meta_id;meta_main |
apertureID |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
UID of aperture from MapApertureIDsultraVistaMapLc |
bigint |
8 |
|
|
meta.main;meta.id |
apertureID |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
UID of this aperture as assigned by MAP selection, see RequiredMatchedApertureProduct {catalogue TType keyword: Aperture_ID} |
bigint |
8 |
|
|
meta.id;meta.main |
apertureID |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
UID of aperture |
bigint |
8 |
|
|
meta_id |
apertureID |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
UID of this aperture as assigned by MAP selection, see RequiredMatchedApertureProduct |
bigint |
8 |
|
|
meta_id;meta_main |
apertureID |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
UID of this aperture as assigned by MAP selection, see RequiredMatchedApertureProduct |
bigint |
8 |
|
|
meta_id;meta_main |
apertureID |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
UID of this aperture as assigned by MAP selection, see RequiredMatchedApertureProduct {catalogue TType keyword: Aperture_ID} |
bigint |
8 |
|
|
meta.id;meta.main |
apertureID |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
UID of this aperture as assigned by MAP selection, see RequiredMatchedApertureProduct {catalogue TType keyword: Aperture_ID} |
bigint |
8 |
|
|
meta.id;meta.main |
apertureID |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
UID of aperture |
bigint |
8 |
|
|
meta_id |
apertureID |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
UID of aperture |
bigint |
8 |
|
|
meta_id |
apFillF |
Detection |
PS1DR2 |
Aperture fill factor. |
real |
4 |
|
-999 |
|
apFlux |
Detection |
PS1DR2 |
Flux in seeing-dependent aperture. |
real |
4 |
Janskys |
-999 |
|
apFluxErr |
Detection |
PS1DR2 |
Error on flux in seeing-dependent aperture. |
real |
4 |
Janskys |
-999 |
|
APPDEC_R |
spectra |
SIXDF |
apparent DEC of field centre |
float |
8 |
radians |
|
|
APPDEC_V |
spectra |
SIXDF |
apparent DEC of field centre |
float |
8 |
radians |
|
|
APPRA_R |
spectra |
SIXDF |
apparent RA of field centre |
float |
8 |
radians |
|
|
APPRA_V |
spectra |
SIXDF |
apparent RA of field centre |
float |
8 |
radians |
|
|
apRadius |
Detection |
PS1DR2 |
Aperture radius. |
real |
4 |
arcsec |
-999 |
|
aProf1 |
sharksDetection |
SHARKSv20210222 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
sharksDetection |
SHARKSv20210421 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
meta.number |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
vhsDetection |
VHSDR2 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSDR3 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSDR4 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSDR5 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSDR6 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20120926 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20130417 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20140409 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20150108 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20160114 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20160507 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20170630 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20180419 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20201209 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20231101 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection |
VHSv20240731 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
videoDetection |
VIDEODR2 |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
meta.number |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
videoDetection |
VIDEODR3 |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
meta.number |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
videoDetection |
VIDEODR4 |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
meta.number |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
videoDetection |
VIDEODR5 |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
meta.number |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
videoDetection |
VIDEOv20100513 |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
meta.number |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
videoDetection |
VIDEOv20111208 |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
meta.number |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
videoListRemeasurement |
VIDEOv20100513 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGDR2 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGDR3 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGDR4 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGv20111019 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGv20130417 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGv20140402 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGv20150421 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGv20151230 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGv20160406 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGv20161202 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection |
VIKINGv20170715 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
meta.number |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
meta.number |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
vmcDetection |
VMCDR1 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCDR2 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCDR3 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCDR4 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCDR5 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20110909 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20120126 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20121128 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20130304 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20130805 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20140428 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20140903 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20150309 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20151218 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20160311 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20160822 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20170109 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20170411 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20171101 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20180702 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20181120 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20191212 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20210708 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20230816 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection |
VMCv20240226 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcdeepDetection |
VMCDEEPv20230713 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vmcdeepDetection |
VMCDEEPv20240506 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vvvDetection |
VVVDR1 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vvvDetection |
VVVDR2 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
meta.number |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf2 |
sharksDetection |
SHARKSv20210222 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
sharksDetection |
SHARKSv20210421 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf2 |
vhsDetection |
VHSDR2 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSDR3 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSDR4 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSDR5 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSDR6 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20120926 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20130417 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20140409 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20150108 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20160114 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20160507 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20170630 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20180419 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20201209 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20231101 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection |
VHSv20240731 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
videoDetection |
VIDEODR2 |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf2 |
videoDetection |
VIDEODR3 |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf2 |
videoDetection |
VIDEODR4 |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf2 |
videoDetection |
VIDEODR5 |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf2 |
videoDetection |
VIDEOv20100513 |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf2 |
videoDetection |
VIDEOv20111208 |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf2 |
videoListRemeasurement |
VIDEOv20100513 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGDR2 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGDR3 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGDR4 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGv20111019 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGv20130417 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGv20140402 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGv20150421 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGv20151230 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGv20160406 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGv20161202 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection |
VIKINGv20170715 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf2 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf2 |
vmcDetection |
VMCDR1 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCDR2 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCDR3 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCDR4 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCDR5 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20110909 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20120126 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20121128 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20130304 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20130805 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20140428 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20140903 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20150309 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20151218 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20160311 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20160822 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20170109 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20170411 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20171101 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20180702 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20181120 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20191212 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20210708 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20230816 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection |
VMCv20240226 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcdeepDetection |
VMCDEEPv20230713 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vmcdeepDetection |
VMCDEEPv20240506 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vvvDetection |
VVVDR1 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vvvDetection |
VVVDR2 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf2 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
sharksDetection |
SHARKSv20210222 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
sharksDetection |
SHARKSv20210421 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf3 |
vhsDetection |
VHSDR2 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSDR3 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSDR4 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSDR5 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSDR6 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20120926 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20130417 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20140409 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20150108 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20160114 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20160507 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20170630 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20180419 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20201209 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20231101 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection |
VHSv20240731 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
videoDetection |
VIDEODR2 |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf3 |
videoDetection |
VIDEODR3 |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf3 |
videoDetection |
VIDEODR4 |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf3 |
videoDetection |
VIDEODR5 |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf3 |
videoDetection |
VIDEOv20100513 |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf3 |
videoDetection |
VIDEOv20111208 |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf3 |
videoListRemeasurement |
VIDEOv20100513 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGDR2 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGDR3 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGDR4 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGv20111019 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGv20130417 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGv20140402 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGv20150421 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGv20151230 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGv20160406 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGv20161202 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection |
VIKINGv20170715 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf3 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf3 |
vmcDetection |
VMCDR1 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCDR2 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCDR3 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCDR4 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCDR5 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20110909 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20120126 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20121128 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20130304 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20130805 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20140428 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20140903 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20150309 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20151218 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20160311 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20160822 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20170109 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20170411 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20171101 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20180702 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20181120 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20191212 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20210708 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20230816 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection |
VMCv20240226 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcdeepDetection |
VMCDEEPv20230713 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vmcdeepDetection |
VMCDEEPv20240506 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vvvDetection |
VVVDR1 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vvvDetection |
VVVDR2 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf3 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
sharksDetection |
SHARKSv20210222 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
sharksDetection |
SHARKSv20210421 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf4 |
vhsDetection |
VHSDR2 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSDR3 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSDR4 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSDR5 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSDR6 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20120926 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20130417 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20140409 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20150108 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20160114 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20160507 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20170630 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20180419 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20201209 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20231101 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection |
VHSv20240731 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
videoDetection |
VIDEODR2 |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf4 |
videoDetection |
VIDEODR3 |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf4 |
videoDetection |
VIDEODR4 |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf4 |
videoDetection |
VIDEODR5 |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf4 |
videoDetection |
VIDEOv20100513 |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf4 |
videoDetection |
VIDEOv20111208 |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf4 |
videoListRemeasurement |
VIDEOv20100513 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGDR2 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGDR3 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGDR4 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGv20111019 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGv20130417 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGv20140402 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGv20150421 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGv20151230 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGv20160406 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGv20161202 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection |
VIKINGv20170715 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf4 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf4 |
vmcDetection |
VMCDR1 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCDR2 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCDR3 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCDR4 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCDR5 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20110909 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20120126 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20121128 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20130304 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20130805 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20140428 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20140903 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20150309 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20151218 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20160311 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20160822 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20170109 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20170411 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20171101 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20180702 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20181120 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20191212 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20210708 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20230816 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection |
VMCv20240226 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcdeepDetection |
VMCDEEPv20230713 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vmcdeepDetection |
VMCDEEPv20240506 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vvvDetection |
VVVDR1 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vvvDetection |
VVVDR2 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf4 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
sharksDetection |
SHARKSv20210222 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
sharksDetection |
SHARKSv20210421 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf5 |
vhsDetection |
VHSDR2 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSDR3 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSDR4 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSDR5 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSDR6 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20120926 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20130417 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20140409 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20150108 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20160114 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20160507 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20170630 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20180419 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20201209 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20231101 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection |
VHSv20240731 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
videoDetection |
VIDEODR2 |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf5 |
videoDetection |
VIDEODR3 |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf5 |
videoDetection |
VIDEODR4 |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf5 |
videoDetection |
VIDEODR5 |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf5 |
videoDetection |
VIDEOv20100513 |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf5 |
videoDetection |
VIDEOv20111208 |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf5 |
videoListRemeasurement |
VIDEOv20100513 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGDR2 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGDR3 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGDR4 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGv20111019 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGv20130417 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGv20140402 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGv20150421 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGv20151230 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGv20160406 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGv20161202 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection |
VIKINGv20170715 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf5 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf5 |
vmcDetection |
VMCDR1 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCDR2 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCDR3 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCDR4 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCDR5 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20110909 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20120126 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20121128 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20130304 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20130805 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20140428 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20140903 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20150309 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20151218 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20160311 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20160822 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20170109 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20170411 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20171101 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20180702 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20181120 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20191212 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20210708 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20230816 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection |
VMCv20240226 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcdeepDetection |
VMCDEEPv20230713 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vmcdeepDetection |
VMCDEEPv20240506 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vvvDetection |
VVVDR1 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vvvDetection |
VVVDR2 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf5 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
sharksDetection |
SHARKSv20210222 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
sharksDetection |
SHARKSv20210421 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf6 |
vhsDetection |
VHSDR2 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSDR3 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSDR4 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSDR5 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSDR6 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20120926 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20130417 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20140409 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20150108 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20160114 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20160507 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20170630 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20180419 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20201209 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20231101 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection |
VHSv20240731 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
videoDetection |
VIDEODR2 |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf6 |
videoDetection |
VIDEODR3 |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf6 |
videoDetection |
VIDEODR4 |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf6 |
videoDetection |
VIDEODR5 |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf6 |
videoDetection |
VIDEOv20100513 |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf6 |
videoDetection |
VIDEOv20111208 |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf6 |
videoListRemeasurement |
VIDEOv20100513 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGDR2 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGDR3 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGDR4 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGv20111019 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGv20130417 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGv20140402 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGv20150421 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGv20151230 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGv20160406 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGv20161202 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection |
VIKINGv20170715 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf6 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf6 |
vmcDetection |
VMCDR1 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCDR2 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCDR3 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCDR4 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCDR5 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20110909 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20120126 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20121128 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20130304 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20130805 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20140428 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20140903 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20150309 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20151218 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20160311 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20160822 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20170109 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20170411 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20171101 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20180702 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20181120 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20191212 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20210708 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20230816 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection |
VMCv20240226 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcdeepDetection |
VMCDEEPv20230713 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vmcdeepDetection |
VMCDEEPv20240506 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vvvDetection |
VVVDR1 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vvvDetection |
VVVDR2 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf6 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
sharksDetection |
SHARKSv20210222 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
sharksDetection |
SHARKSv20210421 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf7 |
vhsDetection |
VHSDR2 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSDR3 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSDR4 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSDR5 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSDR6 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20120926 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20130417 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20140409 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20150108 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20160114 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20160507 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20170630 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20180419 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20201209 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20231101 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection |
VHSv20240731 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
videoDetection |
VIDEODR2 |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf7 |
videoDetection |
VIDEODR3 |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf7 |
videoDetection |
VIDEODR4 |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf7 |
videoDetection |
VIDEODR5 |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf7 |
videoDetection |
VIDEOv20100513 |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf7 |
videoDetection |
VIDEOv20111208 |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf7 |
videoListRemeasurement |
VIDEOv20100513 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGDR2 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGDR3 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGDR4 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGv20111019 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGv20130417 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGv20140402 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGv20150421 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGv20151230 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGv20160406 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGv20161202 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection |
VIKINGv20170715 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf7 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf7 |
vmcDetection |
VMCDR1 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCDR2 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCDR3 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCDR4 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCDR5 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20110909 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20120126 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20121128 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20130304 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20130805 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20140428 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20140903 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20150309 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20151218 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20160311 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20160822 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20170109 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20170411 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20171101 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20180702 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20181120 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20191212 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20210708 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20230816 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection |
VMCv20240226 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcdeepDetection |
VMCDEEPv20230713 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vmcdeepDetection |
VMCDEEPv20240506 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vvvDetection |
VVVDR1 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vvvDetection |
VVVDR2 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf7 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
sharksDetection |
SHARKSv20210222 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
sharksDetection |
SHARKSv20210421 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf8 |
vhsDetection |
VHSDR2 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSDR3 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSDR4 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSDR5 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSDR6 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20120926 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20130417 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20140409 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20150108 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20160114 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20160507 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20170630 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20180419 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20201209 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20231101 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection |
VHSv20240731 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
videoDetection |
VIDEODR2 |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf8 |
videoDetection |
VIDEODR3 |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf8 |
videoDetection |
VIDEODR4 |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf8 |
videoDetection |
VIDEODR5 |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf8 |
videoDetection |
VIDEOv20100513 |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf8 |
videoDetection |
VIDEOv20111208 |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf8 |
videoListRemeasurement |
VIDEOv20100513 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGDR2 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGDR3 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGDR4 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGv20111019 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGv20130417 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGv20140402 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGv20150421 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGv20151230 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGv20160406 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGv20161202 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection |
VIKINGv20170715 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf8 |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
meta.number |
aProf8 |
vmcDetection |
VMCDR1 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCDR2 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCDR3 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCDR4 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCDR5 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20110909 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20120126 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20121128 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20130304 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20130805 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20140428 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20140903 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20150309 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20151218 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20160311 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20160822 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20170109 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20170411 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20171101 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20180702 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20181120 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20191212 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20210708 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20230816 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection |
VMCv20240226 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcdeepDetection |
VMCDEEPv20230713 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vmcdeepDetection |
VMCDEEPv20240506 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vvvDetection |
VVVDR1 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vvvDetection |
VVVDR2 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
aProf8 |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
meta.number |
arcfile |
Multiframe |
SHARKSv20210222 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
SHARKSv20210421 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
ULTRAVISTADR4 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSDR1 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSDR2 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSDR3 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSDR4 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSDR5 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSDR6 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20120926 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20130417 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20140409 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20150108 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20160114 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20160507 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20170630 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20180419 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20201209 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20231101 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VHSv20240731 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIDEODR2 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIDEODR3 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIDEODR4 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIDEODR5 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIDEOv20100513 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIDEOv20111208 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGDR2 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGDR3 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGDR4 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGv20110714 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGv20111019 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGv20130417 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGv20140402 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGv20150421 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGv20151230 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGv20160406 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGv20161202 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VIKINGv20170715 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCDEEPv20230713 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCDEEPv20240506 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCDR1 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCDR2 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCDR3 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCDR4 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCDR5 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20110816 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20110909 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20120126 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20121128 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20130304 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20130805 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20140428 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20140903 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20150309 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20151218 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20160311 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20160822 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20170109 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20170411 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20171101 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20180702 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20181120 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20191212 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20210708 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20230816 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VMCv20240226 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VVVDR1 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VVVDR2 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VVVDR5 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VVVXDR1 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VVVv20100531 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VVVv20110718 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Archive File Name |
varchar |
64 |
|
NONE |
|
archiveName |
RequiredMatchedApertureProduct |
SHARKSv20210222 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
SHARKSv20210421 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
ULTRAVISTADR4 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VHSv20201209 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VHSv20231101 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VHSv20240731 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VMCDEEPv20230713 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VMCDEEPv20240506 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VMCDR5 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VMCv20191212 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VMCv20210708 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VMCv20230816 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VMCv20240226 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VVVDR5 |
Archive of main programme.. |
varchar |
16 |
|
|
|
archiveName |
RequiredMatchedApertureProduct |
VVVXDR1 |
Archive of main programme.. |
varchar |
16 |
|
|
|
AREA |
grs_ngpSource, grs_ranSource, grs_sgpSource |
TWODFGRS |
Isophotal area in pixels |
real |
4 |
|
|
|
areaID |
Multiframe |
SHARKSv20210222 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
SHARKSv20210421 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
ULTRAVISTADR4 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSDR1 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSDR2 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSDR3 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSDR4 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSDR5 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSDR6 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20120926 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20130417 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20140409 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20150108 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20160114 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20160507 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20170630 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20180419 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20201209 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20231101 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VHSv20240731 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIDEODR2 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIDEODR3 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIDEODR4 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIDEODR5 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIDEOv20111208 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGDR2 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGDR3 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGDR4 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGv20110714 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGv20111019 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGv20130417 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGv20140402 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGv20150421 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGv20151230 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGv20160406 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGv20161202 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VIKINGv20170715 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCDEEPv20230713 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCDEEPv20240506 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCDR1 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCDR2 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCDR3 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCDR4 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCDR5 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20110816 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20110909 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20120126 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20121128 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20130304 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20130805 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20140428 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20140903 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20150309 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20151218 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20160311 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20160822 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20170109 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20170411 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20171101 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20180702 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20181120 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20191212 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20210708 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20230816 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VMCv20240226 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VVVDR1 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VVVDR2 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VVVDR5 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VVVXDR1 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VVVv20110718 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
SADT Survey area ID |
int |
4 |
|
-99999999 |
|
astrometric_chi2_al |
gaia_source |
GAIADR2 |
Along-Scan chi-square value |
real |
4 |
|
|
stat.fit.chi2 |
astrometric_chi2_al |
gaia_source |
GAIAEDR3 |
Along-Scan chi-square value |
real |
4 |
|
|
stat.fit.chi2 |
astrometric_delta_q |
gaia_source, tgas_source |
GAIADR1 |
Hipparcos/Gaia data discrepancy (Hipparcos subset of TGAS only) |
real |
4 |
|
|
stat.value |
astrometric_excess_noise |
gaia_source |
GAIADR2 |
Excess noise of the source |
float |
8 |
milliarcsec |
|
stat.value |
astrometric_excess_noise |
gaia_source |
GAIAEDR3 |
Excess noise of the source |
real |
4 |
milliarcsec |
|
stat.value |
astrometric_excess_noise |
gaia_source, tgas_source |
GAIADR1 |
Excess noise of the source |
float |
8 |
milliarcsec |
|
stat.value |
astrometric_excess_noise_sig |
gaia_source |
GAIADR2 |
Significance of the excess noise |
float |
8 |
|
|
stat.value |
astrometric_excess_noise_sig |
gaia_source |
GAIAEDR3 |
Significance of the excess noise |
real |
4 |
|
|
stat.value |
astrometric_excess_noise_sig |
gaia_source, tgas_source |
GAIADR1 |
Significance of the excess noise |
float |
8 |
|
|
stat.value |
astrometric_gof_al |
gaia_source |
GAIADR2 |
Goodness of fit statistic of model wrt Along-Scan observations |
real |
4 |
|
|
stat.fit.goodness |
astrometric_gof_al |
gaia_source |
GAIAEDR3 |
Goodness of fit statistic of model wrt Along-Scan observations |
real |
4 |
|
|
stat.fit.goodness |
astrometric_matched_observations |
gaia_source |
GAIADR2 |
Matched FoV transits used in the AGIS solution |
smallint |
2 |
|
|
meta.number |
astrometric_matched_transits |
gaia_source |
GAIAEDR3 |
Matched FoV transits used in the AGIS solution |
smallint |
2 |
|
|
meta.number |
astrometric_n_bad_obs_ac |
gaia_source, tgas_source |
GAIADR1 |
Number of bad observations in the Across-Scan direction |
int |
4 |
|
|
meta.number |
astrometric_n_bad_obs_al |
gaia_source |
GAIADR2 |
Number of bad observations in the Along-Scan direction |
int |
4 |
|
|
meta.number |
astrometric_n_bad_obs_al |
gaia_source |
GAIAEDR3 |
Number of bad observations in the Along-Scan direction |
smallint |
2 |
|
|
meta.number |
astrometric_n_bad_obs_al |
gaia_source, tgas_source |
GAIADR1 |
Number of bad observations in the Along-Scan direction |
int |
4 |
|
|
meta.number |
astrometric_n_good_obs_ac |
gaia_source, tgas_source |
GAIADR1 |
Number of good observations in the Across-Scan direction |
int |
4 |
|
|
meta.number |
astrometric_n_good_obs_al |
gaia_source |
GAIADR2 |
Number of good observations in the Along-Scan direction |
int |
4 |
|
|
meta.number |
astrometric_n_good_obs_al |
gaia_source |
GAIAEDR3 |
Number of good observations in the Along-Scan direction |
smallint |
2 |
|
|
meta.number |
astrometric_n_good_obs_al |
gaia_source, tgas_source |
GAIADR1 |
Number of good observations in the Along-Scan direction |
int |
4 |
|
|
meta.number |
astrometric_n_obs_ac |
gaia_source |
GAIADR2 |
Total number of observations in the Across-Scan direction |
int |
4 |
|
|
meta.number |
astrometric_n_obs_ac |
gaia_source |
GAIAEDR3 |
Total number of observations in the Across-Scan direction |
smallint |
2 |
|
|
meta.number |
astrometric_n_obs_ac |
gaia_source, tgas_source |
GAIADR1 |
Total number of observations in the Across-Scan direction |
int |
4 |
|
|
meta.number |
astrometric_n_obs_al |
gaia_source |
GAIADR2 |
Total number of observations in the Along-Scan direction |
int |
4 |
|
|
meta.number |
astrometric_n_obs_al |
gaia_source |
GAIAEDR3 |
Total number of observations in the Along-Scan direction |
smallint |
2 |
|
|
meta.number |
astrometric_n_obs_al |
gaia_source, tgas_source |
GAIADR1 |
Total number of observations in the Along-Scan direction |
int |
4 |
|
|
meta.number |
astrometric_params_solved |
gaia_source |
GAIADR2 |
Which parameters have been solved for? |
tinyint |
1 |
|
|
meta.number |
astrometric_params_solved |
gaia_source |
GAIAEDR3 |
Which parameters have been solved for? |
tinyint |
1 |
|
|
meta.number |
astrometric_primary_flag |
gaia_source |
GAIADR2 |
Primary or secondary |
tinyint |
1 |
|
|
meta.code.status |
astrometric_primary_flag |
gaia_source |
GAIAEDR3 |
Primary or secondary |
tinyint |
1 |
|
|
meta.code.status |
astrometric_primary_flag |
gaia_source, tgas_source |
GAIADR1 |
Primary or secondary |
bit |
1 |
|
|
meta.code |
astrometric_priors_used |
aux_qso_icrf2_match |
GAIADR1 |
Type of prior used in the astrometric solution |
int |
4 |
|
|
meta.number |
astrometric_priors_used |
gaia_source, tgas_source |
GAIADR1 |
Type of prior used in the astrometric solution |
int |
4 |
|
|
|
astrometric_pseudo_colour |
gaia_source |
GAIADR2 |
Astrometrically determined pseudocolour of the source |
real |
4 |
micron^-1 |
|
em.wavenumber |
astrometric_pseudo_colour_error |
gaia_source |
GAIADR2 |
STandard error of the pseudocolour of the source |
real |
4 |
micron^-1 |
|
em.wavenumber |
astrometric_relegation_factor |
gaia_source, tgas_source |
GAIADR1 |
Relegation factor |
real |
4 |
|
|
arith.factor |
astrometric_sigma_5d_max |
gaia_source |
GAIADR2 |
The longest semi-major axis of the 5d error ellipsoid |
real |
4 |
mas |
|
pos.errorEllipse;stat.max |
astrometric_sigma_5d_max |
gaia_source |
GAIAEDR3 |
The longest semi-major axis of the 5d error ellipsoid |
real |
4 |
mas |
|
pos.errorEllipse;stat.max |
astrometric_weight_ac |
gaia_source, tgas_source |
GAIADR1 |
Mean astrometric weight of the source Across-Scan |
real |
4 |
|
|
stat.weight;stat.mean |
astrometric_weight_al |
gaia_source |
GAIADR2 |
Mean astrometric weight of the source Along-Scan |
real |
4 |
mas^-2 |
|
stat.weight;stat.mean |
astrometric_weight_al |
gaia_source, tgas_source |
GAIADR1 |
Mean astrometric weight of the source Along-Scan |
real |
4 |
|
|
stat.weight;stat.mean |
attr |
PreviousCalibParams |
SHARKSv20210222 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
SHARKSv20210421 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
VHSv20201209 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
VHSv20231101 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
VHSv20240731 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
VMCDEEPv20230713 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
VMCDEEPv20240506 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
VMCv20210708 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
VMCv20230816 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
VMCv20240226 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
VVVDR5 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
attr |
PreviousCalibParams |
VVVXDR1 |
Attribute that has been modified |
varchar |
32 |
|
NONE |
|
aux_epc |
igsl_source |
GAIADR1 |
Flag indicating presence in Ecliptic Poles Catalogue (0 = no; 1 = yes) |
bit |
1 |
|
|
meta.id;meta.dataset |
aux_gsc23 |
igsl_source |
GAIADR1 |
Flag indicating presence in GSC2.3 (0 = no; 1 = yes) |
bit |
1 |
|
|
meta.id;meta.dataset |
aux_hip |
igsl_source |
GAIADR1 |
Flag indicating presence in Hipparcos (0 = no; 1 = yes) |
bit |
1 |
|
|
meta.id;meta.dataset |
aux_lqrf |
igsl_source |
GAIADR1 |
Flag indicating presence in LQRF (0 = no; 1 = yes) |
bit |
1 |
|
|
meta.id;meta.dataset |
aux_ogle |
igsl_source |
GAIADR1 |
Flag indicating presence in OGLE (0 = no; 1 = yes) |
bit |
1 |
|
|
meta.id;meta.dataset |
aux_ppmxl |
igsl_source |
GAIADR1 |
Flag indicating presence in PPMXL (0 = no; 1 = yes) |
bit |
1 |
|
|
meta.id;meta.dataset |
aux_sdss |
igsl_source |
GAIADR1 |
Flag indicating presence in SDSS (0 = no; 1 = yes) |
bit |
1 |
|
|
meta.id;meta.dataset |
aux_tmass |
igsl_source |
GAIADR1 |
Flag indicating presence in 2MASS PSC (0 = no; 1 = yes) |
bit |
1 |
|
|
meta.id;meta.dataset |
aux_tycho |
igsl_source |
GAIADR1 |
Flag indicating presence in Tycho (0 = no; 1 = yes) |
bit |
1 |
|
|
meta.id;meta.dataset |
aux_ucac |
igsl_source |
GAIADR1 |
Flag indicating presence in UCAC (0 = no; 1 = yes) |
bit |
1 |
|
|
meta.id;meta.dataset |
AV_Schlegel |
ravedr5Source |
RAVE |
|
float |
8 |
mag Total Extinction in V-band from Schlegel et al. (1998) |
|
phys.absorption |
aVar |
vvvVivaCatalogue |
VVVDR5 |
The difference between 5th and 95th percentile of magnitude in order to provide a rough estimation of variability amplitude {catalogue TType keyword: Avar} |
float |
8 |
mag |
-9.999995e8 |
|
averageConf |
sharksDetection |
SHARKSv20210222 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
sharksDetection |
SHARKSv20210421 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
ultravistaDetection |
ULTRAVISTADR4 |
The average confidence level in the default 2 arcsec diameter aperture (aper3), not available in SE output {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Weighted mean average confidence level in the default 2 arcsec diameter aperture (aper3) (SE: default) |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
The average confidence level in the default 2 arcsec diameter aperture (aper3) (SE: default) {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSDR2 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
vhsDetection |
VHSDR3 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSDR4 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSDR5 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSDR6 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20120926 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20130417 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20140409 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20150108 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20160114 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20160507 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20170630 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20180419 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20201209 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20231101 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection |
VHSv20240731 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
videoDetection |
VIDEODR2 |
The average confidence level in the default 2 arcsec diameter aperture (aper3), not available in SE output {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
videoDetection |
VIDEODR3 |
The average confidence level in the default 2 arcsec diameter aperture (aper3), not available in SE output {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
stat.likelihood |
averageConf |
videoDetection |
VIDEODR4 |
The average confidence level in the default 2 arcsec diameter aperture (aper3), not available in SE output {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
videoDetection |
VIDEODR5 |
The average confidence level in the default 2 arcsec diameter aperture (aper3), not available in SE output {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
videoDetection |
VIDEOv20100513 |
The average confidence level in the default 2 arcsec diameter aperture (aper3), not available in SE output {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
videoDetection |
VIDEOv20111208 |
The average confidence level in the default 2 arcsec diameter aperture (aper3), not available in SE output {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
videoListRemeasurement |
VIDEOv20100513 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
vikingDetection |
VIKINGDR2 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
vikingDetection |
VIKINGDR3 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
stat.likelihood |
averageConf |
vikingDetection |
VIKINGDR4 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingDetection |
VIKINGv20111019 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
vikingDetection |
VIKINGv20130417 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingDetection |
VIKINGv20140402 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingDetection |
VIKINGv20150421 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingDetection |
VIKINGv20151230 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingDetection |
VIKINGv20160406 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingDetection |
VIKINGv20161202 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingDetection |
VIKINGv20170715 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Weighted mean average confidence level in the default 2 arcsec diameter aperture (aper3) (SE: default) |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Weighted mean average confidence level in the default 2 arcsec diameter aperture (aper3) (SE: default) |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
The average confidence level in the default 2 arcsec diameter aperture (aper3) (SE: default) {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
The average confidence level in the default 2 arcsec diameter aperture (aper3) (SE: default) {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCDR1 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
vmcDetection |
VMCDR2 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCDR3 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCDR4 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCDR5 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20110909 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
vmcDetection |
VMCv20120126 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
vmcDetection |
VMCv20121128 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20130304 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20130805 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20140428 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20140903 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20150309 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20151218 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20160311 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20160822 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20170109 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20170411 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20171101 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20180702 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20181120 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20191212 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20210708 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20230816 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection |
VMCv20240226 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageConf |
vmcdeepDetection |
VMCDEEPv20230713 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vmcdeepDetection |
VMCDEEPv20240506 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vvvDetection |
VVVDR1 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
stat.likelihood |
averageConf |
vvvDetection |
VVVDR2 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-0.9999995e9 |
stat.likelihood |
averageConf |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
meta.code |
averageCoverage160 |
sage_lmcMips160Source |
SPITZER |
The average coverage (# of independent observations per pixel) |
float |
8 |
|
|
|
averageCoverage24 |
sage_lmcMips24Source |
SPITZER |
The average coverage (# of independent observations per pixel) |
float |
8 |
|
|
|
averageCoverage70 |
sage_lmcMips70Source |
SPITZER |
The average coverage (# of independent observations per pixel) |
float |
8 |
|
|
|
avSaturLevel |
MultiframeDetector |
SHARKSv20210222 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
SHARKSv20210421 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
ULTRAVISTADR4 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSDR1 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSDR2 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSDR3 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSDR4 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSDR5 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSDR6 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20120926 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20130417 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20140409 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20150108 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20160114 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20160507 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20170630 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20180419 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20201209 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20231101 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VHSv20240731 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIDEODR2 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIDEODR3 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIDEODR4 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIDEODR5 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIDEOv20100513 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIDEOv20111208 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGDR2 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGDR3 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGDR4 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGv20110714 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGv20111019 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGv20130417 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGv20140402 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGv20150421 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGv20151230 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGv20160406 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGv20161202 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VIKINGv20170715 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCDEEPv20230713 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCDEEPv20240506 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCDR1 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCDR2 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCDR3 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCDR4 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCDR5 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20110816 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20110909 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20120126 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20121128 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20130304 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20130805 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20140428 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20140903 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20150309 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20151218 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20160311 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20160822 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20170109 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20170411 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20171101 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20180702 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20181120 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20191212 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20210708 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20230816 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VMCv20240226 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VVVDR1 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VVVDR2 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VVVDR5 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VVVXDR1 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VVVv20100531 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VVVv20110718 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Average saturation level in frame |
real |
4 |
|
-0.9999995e9 |
|
avSetupID |
MapProvenance |
ULTRAVISTADR4 |
the UID of the averaging system |
int |
4 |
|
|
|
avStellarEll |
MultiframeDetector |
SHARKSv20210222 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
SHARKSv20210421 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
ULTRAVISTADR4 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSDR1 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSDR2 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSDR3 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSDR4 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSDR5 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSDR6 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20120926 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20130417 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20140409 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20150108 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20160114 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20160507 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20170630 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20180419 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20201209 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20231101 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VHSv20240731 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIDEODR2 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIDEODR3 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIDEODR4 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIDEODR5 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIDEOv20100513 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIDEOv20111208 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGDR2 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGDR3 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGDR4 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGv20110714 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGv20111019 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGv20130417 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGv20140402 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGv20150421 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGv20151230 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGv20160406 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGv20161202 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VIKINGv20170715 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCDEEPv20230713 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCDEEPv20240506 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCDR1 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCDR2 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCDR3 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCDR4 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCDR5 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20110816 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20110909 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20120126 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20121128 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20130304 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20130805 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20140428 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20140903 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20150309 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20151218 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20160311 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20160822 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20170109 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20170411 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20171101 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20180702 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20181120 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20191212 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20210708 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20230816 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VMCv20240226 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VVVDR1 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VVVDR2 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VVVDR5 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VVVXDR1 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VVVv20100531 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
MultiframeDetector |
VVVv20110718 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
avStellarEll |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Average stellar ellipticity (1-b/a) |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
axis1Length |
MultiframeDetector |
SHARKSv20210222 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
SHARKSv20210421 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
ULTRAVISTADR4 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSDR1 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSDR2 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSDR3 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSDR4 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSDR5 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSDR6 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20120926 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20130417 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20140409 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20150108 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20160114 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20160507 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20170630 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20180419 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20201209 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20231101 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VHSv20240731 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIDEODR2 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIDEODR3 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIDEODR4 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIDEODR5 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIDEOv20100513 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIDEOv20111208 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGDR2 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGDR3 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGDR4 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGv20110714 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGv20111019 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGv20130417 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGv20140402 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGv20150421 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGv20151230 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGv20160406 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGv20161202 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VIKINGv20170715 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCDEEPv20230713 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCDEEPv20240506 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCDR1 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCDR2 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCDR3 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCDR4 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCDR5 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20110816 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20110909 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20120126 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20121128 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20130304 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20130805 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20140428 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20140903 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20150309 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20151218 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20160311 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20160822 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20170109 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20170411 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20171101 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20180702 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20181120 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20191212 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20210708 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20230816 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VMCv20240226 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VVVDR1 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VVVDR2 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VVVDR5 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VVVXDR1 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VVVv20100531 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
MultiframeDetector |
VVVv20110718 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
-99999999 |
meta.number |
axis1Length |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
|
meta.number |
axis2Length |
MultiframeDetector |
SHARKSv20210222 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
SHARKSv20210421 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
ULTRAVISTADR4 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSDR1 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSDR2 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSDR3 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSDR4 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSDR5 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSDR6 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20120926 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20130417 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20140409 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20150108 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20160114 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20160507 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20170630 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20180419 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20201209 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20231101 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VHSv20240731 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIDEODR2 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIDEODR3 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIDEODR4 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIDEODR5 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIDEOv20100513 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIDEOv20111208 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGDR2 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGDR3 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGDR4 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGv20110714 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGv20111019 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGv20130417 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGv20140402 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGv20150421 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGv20151230 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGv20160406 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGv20161202 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VIKINGv20170715 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCDEEPv20230713 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCDEEPv20240506 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCDR1 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCDR2 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCDR3 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCDR4 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCDR5 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20110816 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20110909 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20120126 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20121128 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20130304 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20130805 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20140428 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20140903 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20150309 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20151218 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20160311 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20160822 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20170109 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20170411 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20171101 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20180702 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20181120 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20191212 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20210708 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20230816 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VMCv20240226 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VVVDR1 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VVVDR2 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VVVDR5 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VVVXDR1 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VVVv20100531 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
MultiframeDetector |
VVVv20110718 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
-99999999 |
meta.number |
axis2Length |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
|
meta.number |
aY |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSDR1 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aY |
vhsSource |
VHSDR2 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aY |
vhsSource |
VHSDR3 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSDR4 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSDR5 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSDR6 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20120926 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20130417 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20140409 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20150108 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20160114 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20160507 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20170630 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20180419 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20201209 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20231101 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vhsSource |
VHSv20240731 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
videoSource |
VIDEODR2 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aY |
videoSource |
VIDEODR3 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
videoSource |
VIDEODR4 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
videoSource |
VIDEODR5 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
videoSource |
VIDEOv20100513 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aY |
videoSource |
VIDEOv20111208 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aY |
vikingSource |
VIKINGDR2 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aY |
vikingSource |
VIKINGDR3 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vikingSource |
VIKINGDR4 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vikingSource |
VIKINGv20110714 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aY |
vikingSource |
VIKINGv20111019 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aY |
vikingSource |
VIKINGv20130417 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vikingSource |
VIKINGv20140402 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vikingSource |
VIKINGv20150421 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vikingSource |
VIKINGv20151230 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vikingSource |
VIKINGv20160406 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vikingSource |
VIKINGv20161202 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vikingSource |
VIKINGv20170715 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aY |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
videoSource |
VIDEODR2 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aZ |
videoSource |
VIDEODR3 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
videoSource |
VIDEODR4 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
videoSource |
VIDEODR5 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
videoSource |
VIDEOv20100513 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aZ |
videoSource |
VIDEOv20111208 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aZ |
vikingSource |
VIKINGDR2 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aZ |
vikingSource |
VIKINGDR3 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
vikingSource |
VIKINGDR4 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
vikingSource |
VIKINGv20110714 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aZ |
vikingSource |
VIKINGv20111019 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aZ |
vikingSource |
VIKINGv20130417 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
vikingSource |
VIKINGv20140402 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
vikingSource |
VIKINGv20150421 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
vikingSource |
VIKINGv20151230 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
vikingSource |
VIKINGv20160406 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
vikingSource |
VIKINGv20161202 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
vikingSource |
VIKINGv20170715 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
aZ |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |