VSA Browser

Glossary of VSA attributes

This Glossary alphabetically lists all attributes used in the VSAv20240809 database(s) held in the VSA. If you would like to have more information about the schema tables please use the VSAv20240809 Schema Browser (other Browser versions).

A B C D E F G H I J K L M
N O P Q R S T U V W X Y Z

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

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amEnd Multiframe VIDEODR2 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4 -0.9999995e9 obs.airMass

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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

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ampI3 ogle3LpvLmcSource, ogle3LpvSmcSource OGLE I-band amplitude of the tertiary period real 4 mag src.var.amplitude

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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