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Glossary of VSA attributes

This Glossary alphabetically lists all attributes used in the VSAv20150413 database(s) held in the VSA. If you would like to have more information about the schema tables please use the VSAv20150413 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

NameSchema TableDatabaseDescriptionTypeLengthUnitDefault ValueUnified Content Descriptor
a twomass_psc 2MASS 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_IMAGE mgcDetection MGC Flux rms along major axis real 4 pixel    
A_V target SIXDF Schlegel V extinction real 4      
ABEMMA spectra SIXDF redshift type: abs=1,emi=2,man=3 int 4      
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 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 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 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 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 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 VSAQC 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 VVVv20110718 5-sigma limiting AB magnitude for point sources {catalogue extension keyword:  ABMAGLIM} real 4 mag -0.9999995e9  
abMagLim 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 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 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 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 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 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 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 VSAQC 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 VVVv20110718 Saturation limit for point sources (AB magnitude) {catalogue extension keyword:  ABMAGSAT} real 4 mag -0.9999995e9  
abSatMag 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    
adjacentFrameTolerance Programme SVNGC253v20100429 The match tolerance for adjacent frames in the survey real 4 Degrees   ??
adjacentFrameTolerance Programme SVORIONv20100429 The match tolerance for adjacent frames in the survey real 4 Degrees   ??
adjacentFrameTolerance Programme ULTRAVISTAv20100429 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 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 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 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 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 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 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 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 SVNGC253v20100429 The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. real 4   -0.9999995e9  
aebv Filter SVORIONv20100429 The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. real 4   -0.9999995e9  
aebv Filter ULTRAVISTAv20100429 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 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 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 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 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 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 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 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 VHSDR3 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 svNgc253Source SVNGC253v20100429 The galactic extinction correction in the H band for extragalactic objects real 4 mag -0.9999995e9  
aH ultravistaSource ULTRAVISTAv20100429 The galactic extinction correction in the H band for extragalactic objects real 4 mag -0.9999995e9  
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 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 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 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
air_temp twomass_scn 2MASS Air temperature at beginning of scan. real 4 degC   phys.temperature
air_temp twomass_sixx2_scn 2MASS air temperature (deg C) at beginning of scan real 4 degC    
airm twomass_scn 2MASS Airmass at beginning of scan. real 4     obs.airMass
airm twomass_sixx2_scn 2MASS beginning airmass of scan real 4      
aJ svNgc253Source SVNGC253v20100429 The galactic extinction correction in the J band for extragalactic objects real 4 mag -0.9999995e9  
aJ ultravistaSource ULTRAVISTAv20100429 The galactic extinction correction in the J band for extragalactic objects real 4 mag -0.9999995e9  
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 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 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 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
aKs svNgc253Source SVNGC253v20100429 The galactic extinction correction in the Ks band for extragalactic objects real 4 mag -0.9999995e9  
aKs ultravistaSource ULTRAVISTAv20100429 The galactic extinction correction in the Ks band for extragalactic objects real 4 mag -0.9999995e9  
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 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 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 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
amEnd Multiframe SVNGC253v20100429 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe SVORIONv20100429 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe ULTRAVISTAv20100429 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VHSDR1 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VHSDR2 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VHSDR3 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VHSv20120926 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VHSv20130417 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VHSv20140409 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VHSv20150108 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIDEODR2 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIDEODR3 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIDEODR4 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIDEOv20100513 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIDEOv20111208 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIKINGDR2 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIKINGDR3 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIKINGDR4 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIKINGv20110714 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIKINGv20111019 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIKINGv20130417 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIKINGv20140402 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VIKINGv20150421 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCDR1 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCDR2 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCDR3 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCv20110816 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCv20110909 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCv20120126 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCv20121128 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCv20130304 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCv20130805 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCv20140428 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCv20140903 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VMCv20150309 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VSAQC Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VVVDR1 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VVVDR2 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VVVv20100531 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd Multiframe VVVv20110718 Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} real 4   -0.9999995e9 obs.airMass
amEnd ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe VSAQC Airmass at end of observation real 4   -0.9999995e9 obs.airMass
amStart Multiframe SVNGC253v20100429 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe SVORIONv20100429 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe ULTRAVISTAv20100429 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe VHSDR1 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe VHSDR2 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe VHSDR3 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe VHSv20120926 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe VHSv20130417 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe VHSv20140409 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe VHSv20150108 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe VIDEODR2 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe VIDEODR3 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe VIDEODR4 Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} real 4   -0.9999995e9 obs.airMass
amStart Multiframe 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 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 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 VSAQC 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 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 ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe VSAQC Airmass at start of observation real 4   -0.9999995e9 obs.airMass
aNb118 svNgc253Source SVNGC253v20100429 The galactic extinction correction in the Nb118 band for extragalactic objects real 4 mag -0.9999995e9  
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 2MASS 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 2MASS 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 SVNGC253v20100429 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 SVORIONv20100429 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 ULTRAVISTAv20100429 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 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 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 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 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 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 VSAQC 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 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 ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector VSAQC Stellar aperture correction: 1⁄2 × core flux real 4   -0.9999995e9 ??
aperCor2 MultiframeDetector SVNGC253v20100429 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 SVORIONv20100429 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 ULTRAVISTAv20100429 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 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 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 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 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 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 VSAQC 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 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 ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector VSAQC Stellar aperture correction: 1⁄√2 core flux real 4   -0.9999995e9 ??
aperCor3 MultiframeDetector SVNGC253v20100429 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 SVORIONv20100429 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 ULTRAVISTAv20100429 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 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 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 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 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 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 VSAQC 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 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 ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector VSAQC Stellar aperture correction: core flux real 4   -0.9999995e9 ??
aperCor4 MultiframeDetector SVNGC253v20100429 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 SVORIONv20100429 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 ULTRAVISTAv20100429 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 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 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 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 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 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 VSAQC 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 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 ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector VSAQC Stellar aperture correction: √2 × core flux real 4   -0.9999995e9 ??
aperCor5 MultiframeDetector SVNGC253v20100429 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 SVORIONv20100429 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 ULTRAVISTAv20100429 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 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 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 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 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 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 VSAQC 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 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 ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector VSAQC Stellar aperture correction: 2 × core flux real 4   -0.9999995e9 ??
aperCor6 MultiframeDetector SVNGC253v20100429 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 SVORIONv20100429 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 ULTRAVISTAv20100429 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 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 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 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 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 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 VSAQC 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 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 ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector VSAQC Stellar aperture correction: 2√2 × core flux real 4   -0.9999995e9 ??
aperCor7 MultiframeDetector SVNGC253v20100429 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 SVORIONv20100429 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 ULTRAVISTAv20100429 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 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 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 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 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 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 VSAQC 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 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 ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector VSAQC Stellar aperture correction: 4 × core flux real 4   -0.9999995e9 ??
aperCorPeak MultiframeDetector SVNGC253v20100429 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 SVORIONv20100429 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 ULTRAVISTAv20100429 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 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 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 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 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 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 VSAQC 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 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 ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector VSAQC Stellar aperture correction: peak height real 4   -0.9999995e9 ??
aperFlux1 svNgc253Detection SVNGC253v20100429 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 svOrionDetection SVORIONv20100429 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 ultravistaDetection ULTRAVISTAv20100429 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 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 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 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 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 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 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 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 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 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 svNgc253Detection SVNGC253v20100429 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 svOrionDetection SVORIONv20100429 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 ultravistaDetection ULTRAVISTAv20100429 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 vhsDetection 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 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 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 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 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 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 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 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 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 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 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 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, 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
aperFlux10 vvvListRemeasurement VVVv20110718 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 svNgc253Detection SVNGC253v20100429 Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} real 4 ADU   stat.error
aperFlux10err svOrionDetection SVORIONv20100429 Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} real 4 ADU   stat.error
aperFlux10err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 10 (SE: FLUXERR_APER10) {catalogue TType keyword: Aper_flux_10_err} real 4 ADU   stat.error
aperFlux10err vhsDetection VHSDR1 Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} real 4 ADU   stat.error
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 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 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 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 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 VIKINGv20110714 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 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 VMCv20110816 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 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, vvvListRemeasurement VVVv20100531 Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} real 4 ADU   stat.error
aperFlux10err vvvListRemeasurement VVVv20110718 Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} real 4 ADU   stat.error
aperFlux11 svNgc253Detection SVNGC253v20100429 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 svOrionDetection SVORIONv20100429 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 ultravistaDetection ULTRAVISTAv20100429 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 vhsDetection 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 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 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 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 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 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 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 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 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 VMCv20110816 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux11 vmcDetection VMCv20110909 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux11 vmcDetection VMCv20120126 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux11 vmcDetection VMCv20121128 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux11 vmcDetection VMCv20130304 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux11 vmcDetection VMCv20130805 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux11 vmcDetection VMCv20140428 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux11 vmcDetection VMCv20140903 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux11 vmcDetection VMCv20150309 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux11 vvvDetection VVVDR1 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux11 vvvDetection VVVDR2 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux11 vvvDetection, vvvListRemeasurement VVVv20100531 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux11 vvvListRemeasurement VVVv20110718 default aperture flux 11 {catalogue TType keyword: Aper_flux_11}
8 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux11err svNgc253Detection SVNGC253v20100429 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err svOrionDetection SVORIONv20100429 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vhsDetection VHSDR1 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vhsDetection VHSDR2 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vhsDetection VHSDR3 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vhsDetection VHSv20120926 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vhsDetection VHSv20130417 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vhsDetection VHSv20140409 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vhsDetection VHSv20150108 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err videoDetection VIDEODR2 Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err videoDetection VIDEODR3 Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err videoDetection VIDEODR4 Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err videoDetection VIDEOv20100513 Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err videoDetection VIDEOv20111208 Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vikingDetection VIKINGDR2 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vikingDetection VIKINGDR3 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vikingDetection VIKINGDR4 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vikingDetection VIKINGv20110714 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vikingDetection VIKINGv20111019 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vikingDetection VIKINGv20130417 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vikingDetection VIKINGv20140402 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vikingDetection VIKINGv20150421 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCDR1 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCDR2 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCDR3 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCv20110816 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCv20110909 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCv20120126 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCv20121128 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCv20130304 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCv20130805 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCv20140428 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCv20140903 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vmcDetection VMCv20150309 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vvvDetection VVVDR1 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vvvDetection VVVDR2 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux11err vvvListRemeasurement VVVv20110718 Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} real 4 ADU   stat.error
aperFlux12 svNgc253Detection SVNGC253v20100429 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 svOrionDetection SVORIONv20100429 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 ultravistaDetection ULTRAVISTAv20100429 default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vhsDetection VHSDR1 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vhsDetection VHSDR2 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vhsDetection VHSDR3 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vhsDetection VHSv20120926 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vhsDetection VHSv20130417 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vhsDetection VHSv20140409 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vhsDetection VHSv20150108 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 videoDetection VIDEODR2 default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 videoDetection VIDEODR3 default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 videoDetection VIDEODR4 default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 videoDetection VIDEOv20100513 default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 videoDetection VIDEOv20111208 default aperture flux 12, no aperture correction applied (SE: FLUX_APER12) {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vikingDetection VIKINGDR2 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vikingDetection VIKINGDR3 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vikingDetection VIKINGDR4 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vikingDetection VIKINGv20110714 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vikingDetection VIKINGv20111019 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vikingDetection VIKINGv20130417 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vikingDetection VIKINGv20140402 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vikingDetection VIKINGv20150421 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vmcDetection VMCDR1 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vmcDetection VMCDR2 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vmcDetection VMCDR3 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vmcDetection VMCv20110816 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vmcDetection VMCv20110909 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vmcDetection VMCv20120126 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vmcDetection VMCv20121128 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vmcDetection VMCv20130304 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vmcDetection VMCv20130805 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vmcDetection VMCv20140428 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vmcDetection VMCv20140903 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vmcDetection VMCv20150309 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vvvDetection VVVDR1 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vvvDetection VVVDR2 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux12 vvvDetection, vvvListRemeasurement VVVv20100531 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12 vvvListRemeasurement VVVv20110718 default aperture flux 12 {catalogue TType keyword: Aper_flux_12}
10 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux12err svNgc253Detection SVNGC253v20100429 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err svOrionDetection SVORIONv20100429 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vhsDetection VHSDR1 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vhsDetection VHSDR2 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vhsDetection VHSDR3 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vhsDetection VHSv20120926 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vhsDetection VHSv20130417 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vhsDetection VHSv20140409 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vhsDetection VHSv20150108 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err videoDetection VIDEODR2 Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err videoDetection VIDEODR3 Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err videoDetection VIDEODR4 Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err videoDetection VIDEOv20100513 Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err videoDetection VIDEOv20111208 Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vikingDetection VIKINGDR2 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vikingDetection VIKINGDR3 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vikingDetection VIKINGDR4 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vikingDetection VIKINGv20110714 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vikingDetection VIKINGv20111019 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vikingDetection VIKINGv20130417 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vikingDetection VIKINGv20140402 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vikingDetection VIKINGv20150421 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCDR1 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCDR2 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCDR3 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCv20110816 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCv20110909 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCv20120126 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCv20121128 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCv20130304 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCv20130805 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCv20140428 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCv20140903 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vmcDetection VMCv20150309 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vvvDetection VVVDR1 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vvvDetection VVVDR2 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux12err vvvListRemeasurement VVVv20110718 Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} real 4 ADU   stat.error
aperFlux13 svNgc253Detection SVNGC253v20100429 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 svOrionDetection SVORIONv20100429 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 ultravistaDetection ULTRAVISTAv20100429 default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vhsDetection VHSDR1 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vhsDetection VHSDR2 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vhsDetection VHSDR3 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vhsDetection VHSv20120926 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vhsDetection VHSv20130417 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vhsDetection VHSv20140409 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vhsDetection VHSv20150108 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 videoDetection VIDEODR2 default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 videoDetection VIDEODR3 default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 videoDetection VIDEODR4 default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 videoDetection VIDEOv20100513 default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 videoDetection VIDEOv20111208 default aperture flux 13, no aperture correction applied (SE: FLUX_APER13) {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vikingDetection VIKINGDR2 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vikingDetection VIKINGDR3 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vikingDetection VIKINGDR4 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vikingDetection VIKINGv20110714 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vikingDetection VIKINGv20111019 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vikingDetection VIKINGv20130417 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vikingDetection VIKINGv20140402 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vikingDetection VIKINGv20150421 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vmcDetection VMCDR1 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vmcDetection VMCDR2 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vmcDetection VMCDR3 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vmcDetection VMCv20110816 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vmcDetection VMCv20110909 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vmcDetection VMCv20120126 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vmcDetection VMCv20121128 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vmcDetection VMCv20130304 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vmcDetection VMCv20130805 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vmcDetection VMCv20140428 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vmcDetection VMCv20140903 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vmcDetection VMCv20150309 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vvvDetection VVVDR1 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vvvDetection VVVDR2 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux13 vvvDetection, vvvListRemeasurement VVVv20100531 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13 vvvListRemeasurement VVVv20110718 default aperture flux 13 {catalogue TType keyword: Aper_flux_13}
12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux13err svNgc253Detection SVNGC253v20100429 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err svOrionDetection SVORIONv20100429 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vhsDetection VHSDR1 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vhsDetection VHSDR2 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vhsDetection VHSDR3 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vhsDetection VHSv20120926 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vhsDetection VHSv20130417 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vhsDetection VHSv20140409 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vhsDetection VHSv20150108 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err videoDetection VIDEODR2 Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err videoDetection VIDEODR3 Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err videoDetection VIDEODR4 Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err videoDetection VIDEOv20100513 Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err videoDetection VIDEOv20111208 Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vikingDetection VIKINGDR2 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vikingDetection VIKINGDR3 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vikingDetection VIKINGDR4 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vikingDetection VIKINGv20110714 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vikingDetection VIKINGv20111019 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vikingDetection VIKINGv20130417 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vikingDetection VIKINGv20140402 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vikingDetection VIKINGv20150421 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCDR1 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCDR2 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCDR3 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCv20110816 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCv20110909 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCv20120126 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCv20121128 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCv20130304 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCv20130805 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCv20140428 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCv20140903 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vmcDetection VMCv20150309 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vvvDetection VVVDR1 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vvvDetection VVVDR2 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux13err vvvListRemeasurement VVVv20110718 Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} real 4 ADU   stat.error
aperFlux1err svNgc253Detection SVNGC253v20100429 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err svOrionDetection SVORIONv20100429 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vhsDetection VHSDR1 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vhsDetection VHSDR2 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vhsDetection VHSDR3 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vhsDetection VHSv20120926 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vhsDetection VHSv20130417 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vhsDetection VHSv20140409 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vhsDetection VHSv20150108 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err videoDetection VIDEODR2 Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err videoDetection VIDEODR3 Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err videoDetection VIDEODR4 Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err videoDetection VIDEOv20100513 Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err videoDetection VIDEOv20111208 Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vikingDetection VIKINGDR2 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vikingDetection VIKINGDR3 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vikingDetection VIKINGDR4 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vikingDetection VIKINGv20110714 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vikingDetection VIKINGv20111019 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vikingDetection VIKINGv20130417 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vikingDetection VIKINGv20140402 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vikingDetection VIKINGv20150421 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCDR1 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCDR2 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCDR3 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCv20110816 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCv20110909 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCv20120126 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCv20121128 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCv20130304 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCv20130805 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCv20140428 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCv20140903 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vmcDetection VMCv20150309 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vvvDetection VVVDR1 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vvvDetection VVVDR2 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux1err vvvListRemeasurement VVVv20110718 Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} real 4 ADU   stat.error
aperFlux2 svNgc253Detection SVNGC253v20100429 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 svOrionDetection SVORIONv20100429 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 ultravistaDetection ULTRAVISTAv20100429 Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vhsDetection VHSDR1 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vhsDetection VHSDR2 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vhsDetection VHSDR3 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vhsDetection VHSv20120926 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vhsDetection VHSv20130417 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vhsDetection VHSv20140409 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vhsDetection VHSv20150108 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 videoDetection VIDEODR2 Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 videoDetection VIDEODR3 Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 videoDetection VIDEODR4 Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 videoDetection VIDEOv20100513 Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 videoDetection VIDEOv20111208 Default aperture flux 2, no aperture correction applied (SE: FLUX_APER2) {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vikingDetection VIKINGDR2 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vikingDetection VIKINGDR3 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vikingDetection VIKINGDR4 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vikingDetection VIKINGv20110714 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vikingDetection VIKINGv20111019 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vikingDetection VIKINGv20130417 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vikingDetection VIKINGv20140402 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vikingDetection VIKINGv20150421 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vmcDetection VMCDR1 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vmcDetection VMCDR2 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vmcDetection VMCDR3 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vmcDetection VMCv20110816 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vmcDetection VMCv20110909 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vmcDetection VMCv20120126 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vmcDetection VMCv20121128 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vmcDetection VMCv20130304 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vmcDetection VMCv20130805 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vmcDetection VMCv20140428 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vmcDetection VMCv20140903 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vmcDetection VMCv20150309 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vvvDetection VVVDR1 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vvvDetection VVVDR2 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count
aperFlux2 vvvDetection VVVv20100531 Default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU   phot.count;em.opt
aperFlux2 vvvListRemeasurement VVVv20100531 default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux2 vvvListRemeasurement VVVv20110718 default aperture flux 2 {catalogue TType keyword: Aper_flux_2}
1/√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux2err svNgc253Detection SVNGC253v20100429 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err svOrionDetection SVORIONv20100429 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vhsDetection VHSDR1 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vhsDetection VHSDR2 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vhsDetection VHSDR3 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vhsDetection VHSv20120926 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vhsDetection VHSv20130417 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vhsDetection VHSv20140409 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vhsDetection VHSv20150108 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err videoDetection VIDEODR2 Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err videoDetection VIDEODR3 Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err videoDetection VIDEODR4 Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err videoDetection VIDEOv20100513 Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err videoDetection VIDEOv20111208 Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vikingDetection VIKINGDR2 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vikingDetection VIKINGDR3 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vikingDetection VIKINGDR4 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vikingDetection VIKINGv20110714 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vikingDetection VIKINGv20111019 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vikingDetection VIKINGv20130417 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vikingDetection VIKINGv20140402 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vikingDetection VIKINGv20150421 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCDR1 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCDR2 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCDR3 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCv20110816 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCv20110909 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCv20120126 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCv20121128 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCv20130304 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCv20130805 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCv20140428 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCv20140903 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vmcDetection VMCv20150309 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vvvDetection VVVDR1 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vvvDetection VVVDR2 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux2err vvvListRemeasurement VVVv20110718 Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} real 4 ADU   stat.error
aperFlux3 svNgc253Detection SVNGC253v20100429 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 svOrionDetection SVORIONv20100429 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 ultravistaDetection ULTRAVISTAv20100429 default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vhsDetection VHSDR1 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vhsDetection VHSDR2 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vhsDetection VHSDR3 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vhsDetection VHSv20120926 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vhsDetection VHSv20130417 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vhsDetection VHSv20140409 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vhsDetection VHSv20150108 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 videoDetection VIDEODR2 default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 videoDetection VIDEODR3 default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 videoDetection VIDEODR4 default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 videoDetection VIDEOv20100513 default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 videoDetection VIDEOv20111208 default aperture flux 3, no aperture correction applied (SE: FLUX_APER3) {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vikingDetection VIKINGDR2 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vikingDetection VIKINGDR3 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vikingDetection VIKINGDR4 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vikingDetection VIKINGv20110714 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vikingDetection VIKINGv20111019 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vikingDetection VIKINGv20130417 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vikingDetection VIKINGv20140402 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vikingDetection VIKINGv20150421 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vmcDetection VMCDR1 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vmcDetection VMCDR2 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vmcDetection VMCDR3 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vmcDetection VMCv20110816 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vmcDetection VMCv20110909 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vmcDetection VMCv20120126 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vmcDetection VMCv20121128 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vmcDetection VMCv20130304 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vmcDetection VMCv20130805 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vmcDetection VMCv20140428 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vmcDetection VMCv20140903 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vmcDetection VMCv20150309 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vvvDetection VVVDR1 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vvvDetection VVVDR2 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux3 vvvDetection, vvvListRemeasurement VVVv20100531 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3 vvvListRemeasurement VVVv20110718 default aperture flux 3 {catalogue TType keyword: Aper_flux_3}
rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux3err svNgc253Detection SVNGC253v20100429 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err svOrionDetection SVORIONv20100429 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vhsDetection VHSDR1 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vhsDetection VHSDR2 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vhsDetection VHSDR3 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vhsDetection VHSv20120926 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vhsDetection VHSv20130417 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vhsDetection VHSv20140409 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vhsDetection VHSv20150108 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err videoDetection VIDEODR2 Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err videoDetection VIDEODR3 Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err videoDetection VIDEODR4 Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err videoDetection VIDEOv20100513 Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err videoDetection VIDEOv20111208 Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vikingDetection VIKINGDR2 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vikingDetection VIKINGDR3 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vikingDetection VIKINGDR4 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vikingDetection VIKINGv20110714 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vikingDetection VIKINGv20111019 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vikingDetection VIKINGv20130417 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vikingDetection VIKINGv20140402 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vikingDetection VIKINGv20150421 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCDR1 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCDR2 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCDR3 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCv20110816 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCv20110909 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCv20120126 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCv20121128 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCv20130304 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCv20130805 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCv20140428 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCv20140903 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vmcDetection VMCv20150309 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vvvDetection VVVDR1 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vvvDetection VVVDR2 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux3err vvvListRemeasurement VVVv20110718 Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} real 4 ADU   stat.error
aperFlux4 svNgc253Detection SVNGC253v20100429 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 svOrionDetection SVORIONv20100429 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 ultravistaDetection ULTRAVISTAv20100429 default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vhsDetection VHSDR1 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vhsDetection VHSDR2 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vhsDetection VHSDR3 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vhsDetection VHSv20120926 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vhsDetection VHSv20130417 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vhsDetection VHSv20140409 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vhsDetection VHSv20150108 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 videoDetection VIDEODR2 default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 videoDetection VIDEODR3 default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 videoDetection VIDEODR4 default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 videoDetection VIDEOv20100513 default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 videoDetection VIDEOv20111208 default aperture flux 4, no aperture correction applied (SE: FLUX_APER4) {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vikingDetection VIKINGDR2 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vikingDetection VIKINGDR3 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vikingDetection VIKINGDR4 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vikingDetection VIKINGv20110714 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vikingDetection VIKINGv20111019 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vikingDetection VIKINGv20130417 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vikingDetection VIKINGv20140402 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vikingDetection VIKINGv20150421 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vmcDetection VMCDR1 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vmcDetection VMCDR2 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vmcDetection VMCDR3 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vmcDetection VMCv20110816 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vmcDetection VMCv20110909 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vmcDetection VMCv20120126 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vmcDetection VMCv20121128 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vmcDetection VMCv20130304 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vmcDetection VMCv20130805 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vmcDetection VMCv20140428 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vmcDetection VMCv20140903 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vmcDetection VMCv20150309 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vvvDetection VVVDR1 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vvvDetection VVVDR2 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux4 vvvDetection, vvvListRemeasurement VVVv20100531 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4 vvvListRemeasurement VVVv20110718 default aperture flux 4 {catalogue TType keyword: Aper_flux_4}
√2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux4err svNgc253Detection SVNGC253v20100429 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err svOrionDetection SVORIONv20100429 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vhsDetection VHSDR1 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vhsDetection VHSDR2 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vhsDetection VHSDR3 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vhsDetection VHSv20120926 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vhsDetection VHSv20130417 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vhsDetection VHSv20140409 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vhsDetection VHSv20150108 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err videoDetection VIDEODR2 Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err videoDetection VIDEODR3 Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err videoDetection VIDEODR4 Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err videoDetection VIDEOv20100513 Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err videoDetection VIDEOv20111208 Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vikingDetection VIKINGDR2 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vikingDetection VIKINGDR3 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vikingDetection VIKINGDR4 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vikingDetection VIKINGv20110714 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vikingDetection VIKINGv20111019 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vikingDetection VIKINGv20130417 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vikingDetection VIKINGv20140402 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vikingDetection VIKINGv20150421 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCDR1 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCDR2 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCDR3 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCv20110816 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCv20110909 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCv20120126 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCv20121128 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCv20130304 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCv20130805 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCv20140428 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCv20140903 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vmcDetection VMCv20150309 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vvvDetection VVVDR1 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vvvDetection VVVDR2 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux4err vvvListRemeasurement VVVv20110718 Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} real 4 ADU   stat.error
aperFlux5 svNgc253Detection SVNGC253v20100429 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 svOrionDetection SVORIONv20100429 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 ultravistaDetection ULTRAVISTAv20100429 default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vhsDetection VHSDR1 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vhsDetection VHSDR2 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vhsDetection VHSDR3 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vhsDetection VHSv20120926 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vhsDetection VHSv20130417 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vhsDetection VHSv20140409 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vhsDetection VHSv20150108 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 videoDetection VIDEODR2 default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 videoDetection VIDEODR3 default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 videoDetection VIDEODR4 default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 videoDetection VIDEOv20100513 default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 videoDetection VIDEOv20111208 default aperture flux 5, no aperture correction applied (SE: FLUX_APER5) {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vikingDetection VIKINGDR2 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vikingDetection VIKINGDR3 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vikingDetection VIKINGDR4 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vikingDetection VIKINGv20110714 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vikingDetection VIKINGv20111019 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vikingDetection VIKINGv20130417 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vikingDetection VIKINGv20140402 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vikingDetection VIKINGv20150421 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vmcDetection VMCDR1 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vmcDetection VMCDR2 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vmcDetection VMCDR3 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vmcDetection VMCv20110816 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vmcDetection VMCv20110909 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vmcDetection VMCv20120126 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vmcDetection VMCv20121128 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vmcDetection VMCv20130304 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vmcDetection VMCv20130805 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vmcDetection VMCv20140428 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vmcDetection VMCv20140903 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vmcDetection VMCv20150309 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vvvDetection VVVDR1 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vvvDetection VVVDR2 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux5 vvvDetection, vvvListRemeasurement VVVv20100531 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5 vvvListRemeasurement VVVv20110718 default aperture flux 5 {catalogue TType keyword: Aper_flux_5}
2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux5err svNgc253Detection SVNGC253v20100429 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err svOrionDetection SVORIONv20100429 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vhsDetection VHSDR1 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vhsDetection VHSDR2 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vhsDetection VHSDR3 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vhsDetection VHSv20120926 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vhsDetection VHSv20130417 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vhsDetection VHSv20140409 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vhsDetection VHSv20150108 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err videoDetection VIDEODR2 Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err videoDetection VIDEODR3 Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err videoDetection VIDEODR4 Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err videoDetection VIDEOv20100513 Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err videoDetection VIDEOv20111208 Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vikingDetection VIKINGDR2 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vikingDetection VIKINGDR3 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vikingDetection VIKINGDR4 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vikingDetection VIKINGv20110714 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vikingDetection VIKINGv20111019 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vikingDetection VIKINGv20130417 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vikingDetection VIKINGv20140402 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vikingDetection VIKINGv20150421 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCDR1 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCDR2 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCDR3 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCv20110816 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCv20110909 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCv20120126 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCv20121128 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCv20130304 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCv20130805 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCv20140428 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCv20140903 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vmcDetection VMCv20150309 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vvvDetection VVVDR1 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vvvDetection VVVDR2 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux5err vvvListRemeasurement VVVv20110718 Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} real 4 ADU   stat.error
aperFlux6 svNgc253Detection SVNGC253v20100429 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 svOrionDetection SVORIONv20100429 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 ultravistaDetection ULTRAVISTAv20100429 default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vhsDetection VHSDR1 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vhsDetection VHSDR2 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vhsDetection VHSDR3 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vhsDetection VHSv20120926 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vhsDetection VHSv20130417 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vhsDetection VHSv20140409 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vhsDetection VHSv20150108 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 videoDetection VIDEODR2 default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 videoDetection VIDEODR3 default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 videoDetection VIDEODR4 default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 videoDetection VIDEOv20100513 default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 videoDetection VIDEOv20111208 default aperture flux 6, no aperture correction applied (SE: FLUX_APER6) {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vikingDetection VIKINGDR2 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vikingDetection VIKINGDR3 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vikingDetection VIKINGDR4 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vikingDetection VIKINGv20110714 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vikingDetection VIKINGv20111019 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vikingDetection VIKINGv20130417 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vikingDetection VIKINGv20140402 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vikingDetection VIKINGv20150421 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vmcDetection VMCDR1 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vmcDetection VMCDR2 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vmcDetection VMCDR3 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vmcDetection VMCv20110816 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vmcDetection VMCv20110909 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vmcDetection VMCv20120126 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vmcDetection VMCv20121128 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vmcDetection VMCv20130304 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vmcDetection VMCv20130805 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vmcDetection VMCv20140428 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vmcDetection VMCv20140903 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vmcDetection VMCv20150309 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vvvDetection VVVDR1 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vvvDetection VVVDR2 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux6 vvvDetection, vvvListRemeasurement VVVv20100531 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6 vvvListRemeasurement VVVv20110718 default aperture flux 6 {catalogue TType keyword: Aper_flux_6}
2√2 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux6err svNgc253Detection SVNGC253v20100429 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err svOrionDetection SVORIONv20100429 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vhsDetection VHSDR1 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vhsDetection VHSDR2 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vhsDetection VHSDR3 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vhsDetection VHSv20120926 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vhsDetection VHSv20130417 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vhsDetection VHSv20140409 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vhsDetection VHSv20150108 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err videoDetection VIDEODR2 Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err videoDetection VIDEODR3 Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err videoDetection VIDEODR4 Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err videoDetection VIDEOv20100513 Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err videoDetection VIDEOv20111208 Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vikingDetection VIKINGDR2 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vikingDetection VIKINGDR3 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vikingDetection VIKINGDR4 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vikingDetection VIKINGv20110714 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vikingDetection VIKINGv20111019 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vikingDetection VIKINGv20130417 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vikingDetection VIKINGv20140402 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vikingDetection VIKINGv20150421 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCDR1 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCDR2 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCDR3 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCv20110816 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCv20110909 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCv20120126 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCv20121128 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCv20130304 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCv20130805 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCv20140428 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCv20140903 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vmcDetection VMCv20150309 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vvvDetection VVVDR1 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vvvDetection VVVDR2 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux6err vvvListRemeasurement VVVv20110718 Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} real 4 ADU   stat.error
aperFlux7 svNgc253Detection SVNGC253v20100429 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 svOrionDetection SVORIONv20100429 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 ultravistaDetection ULTRAVISTAv20100429 default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vhsDetection VHSDR1 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vhsDetection VHSDR2 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vhsDetection VHSDR3 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vhsDetection VHSv20120926 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vhsDetection VHSv20130417 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vhsDetection VHSv20140409 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vhsDetection VHSv20150108 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 videoDetection VIDEODR2 default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 videoDetection VIDEODR3 default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 videoDetection VIDEODR4 default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 videoDetection VIDEOv20100513 default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 videoDetection VIDEOv20111208 default aperture flux 7, no aperture correction applied (SE: FLUX_APER7) {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vikingDetection VIKINGDR2 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vikingDetection VIKINGDR3 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vikingDetection VIKINGDR4 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vikingDetection VIKINGv20110714 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vikingDetection VIKINGv20111019 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vikingDetection VIKINGv20130417 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vikingDetection VIKINGv20140402 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vikingDetection VIKINGv20150421 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vmcDetection VMCDR1 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vmcDetection VMCDR2 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vmcDetection VMCDR3 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vmcDetection VMCv20110816 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vmcDetection VMCv20110909 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vmcDetection VMCv20120126 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vmcDetection VMCv20121128 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vmcDetection VMCv20130304 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vmcDetection VMCv20130805 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vmcDetection VMCv20140428 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vmcDetection VMCv20140903 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vmcDetection VMCv20150309 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vvvDetection VVVDR1 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vvvDetection VVVDR2 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux7 vvvDetection, vvvListRemeasurement VVVv20100531 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7 vvvListRemeasurement VVVv20110718 default aperture flux 7 {catalogue TType keyword: Aper_flux_7}
4 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux7err svNgc253Detection SVNGC253v20100429 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err svOrionDetection SVORIONv20100429 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vhsDetection VHSDR1 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vhsDetection VHSDR2 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vhsDetection VHSDR3 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vhsDetection VHSv20120926 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vhsDetection VHSv20130417 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vhsDetection VHSv20140409 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vhsDetection VHSv20150108 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err videoDetection VIDEODR2 Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err videoDetection VIDEODR3 Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err videoDetection VIDEODR4 Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err videoDetection VIDEOv20100513 Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err videoDetection VIDEOv20111208 Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vikingDetection VIKINGDR2 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vikingDetection VIKINGDR3 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vikingDetection VIKINGDR4 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vikingDetection VIKINGv20110714 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vikingDetection VIKINGv20111019 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vikingDetection VIKINGv20130417 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vikingDetection VIKINGv20140402 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vikingDetection VIKINGv20150421 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCDR1 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCDR2 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCDR3 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCv20110816 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCv20110909 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCv20120126 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCv20121128 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCv20130304 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCv20130805 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCv20140428 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCv20140903 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vmcDetection VMCv20150309 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vvvDetection VVVDR1 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vvvDetection VVVDR2 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux7err vvvListRemeasurement VVVv20110718 Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} real 4 ADU   stat.error
aperFlux8 svNgc253Detection SVNGC253v20100429 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 svOrionDetection SVORIONv20100429 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 ultravistaDetection ULTRAVISTAv20100429 default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vhsDetection VHSDR1 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vhsDetection VHSDR2 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vhsDetection VHSDR3 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vhsDetection VHSv20120926 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vhsDetection VHSv20130417 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vhsDetection VHSv20140409 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vhsDetection VHSv20150108 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 videoDetection VIDEODR2 default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 videoDetection VIDEODR3 default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 videoDetection VIDEODR4 default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 videoDetection VIDEOv20100513 default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 videoDetection VIDEOv20111208 default aperture flux 8, no aperture correction applied (SE: FLUX_APER8) {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vikingDetection VIKINGDR2 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vikingDetection VIKINGDR3 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vikingDetection VIKINGDR4 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vikingDetection VIKINGv20110714 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vikingDetection VIKINGv20111019 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vikingDetection VIKINGv20130417 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vikingDetection VIKINGv20140402 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vikingDetection VIKINGv20150421 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vmcDetection VMCDR1 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vmcDetection VMCDR2 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vmcDetection VMCDR3 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vmcDetection VMCv20110816 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vmcDetection VMCv20110909 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vmcDetection VMCv20120126 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vmcDetection VMCv20121128 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vmcDetection VMCv20130304 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vmcDetection VMCv20130805 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vmcDetection VMCv20140428 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vmcDetection VMCv20140903 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vmcDetection VMCv20150309 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vvvDetection VVVDR1 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vvvDetection VVVDR2 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux8 vvvDetection, vvvListRemeasurement VVVv20100531 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8 vvvListRemeasurement VVVv20110718 default aperture flux 8 {catalogue TType keyword: Aper_flux_8}
5 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux8err svNgc253Detection SVNGC253v20100429 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err svOrionDetection SVORIONv20100429 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vhsDetection VHSDR1 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vhsDetection VHSDR2 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vhsDetection VHSDR3 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vhsDetection VHSv20120926 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vhsDetection VHSv20130417 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vhsDetection VHSv20140409 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vhsDetection VHSv20150108 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err videoDetection VIDEODR2 Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err videoDetection VIDEODR3 Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err videoDetection VIDEODR4 Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err videoDetection VIDEOv20100513 Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err videoDetection VIDEOv20111208 Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vikingDetection VIKINGDR2 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vikingDetection VIKINGDR3 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vikingDetection VIKINGDR4 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vikingDetection VIKINGv20110714 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vikingDetection VIKINGv20111019 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vikingDetection VIKINGv20130417 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vikingDetection VIKINGv20140402 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vikingDetection VIKINGv20150421 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCDR1 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCDR2 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCDR3 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCv20110816 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCv20110909 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCv20120126 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCv20121128 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCv20130304 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCv20130805 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCv20140428 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCv20140903 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vmcDetection VMCv20150309 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vvvDetection VVVDR1 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vvvDetection VVVDR2 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux8err vvvListRemeasurement VVVv20110718 Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} real 4 ADU   stat.error
aperFlux9 svNgc253Detection SVNGC253v20100429 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 svOrionDetection SVORIONv20100429 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 ultravistaDetection ULTRAVISTAv20100429 default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vhsDetection VHSDR1 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vhsDetection VHSDR2 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vhsDetection VHSDR3 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vhsDetection VHSv20120926 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vhsDetection VHSv20130417 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vhsDetection VHSv20140409 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vhsDetection VHSv20150108 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 videoDetection VIDEODR2 default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 videoDetection VIDEODR3 default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 videoDetection VIDEODR4 default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 videoDetection VIDEOv20100513 default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 videoDetection VIDEOv20111208 default aperture flux 9, no aperture correction applied (SE: FLUX_APER9) {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vikingDetection VIKINGDR2 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vikingDetection VIKINGDR3 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vikingDetection VIKINGDR4 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vikingDetection VIKINGv20110714 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vikingDetection VIKINGv20111019 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vikingDetection VIKINGv20130417 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vikingDetection VIKINGv20140402 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vikingDetection VIKINGv20150421 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vmcDetection VMCDR1 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vmcDetection VMCDR2 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vmcDetection VMCDR3 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vmcDetection VMCv20110816 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vmcDetection VMCv20110909 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vmcDetection VMCv20120126 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vmcDetection VMCv20121128 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vmcDetection VMCv20130304 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vmcDetection VMCv20130805 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vmcDetection VMCv20140428 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vmcDetection VMCv20140903 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vmcDetection VMCv20150309 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vvvDetection VVVDR1 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vvvDetection VVVDR2 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count
aperFlux9 vvvDetection, vvvListRemeasurement VVVv20100531 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9 vvvListRemeasurement VVVv20110718 default aperture flux 9 {catalogue TType keyword: Aper_flux_9}
6 × rcore (see glossary entry for aperFlux1)
real 4 ADU aperture phot.count;em.opt
aperFlux9err svNgc253Detection SVNGC253v20100429 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err svOrionDetection SVORIONv20100429 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err ultravistaDetection ULTRAVISTAv20100429 Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vhsDetection VHSDR1 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vhsDetection VHSDR2 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vhsDetection VHSDR3 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vhsDetection VHSv20120926 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vhsDetection VHSv20130417 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vhsDetection VHSv20140409 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vhsDetection VHSv20150108 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err videoDetection VIDEODR2 Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err videoDetection VIDEODR3 Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err videoDetection VIDEODR4 Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err videoDetection VIDEOv20100513 Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err videoDetection VIDEOv20111208 Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vikingDetection VIKINGDR2 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vikingDetection VIKINGDR3 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vikingDetection VIKINGDR4 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vikingDetection VIKINGv20110714 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vikingDetection VIKINGv20111019 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vikingDetection VIKINGv20130417 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vikingDetection VIKINGv20140402 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vikingDetection VIKINGv20150421 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCDR1 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCDR2 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCDR3 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCv20110816 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCv20110909 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCv20120126 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCv20121128 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCv20130304 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCv20130805 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCv20140428 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCv20140903 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vmcDetection VMCv20150309 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vvvDetection VVVDR1 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vvvDetection VVVDR2 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vvvDetection, vvvListRemeasurement VVVv20100531 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperFlux9err vvvListRemeasurement VVVv20110718 Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} real 4 ADU   stat.error
aperMag1 svNgc253Detection SVNGC253v20100429 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
aperMag1 svOrionDetection SVORIONv20100429 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
aperMag1 ultravistaDetection ULTRAVISTAv20100429 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
aperMag1 vhsDetection VHSDR1 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vhsDetection VHSDR2 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vhsDetection VHSDR3 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vhsDetection VHSv20120926 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vhsDetection VHSv20130417 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vhsDetection VHSv20140409 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vhsDetection VHSv20150108 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 videoDetection VIDEODR2 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
aperMag1 videoDetection VIDEODR3 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
aperMag1 videoDetection VIDEODR4 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
aperMag1 videoDetection VIDEOv20100513 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
aperMag1 videoDetection VIDEOv20111208 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
aperMag1 vikingDetection VIKINGDR2 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vikingDetection VIKINGDR3 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vikingDetection VIKINGDR4 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vikingDetection VIKINGv20110714 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vikingDetection VIKINGv20111019 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vikingDetection VIKINGv20130417 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vikingDetection VIKINGv20140402 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vikingDetection VIKINGv20150421 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCDR1 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCDR2 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCDR3 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCv20110816 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCv20110909 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCv20120126 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCv20121128 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCv20130304 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCv20130805 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCv20140428 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCv20140903 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vmcDetection VMCv20150309 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vvvDetection VVVDR1 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vvvDetection VVVDR2 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag1 vvvDetection, vvvListRemeasurement VVVv20100531 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
aperMag1 vvvListRemeasurement VVVv20110718 Calibrated and corrected aperture magnitude 1 real 4 mag   phot.mag
aperMag10 svNgc253Detection SVNGC253v20100429 Calibrated and corrected aperture magnitude 10 real 4 mag   phot.mag
aperMag10 svOrionDetection SVORIONv20100429 Calibrated and corrected aperture magnitude 10 real 4 mag   phot.mag
aperMag10 ultravistaDetection ULTRAVISTAv20100429 Calibrated and corrected aperture magnitude 10 real 4 mag   phot.mag
aperMag10 vhsDetection VHSDR1 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vhsDetection VHSDR2 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vhsDetection VHSDR3 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vhsDetection VHSv20120926 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vhsDetection VHSv20130417 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vhsDetection VHSv20140409 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vhsDetection VHSv20150108 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 videoDetection VIDEODR2 Calibrated and corrected aperture magnitude 10 real 4 mag   phot.mag
aperMag10 videoDetection VIDEODR3 Calibrated and corrected aperture magnitude 10 real 4 mag   phot.mag
aperMag10 videoDetection VIDEODR4 Calibrated and corrected aperture magnitude 10 real 4 mag   phot.mag
aperMag10 videoDetection VIDEOv20100513 Calibrated and corrected aperture magnitude 10 real 4 mag   phot.mag
aperMag10 videoDetection VIDEOv20111208 Calibrated and corrected aperture magnitude 10 real 4 mag   phot.mag
aperMag10 vikingDetection VIKINGDR2 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vikingDetection VIKINGDR3 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vikingDetection VIKINGDR4 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vikingDetection VIKINGv20110714 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vikingDetection VIKINGv20111019 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vikingDetection VIKINGv20130417 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vikingDetection VIKINGv20140402 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vikingDetection VIKINGv20150421 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCDR1 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCDR2 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCDR3 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCv20110816 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCv20110909 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCv20120126 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCv20121128 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCv20130304 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCv20130805 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCv20140428 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCv20140903 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vmcDetection VMCv20150309 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vvvDetection VVVDR1 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vvvDetection VVVDR2 Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag10 vvvDetection, vvvListRemeasurement VVVv20100531 Calibrated and corrected aperture magnitude 10 real 4 mag   phot.mag
aperMag10 vvvListRemeasurement VVVv20110718 Calibrated and corrected aperture magnitude 10 real 4 mag   phot.mag
aperMag10err svNgc253Detection SVNGC253v20100429 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err svOrionDetection SVORIONv20100429 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err ultravistaDetection ULTRAVISTAv20100429 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vhsDetection VHSDR1 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vhsDetection VHSDR2 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vhsDetection VHSDR3 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vhsDetection VHSv20120926 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vhsDetection VHSv20130417 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vhsDetection VHSv20140409 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vhsDetection VHSv20150108 Error in calibrated aperture magnitude 10 real 4 mag   stat.error;phot.mag
aperMag10err videoDetection VIDEODR2 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err videoDetection VIDEODR3 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err videoDetection VIDEODR4 Error in calibrated aperture magnitude 10 real 4 mag   stat.error;phot.mag
aperMag10err videoDetection VIDEOv20100513 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err videoDetection VIDEOv20111208 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vikingDetection VIKINGDR2 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vikingDetection VIKINGDR3 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vikingDetection VIKINGDR4 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vikingDetection VIKINGv20110714 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vikingDetection VIKINGv20111019 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vikingDetection VIKINGv20130417 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vikingDetection VIKINGv20140402 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vikingDetection VIKINGv20150421 Error in calibrated aperture magnitude 10 real 4 mag   stat.error;phot.mag
aperMag10err vmcDetection VMCDR1 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vmcDetection VMCDR2 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vmcDetection VMCDR3 Error in calibrated aperture magnitude 10 real 4 mag   stat.error;phot.mag
aperMag10err vmcDetection VMCv20110816 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vmcDetection VMCv20110909 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vmcDetection VMCv20120126 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vmcDetection VMCv20121128 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vmcDetection VMCv20130304 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vmcDetection VMCv20130805 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vmcDetection VMCv20140428 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vmcDetection VMCv20140903 Error in calibrated aperture magnitude 10 real 4 mag   stat.error;phot.mag
aperMag10err vmcDetection VMCv20150309 Error in calibrated aperture magnitude 10 real 4 mag   stat.error;phot.mag
aperMag10err vvvDetection VVVDR1 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vvvDetection VVVDR2 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vvvDetection, vvvListRemeasurement VVVv20100531 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag10err vvvListRemeasurement VVVv20110718 Error in calibrated aperture magnitude 10 real 4 mag   stat.error
aperMag11 svNgc253Detection SVNGC253v20100429 Calibrated and corrected aperture magnitude 11 real 4 mag   phot.mag
aperMag11 svOrionDetection SVORIONv20100429 Calibrated and corrected aperture magnitude 11 real 4 mag   phot.mag
aperMag11 ultravistaDetection ULTRAVISTAv20100429 Calibrated and corrected aperture magnitude 11 real 4 mag   phot.mag
aperMag11 vhsDetection VHSDR1 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vhsDetection VHSDR2 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vhsDetection VHSDR3 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vhsDetection VHSv20120926 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vhsDetection VHSv20130417 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vhsDetection VHSv20140409 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vhsDetection VHSv20150108 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 videoDetection VIDEODR2 Calibrated and corrected aperture magnitude 11 real 4 mag   phot.mag
aperMag11 videoDetection VIDEODR3 Calibrated and corrected aperture magnitude 11 real 4 mag   phot.mag
aperMag11 videoDetection VIDEODR4 Calibrated and corrected aperture magnitude 11 real 4 mag   phot.mag
aperMag11 videoDetection VIDEOv20100513 Calibrated and corrected aperture magnitude 11 real 4 mag   phot.mag
aperMag11 videoDetection VIDEOv20111208 Calibrated and corrected aperture magnitude 11 real 4 mag   phot.mag
aperMag11 vikingDetection VIKINGDR2 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vikingDetection VIKINGDR3 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vikingDetection VIKINGDR4 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vikingDetection VIKINGv20110714 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vikingDetection VIKINGv20111019 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vikingDetection VIKINGv20130417 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vikingDetection VIKINGv20140402 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vikingDetection VIKINGv20150421 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCDR1 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCDR2 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCDR3 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCv20110816 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCv20110909 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCv20120126 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCv20121128 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCv20130304 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCv20130805 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCv20140428 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCv20140903 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vmcDetection VMCv20150309 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vvvDetection VVVDR1 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vvvDetection VVVDR2 Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag11 vvvDetection, vvvListRemeasurement VVVv20100531 Calibrated and corrected aperture magnitude 11 real 4 mag   phot.mag
aperMag11 vvvListRemeasurement VVVv20110718 Calibrated and corrected aperture magnitude 11 real 4 mag   phot.mag
aperMag11err svNgc253Detection SVNGC253v20100429 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err svOrionDetection SVORIONv20100429 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err ultravistaDetection ULTRAVISTAv20100429 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vhsDetection VHSDR1 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vhsDetection VHSDR2 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vhsDetection VHSDR3 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vhsDetection VHSv20120926 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vhsDetection VHSv20130417 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vhsDetection VHSv20140409 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vhsDetection VHSv20150108 Error in calibrated aperture magnitude 11 real 4 mag   stat.error;phot.mag
aperMag11err videoDetection VIDEODR2 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err videoDetection VIDEODR3 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err videoDetection VIDEODR4 Error in calibrated aperture magnitude 11 real 4 mag   stat.error;phot.mag
aperMag11err videoDetection VIDEOv20100513 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err videoDetection VIDEOv20111208 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vikingDetection VIKINGDR2 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vikingDetection VIKINGDR3 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vikingDetection VIKINGDR4 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vikingDetection VIKINGv20110714 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vikingDetection VIKINGv20111019 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vikingDetection VIKINGv20130417 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vikingDetection VIKINGv20140402 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vikingDetection VIKINGv20150421 Error in calibrated aperture magnitude 11 real 4 mag   stat.error;phot.mag
aperMag11err vmcDetection VMCDR1 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vmcDetection VMCDR2 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vmcDetection VMCDR3 Error in calibrated aperture magnitude 11 real 4 mag   stat.error;phot.mag
aperMag11err vmcDetection VMCv20110816 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vmcDetection VMCv20110909 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vmcDetection VMCv20120126 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vmcDetection VMCv20121128 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vmcDetection VMCv20130304 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vmcDetection VMCv20130805 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vmcDetection VMCv20140428 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vmcDetection VMCv20140903 Error in calibrated aperture magnitude 11 real 4 mag   stat.error;phot.mag
aperMag11err vmcDetection VMCv20150309 Error in calibrated aperture magnitude 11 real 4 mag   stat.error;phot.mag
aperMag11err vvvDetection VVVDR1 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vvvDetection VVVDR2 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vvvDetection, vvvListRemeasurement VVVv20100531 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag11err vvvListRemeasurement VVVv20110718 Error in calibrated aperture magnitude 11 real 4 mag   stat.error
aperMag12 svNgc253Detection SVNGC253v20100429 Calibrated and corrected aperture magnitude 12 real 4 mag   phot.mag
aperMag12 svOrionDetection SVORIONv20100429 Calibrated and corrected aperture magnitude 12 real 4 mag   phot.mag
aperMag12 ultravistaDetection ULTRAVISTAv20100429 Calibrated and corrected aperture magnitude 12 real 4 mag   phot.mag
aperMag12 vhsDetection VHSDR1 Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag12 vhsDetection VHSDR2 Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. real 4 mag   phot.mag
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate.
aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values.
aperMag12 vhsDetection VHSDR3