A |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified 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 |
|
|
ID_ALTERNATIVE |
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 |
VSASVNGC253 |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VSASVORION |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VSAUltraVISTA |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VSAVHS |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VSAVIDEO |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VSAVIKING |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VSAVMC |
5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} |
real |
4 |
mag |
-0.9999995e9 |
|
abMagLim |
MultiframeDetector |
VSAVVV |
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 |
VSASVNGC253 |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VSASVORION |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VSAUltraVISTA |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VSAVHS |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VSAVIDEO |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VSAVIKING |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VSAVMC |
Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} |
real |
4 |
mag |
-0.9999995e9 |
|
abSatMag |
MultiframeDetector |
VSAVVV |
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 |
VSAQC |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VSASVNGC253 |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VSASVORION |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VSAUltraVISTA |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VSAVHS |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VSAVIDEO |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VSAVIKING |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VSAVMC |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
adjacentFrameTolerance |
Programme |
VSAVVV |
The match tolerance for adjacent frames in the survey |
real |
4 |
Degrees |
|
?? |
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 |
VSASVNGC253 |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VSASVORION |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VSAUltraVISTA |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VSAVHS |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VSAVIDEO |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VSAVIKING |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VSAVMC |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aebv |
Filter |
VSAVVV |
The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. |
real |
4 |
|
-0.9999995e9 |
|
aH |
svNgc253Source |
VSASVNGC253 |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aH |
ultravistaSource |
VSAUltraVISTA |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aH |
ultravistaSource, vhsSource, videoSource, vikingSource |
VSAQC |
The galactic extinction correction in the H band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
air_temp |
twomass_scn |
2MASS |
Air temperature at beginning of scan. |
real |
4 |
degC |
|
PHYS_TEMP_MISC |
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 |
|
|
PHOT_ATM_AIRMASS |
airm |
twomass_sixx2_scn |
2MASS |
beginning airmass of scan |
real |
4 |
|
|
|
aJ |
svNgc253Source |
VSASVNGC253 |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aJ |
ultravistaSource |
VSAUltraVISTA |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aJ |
ultravistaSource, vhsSource, videoSource, vikingSource |
VSAQC |
The galactic extinction correction in the J band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
svNgc253Source |
VSASVNGC253 |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
ultravistaSource |
VSAUltraVISTA |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aKs |
ultravistaSource, vhsSource, videoSource, vikingSource |
VSAQC |
The galactic extinction correction in the Ks band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
amEnd |
Multiframe |
VSASVNGC253 |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amEnd |
Multiframe |
VSASVORION |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amEnd |
Multiframe |
VSAUltraVISTA |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amEnd |
Multiframe |
VSAVHS |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amEnd |
Multiframe |
VSAVIDEO |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amEnd |
Multiframe |
VSAVIKING |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amEnd |
Multiframe |
VSAVMC |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amEnd |
Multiframe |
VSAVVV |
Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amEnd |
ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Airmass at end of observation |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amStart |
Multiframe |
VSASVNGC253 |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amStart |
Multiframe |
VSASVORION |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amStart |
Multiframe |
VSAUltraVISTA |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amStart |
Multiframe |
VSAVHS |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amStart |
Multiframe |
VSAVIDEO |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amStart |
Multiframe |
VSAVIKING |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amStart |
Multiframe |
VSAVMC |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amStart |
Multiframe |
VSAVVV |
Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
amStart |
ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Airmass at start of observation |
real |
4 |
|
-0.9999995e9 |
PHOT_ATM_AIRMASS |
aNb118 |
svNgc253Source |
VSASVNGC253 |
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 |
|
|
CODE_MISC |
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 |
|
|
|
Ap_Rmag |
combo17CDFSSource |
COMBO17 |
aperture magnitude in R |
real |
4 |
mag |
|
|
ApD_Rmag |
combo17CDFSSource |
COMBO17 |
aperture difference of Rmag (=Rmag-Ap_Rmag, zero for point sources) |
real |
4 |
mag |
|
|
aperCor1 |
MultiframeDetector |
VSASVNGC253 |
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 |
VSASVORION |
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 |
VSAUltraVISTA |
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 |
VSAVHS |
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 |
VSAVIDEO |
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 |
VSAVIKING |
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 |
VSAVMC |
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 |
VSAVVV |
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 |
VSASVNGC253 |
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 |
VSASVORION |
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 |
VSAUltraVISTA |
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 |
VSAVHS |
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 |
VSAVIDEO |
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 |
VSAVIKING |
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 |
VSAVMC |
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 |
VSAVVV |
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 |
VSASVNGC253 |
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 |
VSASVORION |
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 |
VSAUltraVISTA |
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 |
VSAVHS |
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 |
VSAVIDEO |
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 |
VSAVIKING |
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 |
VSAVMC |
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 |
VSAVVV |
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 |
VSASVNGC253 |
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 |
VSASVORION |
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 |
VSAUltraVISTA |
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 |
VSAVHS |
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 |
VSAVIDEO |
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 |
VSAVIKING |
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 |
VSAVMC |
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 |
VSAVVV |
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 |
VSASVNGC253 |
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 |
VSASVORION |
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 |
VSAUltraVISTA |
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 |
VSAVHS |
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 |
VSAVIDEO |
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 |
VSAVIKING |
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 |
VSAVMC |
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 |
VSAVVV |
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 |
VSASVNGC253 |
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 |
VSASVORION |
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 |
VSAUltraVISTA |
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 |
VSAVHS |
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 |
VSAVIDEO |
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 |
VSAVIKING |
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 |
VSAVMC |
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 |
VSAVVV |
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 |
VSASVNGC253 |
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 |
VSASVORION |
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 |
VSAUltraVISTA |
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 |
VSAVHS |
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 |
VSAVIDEO |
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 |
VSAVIKING |
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 |
VSAVMC |
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 |
VSAVVV |
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 |
VSASVNGC253 |
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 |
VSASVORION |
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 |
VSAUltraVISTA |
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 |
VSAVHS |
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 |
VSAVIDEO |
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 |
VSAVIKING |
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 |
VSAVMC |
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 |
VSAVVV |
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 |
VSASVNGC253 |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
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 |
VSASVORION |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
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 |
VSAUltraVISTA |
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_INTENSITY_ADU |
Flux vector within fixed circular aperture, but no aperture correction. |
aperFlux1 |
ultravistaDetection, videoDetection |
VSAQC |
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_INTENSITY_ADU |
Flux vector within fixed circular aperture, but no aperture correction. |
aperFlux1 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
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 |
ultravistaListRemeasurement, vhsListRemeasurement, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvListRemeasurement |
VSAQC |
default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
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 |
VSAVHS |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
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, vikingDetection, vmcDetection, vvvDetection |
VSAQC |
Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
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 |
VSASVNGC253 |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux10 |
svOrionDetection |
VSASVORION |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux10 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux10 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux10 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux10 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux10err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux10err |
svOrionDetection |
VSASVORION |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux10err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 10 (SE: FLUXERR_APER10) {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux10err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 10 (SE: FLUXERR_APER10) {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux10err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux10err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux11 |
svNgc253Detection |
VSASVNGC253 |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux11 |
svOrionDetection |
VSASVORION |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux11 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux11 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux11 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux11 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux11err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux11err |
svOrionDetection |
VSASVORION |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux11err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux11err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 11 (SE: FLUXERR_APER11) {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux11err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux11err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux12 |
svNgc253Detection |
VSASVNGC253 |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux12 |
svOrionDetection |
VSASVORION |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux12 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux12 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux12 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux12 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux12err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux12err |
svOrionDetection |
VSASVORION |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux12err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux12err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 12 (SE: FLUXERR_APER12) {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux12err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux12err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux13 |
svNgc253Detection |
VSASVNGC253 |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux13 |
svOrionDetection |
VSASVORION |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux13 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux13 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux13 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux13 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux13err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux13err |
svOrionDetection |
VSASVORION |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux13err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux13err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 13 (SE: FLUXERR_APER13) {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux13err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux13err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux1err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux1err |
svOrionDetection |
VSASVORION |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux1err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux1err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux counts 1 (SE: FLUXERR_APER1) {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux1err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux1err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux2 |
svNgc253Detection |
VSASVNGC253 |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux2 |
svOrionDetection |
VSASVORION |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux2 |
ultravistaDetection |
VSAUltraVISTA |
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_INTENSITY_ADU |
aperFlux2 |
ultravistaDetection, videoDetection |
VSAQC |
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_INTENSITY_ADU |
aperFlux2 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux2 |
ultravistaListRemeasurement, vhsListRemeasurement, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvListRemeasurement |
VSAQC |
default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux2 |
vhsDetection |
VSAVHS |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux2 |
vhsDetection, vikingDetection, vmcDetection, vvvDetection |
VSAQC |
Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux2err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux2err |
svOrionDetection |
VSASVORION |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux2err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux2err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 2 (SE: FLUXERR_APER2) {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux2err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux2err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux3 |
svNgc253Detection |
VSASVNGC253 |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux3 |
svOrionDetection |
VSASVORION |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux3 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux3 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux3 |
ultravistaListRemeasurement |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux3 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux3err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux3err |
svOrionDetection |
VSASVORION |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux3err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux3err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 3 (SE: FLUXERR_APER3) {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux3err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux3err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux4 |
svNgc253Detection |
VSASVNGC253 |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux4 |
svOrionDetection |
VSASVORION |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux4 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux4 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux4 |
ultravistaListRemeasurement |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux4 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux4err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux4err |
svOrionDetection |
VSASVORION |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux4err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux4err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 4 (SE: FLUXERR_APER4) {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux4err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux4err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux5 |
svNgc253Detection |
VSASVNGC253 |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux5 |
svOrionDetection |
VSASVORION |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux5 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux5 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux5 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux5 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux5err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux5err |
svOrionDetection |
VSASVORION |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux5err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux5err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 5 (SE: FLUXERR_APER5) {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux5err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux5err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux6 |
svNgc253Detection |
VSASVNGC253 |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux6 |
svOrionDetection |
VSASVORION |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux6 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux6 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux6 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux6 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux6err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux6err |
svOrionDetection |
VSASVORION |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux6err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux6err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 6 (SE: FLUXERR_APER6) {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux6err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux6err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux7 |
svNgc253Detection |
VSASVNGC253 |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux7 |
svOrionDetection |
VSASVORION |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux7 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux7 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux7 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux7 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux7err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux7err |
svOrionDetection |
VSASVORION |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux7err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux7err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 7 (SE: FLUXERR_APER7) {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux7err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux7err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux8 |
svNgc253Detection |
VSASVNGC253 |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux8 |
svOrionDetection |
VSASVORION |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux8 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux8 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux8 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux8 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux8err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux8err |
svOrionDetection |
VSASVORION |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux8err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux8err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 8 (SE: FLUXERR_APER8) {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux8err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux8err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux9 |
svNgc253Detection |
VSASVNGC253 |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux9 |
svOrionDetection |
VSASVORION |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux9 |
ultravistaDetection |
VSAUltraVISTA |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux9 |
ultravistaDetection, videoDetection |
VSAQC |
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 |
|
PHOT_INTENSITY_ADU |
aperFlux9 |
ultravistaListRemeasurement |
VSAUltraVISTA |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux9 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
aperFlux9err |
svNgc253Detection |
VSASVNGC253 |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux9err |
svOrionDetection |
VSASVORION |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux9err |
ultravistaDetection |
VSAUltraVISTA |
Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux9err |
ultravistaDetection, videoDetection |
VSAQC |
Error in aperture flux 9 (SE: FLUXERR_APER9) {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux9err |
ultravistaListRemeasurement |
VSAUltraVISTA |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
ERROR |
aperFlux9err |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} |
real |
4 |
ADU |
|
ERROR |
aperMag1 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag1 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag1 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag1 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag1 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr 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, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr 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 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag10 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag10 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag10 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 10 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag10 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr 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, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag10err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
ERROR |
aperMag10err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
ERROR |
aperMag10err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
ERROR |
aperMag10err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 10 |
real |
4 |
mag |
|
ERROR |
aperMag11 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag11 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag11 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag11 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 11 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag11 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr 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, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag11err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
ERROR |
aperMag11err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
ERROR |
aperMag11err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
ERROR |
aperMag11err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 11 |
real |
4 |
mag |
|
ERROR |
aperMag12 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag12 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag12 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag12 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 12 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag12 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr 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, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag12err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
ERROR |
aperMag12err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
ERROR |
aperMag12err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
ERROR |
aperMag12err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 12 |
real |
4 |
mag |
|
ERROR |
aperMag13 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag13 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag13 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag13 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 13 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag13 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag13err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
ERROR |
aperMag13err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
ERROR |
aperMag13err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
ERROR |
aperMag13err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 13 |
real |
4 |
mag |
|
ERROR |
aperMag1err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
ERROR |
aperMag1err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
ERROR |
aperMag1err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
ERROR |
aperMag1err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 1 |
real |
4 |
mag |
|
ERROR |
aperMag2 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag2 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag2 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag2 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag2 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 2 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag2err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
ERROR |
aperMag2err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
ERROR |
aperMag2err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
ERROR |
aperMag2err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 2 |
real |
4 |
mag |
|
ERROR |
aperMag3 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag3 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag3 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag3 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 3 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag3 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag3err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
ERROR |
aperMag3err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
ERROR |
aperMag3err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
ERROR |
aperMag3err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 3 |
real |
4 |
mag |
|
ERROR |
aperMag4 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag4 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag4 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag4 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag4 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 4 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag4err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
ERROR |
aperMag4err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
ERROR |
aperMag4err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
ERROR |
aperMag4err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 4 |
real |
4 |
mag |
|
ERROR |
aperMag5 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag5 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag5 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag5 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag5 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 5 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag5err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
ERROR |
aperMag5err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
ERROR |
aperMag5err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
ERROR |
aperMag5err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 5 |
real |
4 |
mag |
|
ERROR |
aperMag6 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag6 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag6 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag6 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag6 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 6 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag6err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
ERROR |
aperMag6err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
ERROR |
aperMag6err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
ERROR |
aperMag6err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 6 |
real |
4 |
mag |
|
ERROR |
aperMag7 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag7 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag7 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag7 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag7 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 7 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag7err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
ERROR |
aperMag7err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
ERROR |
aperMag7err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
ERROR |
aperMag7err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 7 |
real |
4 |
mag |
|
ERROR |
aperMag8 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag8 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag8 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag8 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 8 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag8 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag8err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
ERROR |
aperMag8err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
ERROR |
aperMag8err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
ERROR |
aperMag8err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 8 |
real |
4 |
mag |
|
ERROR |
aperMag9 |
svNgc253Detection |
VSASVNGC253 |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag9 |
svOrionDetection |
VSASVORION |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag9 |
ultravistaDetection |
VSAUltraVISTA |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag9 |
ultravistaDetection, ultravistaListRemeasurement, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingListRemeasurement, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Calibrated and corrected aperture magnitude 9 |
real |
4 |
mag |
|
PHOT_INT-MAG |
aperMag9 |
vhsDetection |
VSAVHS |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMag9err |
svNgc253Detection |
VSASVNGC253 |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
ERROR |
aperMag9err |
svOrionDetection |
VSASVORION |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
ERROR |
aperMag9err |
ultravistaDetection |
VSAUltraVISTA |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
ERROR |
aperMag9err |
ultravistaDetection, ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoDetection, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
Error in calibrated aperture magnitude 9 |
real |
4 |
mag |
|
ERROR |
aperMagNoAperCorr1 |
vhsDetection |
VSAVHS |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr1 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection |
VSAVHS |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr2 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection |
VSAVHS |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr3 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection |
VSAVHS |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr4 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection |
VSAVHS |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr5 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection |
VSAVHS |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr6 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection |
VSAVHS |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperMagNoAperCorr7 |
vhsDetection, vikingDetection, vmcDetection |
VSAQC |
Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 |
real |
4 |
mag |
|
PHOT_INT-MAG |
The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. |
aperture |
RequiredListDrivenProduct |
VSASVNGC253 |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VSASVORION |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VSAUltraVISTA |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VSAVHS |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VSAVIDEO |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VSAVIKING |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VSAVMC |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
aperture |
RequiredListDrivenProduct |
VSAVVV |
CASU list-driven photometry tool option specifying the fixed radius to be used for photometry |
real |
4 |
pixels |
|
?? |
APPDEC_R |
spectra |
SIXDF |
apparent DEC of field centre |
float |
8 |
radians |
|
|
APPDEC_V |
spectra |
SIXDF |
apparent DEC of field centre |
float |
8 |
radians |
|
|
APPRA_R |
spectra |
SIXDF |
apparent RA of field centre |
float |
8 |
radians |
|
|
APPRA_V |
spectra |
SIXDF |
apparent RA of field centre |
float |
8 |
radians |
|
|
aProf1 |
svNgc253Detection |
VSASVNGC253 |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
NUMBER |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
svOrionDetection |
VSASVORION |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
NUMBER |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
ultravistaDetection |
VSAUltraVISTA |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
NUMBER |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
ultravistaDetection, videoDetection |
VSAQC |
Isophotal area at level 0 (analysis threshold) (SE: ISO0) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixel² |
|
NUMBER |
SExtractor calculates areal profiles at thresholds spaced by a constant factor between the detection threshold and the peak brightness of the object. |
aProf1 |
ultravistaListRemeasurement |
VSAUltraVISTA |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
NUMBER |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf1 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} |
real |
4 |
pixels |
|
NUMBER |
Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. |
aProf2 |
svNgc253Detection |
VSASVNGC253 |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf2 |
svOrionDetection |
VSASVORION |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf2 |
ultravistaDetection |
VSAUltraVISTA |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf2 |
ultravistaDetection, videoDetection |
VSAQC |
Isophotal area at level 1 above analysis threshold (SE: ISO1) {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf2 |
ultravistaListRemeasurement |
VSAUltraVISTA |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf2 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf3 |
svNgc253Detection |
VSASVNGC253 |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf3 |
svOrionDetection |
VSASVORION |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf3 |
ultravistaDetection |
VSAUltraVISTA |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf3 |
ultravistaDetection, videoDetection |
VSAQC |
Isophotal area at level 2 above analysis threshold (SE: ISO2) {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf3 |
ultravistaListRemeasurement |
VSAUltraVISTA |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf3 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf4 |
svNgc253Detection |
VSASVNGC253 |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf4 |
svOrionDetection |
VSASVORION |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf4 |
ultravistaDetection |
VSAUltraVISTA |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf4 |
ultravistaDetection, videoDetection |
VSAQC |
Isophotal area at level 3 above analysis threshold (SE: ISO3) {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf4 |
ultravistaListRemeasurement |
VSAUltraVISTA |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf4 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf5 |
svNgc253Detection |
VSASVNGC253 |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf5 |
svOrionDetection |
VSASVORION |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf5 |
ultravistaDetection |
VSAUltraVISTA |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf5 |
ultravistaDetection, videoDetection |
VSAQC |
Isophotal area at level 4 above analysis threshold (SE: ISO4) {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf5 |
ultravistaListRemeasurement |
VSAUltraVISTA |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf5 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf6 |
svNgc253Detection |
VSASVNGC253 |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf6 |
svOrionDetection |
VSASVORION |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf6 |
ultravistaDetection |
VSAUltraVISTA |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf6 |
ultravistaDetection, videoDetection |
VSAQC |
Isophotal area at level 5 above analysis threshold (SE: ISO5) {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf6 |
ultravistaListRemeasurement |
VSAUltraVISTA |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf6 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf7 |
svNgc253Detection |
VSASVNGC253 |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf7 |
svOrionDetection |
VSASVORION |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf7 |
ultravistaDetection |
VSAUltraVISTA |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf7 |
ultravistaDetection, videoDetection |
VSAQC |
Isophotal area at level 6 above analysis threshold (SE: ISO6) {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf7 |
ultravistaListRemeasurement |
VSAUltraVISTA |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf7 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf8 |
svNgc253Detection |
VSASVNGC253 |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf8 |
svOrionDetection |
VSASVORION |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf8 |
ultravistaDetection |
VSAUltraVISTA |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf8 |
ultravistaDetection, videoDetection |
VSAQC |
Isophotal area at level 7 above analysis threshold (SE: ISO7) {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixel² |
|
NUMBER |
aProf8 |
ultravistaListRemeasurement |
VSAUltraVISTA |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
aProf8 |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int |
4 |
pixels |
|
NUMBER |
arcfile |
Multiframe |
VSASVNGC253 |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VSASVORION |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VSAUltraVISTA |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VSAVHS |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VSAVIDEO |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VSAVIKING |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VSAVMC |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
Multiframe |
VSAVVV |
Archive File Name {image primary HDU keyword: ARCFILE} |
varchar |
64 |
|
NONE |
|
arcfile |
ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Archive File Name |
varchar |
64 |
|
NONE |
|
AREA |
grs_ngpSource, grs_ranSource, grs_sgpSource |
TWODFGRS |
Isophotal area in pixels |
real |
4 |
|
|
|
areaID |
Multiframe |
VSASVNGC253 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VSASVORION |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VSAUltraVISTA |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VSAVHS |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VSAVIDEO |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VSAVIKING |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VSAVMC |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
Multiframe |
VSAVVV |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
areaID |
ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
SADT Survey area ID |
int |
4 |
|
-99999999 |
|
averageConf |
svNgc253Detection |
VSASVNGC253 |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
CODE_MISC |
averageConf |
svOrionDetection |
VSASVORION |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
CODE_MISC |
averageConf |
ultravistaDetection |
VSAUltraVISTA |
The average confidence level in the default 2 arcsec diameter aperture (aper3), not available in SE output {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
CODE_MISC |
averageConf |
ultravistaDetection, videoDetection |
VSAQC |
The average confidence level in the default 2 arcsec diameter aperture (aper3), not available in SE output {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
CODE_MISC |
averageConf |
ultravistaListRemeasurement |
VSAUltraVISTA |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
CODE_MISC |
averageConf |
ultravistaListRemeasurement, vhsDetection, vhsListRemeasurement, videoListRemeasurement, vikingDetection, vikingListRemeasurement, vmcDetection, vmcListRemeasurement, vvvDetection, vvvListRemeasurement |
VSAQC |
The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} |
real |
4 |
|
-99999999 |
CODE_MISC |
averageCoverage160 |
sage_lmcMips160Source |
SPITZER |
The average coverage (# of independent observations per pixel) |
float |
8 |
|
|
|
averageCoverage24 |
sage_lmcMips24Source |
SPITZER |
The average coverage (# of independent observations per pixel) |
float |
8 |
|
|
|
averageCoverage70 |
sage_lmcMips70Source |
SPITZER |
The average coverage (# of independent observations per pixel) |
float |
8 |
|
|
|
avSaturLevel |
MultiframeDetector |
VSASVNGC253 |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VSASVORION |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VSAUltraVISTA |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VSAVHS |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VSAVIDEO |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VSAVIKING |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VSAVMC |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
MultiframeDetector |
VSAVVV |
Average saturation level in frame {catalogue extension keyword: SATURATE} |
real |
4 |
|
-0.9999995e9 |
|
avSaturLevel |
ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Average saturation level in frame |
real |
4 |
|
-0.9999995e9 |
|
avStellarEll |
MultiframeDetector |
VSASVNGC253 |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
avStellarEll |
MultiframeDetector |
VSASVORION |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
avStellarEll |
MultiframeDetector |
VSAUltraVISTA |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
avStellarEll |
MultiframeDetector |
VSAVHS |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
avStellarEll |
MultiframeDetector |
VSAVIDEO |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
avStellarEll |
MultiframeDetector |
VSAVIKING |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
avStellarEll |
MultiframeDetector |
VSAVMC |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
avStellarEll |
MultiframeDetector |
VSAVVV |
Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
avStellarEll |
ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Average stellar ellipticity (1-b/a) |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
axis1Length |
MultiframeDetector |
VSASVNGC253 |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
|
NUMBER |
axis1Length |
MultiframeDetector |
VSASVORION |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
|
NUMBER |
axis1Length |
MultiframeDetector |
VSAUltraVISTA |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
|
NUMBER |
axis1Length |
MultiframeDetector |
VSAVHS |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
|
NUMBER |
axis1Length |
MultiframeDetector |
VSAVIDEO |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
|
NUMBER |
axis1Length |
MultiframeDetector |
VSAVIKING |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
|
NUMBER |
axis1Length |
MultiframeDetector |
VSAVMC |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
|
NUMBER |
axis1Length |
MultiframeDetector |
VSAVVV |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
|
NUMBER |
axis1Length |
ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} |
int |
4 |
|
|
NUMBER |
axis2Length |
MultiframeDetector |
VSASVNGC253 |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
|
NUMBER |
axis2Length |
MultiframeDetector |
VSASVORION |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
|
NUMBER |
axis2Length |
MultiframeDetector |
VSAUltraVISTA |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
|
NUMBER |
axis2Length |
MultiframeDetector |
VSAVHS |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
|
NUMBER |
axis2Length |
MultiframeDetector |
VSAVIDEO |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
|
NUMBER |
axis2Length |
MultiframeDetector |
VSAVIKING |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
|
NUMBER |
axis2Length |
MultiframeDetector |
VSAVMC |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
|
NUMBER |
axis2Length |
MultiframeDetector |
VSAVVV |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
|
NUMBER |
axis2Length |
ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} |
int |
4 |
|
|
NUMBER |
aY |
svNgc253Source |
VSASVNGC253 |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aY |
ultravistaSource |
VSAUltraVISTA |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aY |
ultravistaSource, vhsSource, videoSource, vikingSource |
VSAQC |
The galactic extinction correction in the Y band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aZ |
svNgc253Source |
VSASVNGC253 |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aZ |
ultravistaSource |
VSAUltraVISTA |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|
aZ |
ultravistaSource, videoSource, vikingSource |
VSAQC |
The galactic extinction correction in the Z band for extragalactic objects |
real |
4 |
mag |
-0.9999995e9 |
|