I |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
iAperMag3 |
atlasSource |
ATLASDR1 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMag3 |
atlasSource |
ATLASDR2 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMag3 |
atlasSource |
ATLASDR3 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag3 |
atlasSource |
ATLASDR4 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag3 |
atlasSource |
ATLASDR5 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag3 |
atlasSource |
ATLASv20131127 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMag3 |
atlasSource |
ATLASv20160425 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag3 |
atlasSource |
ATLASv20180209 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag3 |
vphasSource |
VPHASDR3 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag3 |
vphasSource |
VPHASv20160112 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag3 |
vphasSource |
VPHASv20170222 |
Default point source I aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag3Err |
atlasSource |
ATLASDR1 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iAperMag3Err |
atlasSource |
ATLASDR2 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iAperMag3Err |
atlasSource |
ATLASDR3 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag3Err |
atlasSource |
ATLASDR4 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag3Err |
atlasSource |
ATLASDR5 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag3Err |
atlasSource |
ATLASv20131127 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iAperMag3Err |
atlasSource |
ATLASv20160425 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag3Err |
atlasSource |
ATLASv20180209 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag3Err |
vphasSource |
VPHASDR3 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag3Err |
vphasSource |
VPHASv20160112 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag3Err |
vphasSource |
VPHASv20170222 |
Error in default point/extended source I mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag4 |
atlasSource |
ATLASDR1 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMag4 |
atlasSource |
ATLASDR2 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMag4 |
atlasSource |
ATLASDR3 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag4 |
atlasSource |
ATLASDR4 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag4 |
atlasSource |
ATLASDR5 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag4 |
atlasSource |
ATLASv20131127 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMag4 |
atlasSource |
ATLASv20160425 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag4 |
atlasSource |
ATLASv20180209 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag4 |
vphasSource |
VPHASDR3 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag4 |
vphasSource |
VPHASv20160112 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag4 |
vphasSource |
VPHASv20170222 |
Point source I aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag4Err |
atlasSource |
ATLASDR1 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iAperMag4Err |
atlasSource |
ATLASDR2 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iAperMag4Err |
atlasSource |
ATLASDR3 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag4Err |
atlasSource |
ATLASDR4 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag4Err |
atlasSource |
ATLASDR5 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag4Err |
atlasSource |
ATLASv20131127 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iAperMag4Err |
atlasSource |
ATLASv20160425 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag4Err |
atlasSource |
ATLASv20180209 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag4Err |
vphasSource |
VPHASDR3 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag4Err |
vphasSource |
VPHASv20160112 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag4Err |
vphasSource |
VPHASv20170222 |
Error in point/extended source I mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag6 |
atlasSource |
ATLASDR1 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMag6 |
atlasSource |
ATLASDR2 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMag6 |
atlasSource |
ATLASDR3 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag6 |
atlasSource |
ATLASDR4 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag6 |
atlasSource |
ATLASDR5 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag6 |
atlasSource |
ATLASv20131127 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMag6 |
atlasSource |
ATLASv20160425 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag6 |
atlasSource |
ATLASv20180209 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag6 |
vphasSource |
VPHASDR3 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag6 |
vphasSource |
VPHASv20160112 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag6 |
vphasSource |
VPHASv20170222 |
Point source I aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMag6Err |
atlasSource |
ATLASDR1 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iAperMag6Err |
atlasSource |
ATLASDR2 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iAperMag6Err |
atlasSource |
ATLASDR3 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag6Err |
atlasSource |
ATLASDR4 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag6Err |
atlasSource |
ATLASDR5 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag6Err |
atlasSource |
ATLASv20131127 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iAperMag6Err |
atlasSource |
ATLASv20160425 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag6Err |
atlasSource |
ATLASv20180209 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag6Err |
vphasSource |
VPHASDR3 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag6Err |
vphasSource |
VPHASv20160112 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMag6Err |
vphasSource |
VPHASv20170222 |
Error in point/extended source I mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iAperMagNoAperCorr3 |
atlasSource |
ATLASDR1 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMagNoAperCorr3 |
atlasSource |
ATLASDR2 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMagNoAperCorr3 |
atlasSource |
ATLASDR3 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr3 |
atlasSource |
ATLASDR4 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr3 |
atlasSource |
ATLASDR5 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr3 |
atlasSource |
ATLASv20131127 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMagNoAperCorr3 |
atlasSource |
ATLASv20160425 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr3 |
atlasSource |
ATLASv20180209 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr3 |
vphasSource |
VPHASDR3 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr3 |
vphasSource |
VPHASv20160112 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr3 |
vphasSource |
VPHASv20170222 |
Default extended source I aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr4 |
atlasSource |
ATLASDR1 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMagNoAperCorr4 |
atlasSource |
ATLASDR2 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMagNoAperCorr4 |
atlasSource |
ATLASDR3 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr4 |
atlasSource |
ATLASDR4 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr4 |
atlasSource |
ATLASDR5 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr4 |
atlasSource |
ATLASv20131127 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMagNoAperCorr4 |
atlasSource |
ATLASv20160425 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr4 |
atlasSource |
ATLASv20180209 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr4 |
vphasSource |
VPHASDR3 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr4 |
vphasSource |
VPHASv20160112 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr4 |
vphasSource |
VPHASv20170222 |
Extended source I aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr6 |
atlasSource |
ATLASDR1 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMagNoAperCorr6 |
atlasSource |
ATLASDR2 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMagNoAperCorr6 |
atlasSource |
ATLASDR3 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr6 |
atlasSource |
ATLASDR4 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr6 |
atlasSource |
ATLASDR5 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr6 |
atlasSource |
ATLASv20131127 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iAperMagNoAperCorr6 |
atlasSource |
ATLASv20160425 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr6 |
atlasSource |
ATLASv20180209 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr6 |
vphasSource |
VPHASDR3 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr6 |
vphasSource |
VPHASv20160112 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iAperMagNoAperCorr6 |
vphasSource |
VPHASv20170222 |
Extended source I aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
IAUNAME |
twoxmm, twoxmm_v1_2 |
XMM |
The IAU name assigned to the unique SRCID. |
varchar |
21 |
|
|
|
IAUNAME |
twoxmmi_dr3_v1_0 |
XMM |
The IAU name assigned to the unique SRCID. |
varchar |
30 |
|
|
|
IAUNAME |
xmm3dr4 |
XMM |
The IAU name assigned to the unique SRCID. |
varchar |
50 |
|
|
|
iAverageConf |
atlasSource |
ATLASDR1 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
meta.code |
iAverageConf |
atlasSource |
ATLASDR2 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
meta.code |
iAverageConf |
atlasSource |
ATLASDR3 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
stat.likelihood;em.opt.I |
iAverageConf |
atlasSource |
ATLASDR4 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
stat.likelihood;em.opt.I |
iAverageConf |
atlasSource |
ATLASDR5 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
stat.likelihood;em.opt.I |
iAverageConf |
atlasSource |
ATLASv20131127 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
meta.code |
iAverageConf |
atlasSource |
ATLASv20160425 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
stat.likelihood;em.opt.I |
iAverageConf |
atlasSource |
ATLASv20180209 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
stat.likelihood;em.opt.I |
iAverageConf |
vphasSource |
VPHASDR3 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
stat.likelihood;em.opt.I |
iAverageConf |
vphasSource |
VPHASv20160112 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
stat.likelihood;em.opt.I |
iAverageConf |
vphasSource |
VPHASv20170222 |
average confidence in 2 arcsec diameter default aperture (aper3) I |
real |
4 |
|
-99999999 |
stat.likelihood;em.opt.I |
ic |
hipparcos_new_reduction |
GAIADR1 |
Entry in one of the supplementary catalogues |
int |
4 |
|
|
meta.id.cross |
iCalCorr |
twompzPhotoz |
TWOMPZ |
SuperCOSMOS IgCorMag corrected for Galactic dust extinction. Southern hemisphere [dec(1950)<2.5] have been corrected for a small colour dependent offset between UKST and POSS-II. {image primary HDU keyword: IcalCorr} |
real |
4 |
|
-0.9999995e9 |
|
iCalCorrErr |
twompzPhotoz |
TWOMPZ |
Estimated error in I band {image primary HDU keyword: errI} |
real |
4 |
mag |
-0.9999995e9 |
|
iClass |
atlasSource |
ATLASDR1 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class |
iClass |
atlasSource |
ATLASDR2 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class |
iClass |
atlasSource |
ATLASDR3 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class;em.opt.I |
iClass |
atlasSource |
ATLASDR4 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class;em.opt.I |
iClass |
atlasSource |
ATLASDR5 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class;em.opt.I |
iClass |
atlasSource |
ATLASv20131127 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class |
iClass |
atlasSource |
ATLASv20160425 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class;em.opt.I |
iClass |
atlasSource |
ATLASv20180209 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class;em.opt.I |
iClass |
vphasSource |
VPHASDR3 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class;em.opt.I |
iClass |
vphasSource |
VPHASv20160112 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class;em.opt.I |
iClass |
vphasSource |
VPHASv20170222 |
discrete image classification flag in I |
smallint |
2 |
|
-9999 |
src.class;em.opt.I |
iClassStat |
atlasSource |
ATLASDR1 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat |
iClassStat |
atlasSource |
ATLASDR2 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat |
iClassStat |
atlasSource |
ATLASDR3 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat;em.opt.I |
iClassStat |
atlasSource |
ATLASDR4 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat;em.opt.I |
iClassStat |
atlasSource |
ATLASDR5 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat;em.opt.I |
iClassStat |
atlasSource |
ATLASv20131127 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat |
iClassStat |
atlasSource |
ATLASv20160425 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat;em.opt.I |
iClassStat |
atlasSource |
ATLASv20180209 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat;em.opt.I |
iClassStat |
vphasSource |
VPHASDR3 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat;em.opt.I |
iClassStat |
vphasSource |
VPHASv20160112 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat;em.opt.I |
iClassStat |
vphasSource |
VPHASv20170222 |
N(0,1) stellarness-of-profile statistic in I |
real |
4 |
|
-0.9999995e9 |
stat;em.opt.I |
icrf2_match |
aux_qso_icrf2_match |
GAIADR1 |
ICRF2 designation of the source matched to this Gaia source |
varchar |
32 |
|
|
meta.id.cross |
id |
twomass_xsc |
TWOMASS |
source ID number (unique within scan, coadd). |
int |
4 |
|
|
meta.number |
id |
tycho2 |
GAIADR1 |
Tycho2 identifier (constructed from the GSC region number) |
varchar |
32 |
|
|
meta.id;meta.main |
ID_2MASS |
ravedr5Source |
RAVE |
2MASS identifier |
varchar |
20 |
|
|
meta.id |
ID_ALLWISE |
ravedr5Source |
RAVE |
ALLWISE identifier |
varchar |
20 |
|
|
meta.id |
id_cat |
twomass_xsc |
TWOMASS |
matched galaxy's catalog name. |
varchar |
20 |
|
|
NAME |
ID_DENIS |
ravedr5Source |
RAVE |
DENIS identifier |
varchar |
17 |
|
|
meta.id |
id_epc |
igsl_source_catalog_ids |
GAIADR1 |
Identifier in Ecliptic Poles Catalogue |
varchar |
20 |
|
|
meta.id;meta.dataset |
id_flg |
twomass_xsc |
TWOMASS |
type/galaxy ID flag (0=non-catalog, 1=catalog, 2=LCSB). |
smallint |
2 |
|
|
meta.code |
id_gsc23 |
igsl_source_catalog_ids |
GAIADR1 |
Identifier in GSC2.3 |
bigint |
8 |
|
|
meta.id;meta.dataset |
id_hip |
igsl_source_catalog_ids |
GAIADR1 |
Identifier in Hipparcos |
int |
4 |
|
|
meta.id;meta.dataset |
ID_Hipparcos |
ravedr5Source |
RAVE |
Hipparcos identifier |
varchar |
6 |
|
|
meta.id |
id_lqrf |
igsl_source_catalog_ids |
GAIADR1 |
Identifier in LQRF |
int |
4 |
|
|
meta.id;meta.dataset |
id_ogle |
igsl_source_catalog_ids |
GAIADR1 |
Identifier in OGLE |
bigint |
8 |
|
|
meta.id;meta.dataset |
ID_PPMXL |
ravedr5Source |
RAVE |
PPMXL identifier |
bigint |
8 |
|
|
meta.id |
id_ppmxl |
igsl_source_catalog_ids |
GAIADR1 |
Identifier in PPMXL |
bigint |
8 |
|
|
meta.id;meta.dataset |
id_sdss |
igsl_source_catalog_ids |
GAIADR1 |
Identifier in SDSS |
bigint |
8 |
|
|
meta.id;meta.dataset |
ID_TGAS_source |
ravedr5Source |
RAVE |
TGAS source identifier |
bigint |
8 |
|
|
meta.id |
id_tmass |
igsl_source_catalog_ids |
GAIADR1 |
Identifier in 2MASS PSC |
bigint |
8 |
|
|
meta.id;meta.dataset |
id_tycho |
igsl_source_catalog_ids |
GAIADR1 |
Identifier in Tycho |
bigint |
8 |
|
|
meta.id;meta.dataset |
id_tycho |
tycho2 |
GAIADR1 |
Numerical Tycho2 identifier |
bigint |
8 |
|
|
meta.id;meta.dataset |
ID_TYCHO2 |
ravedr5Source |
RAVE |
TYCHO2 identifier |
varchar |
12 |
|
|
meta.id |
id_ucac |
igsl_source_catalog_ids |
GAIADR1 |
Identifier in UCAC |
int |
4 |
|
|
meta.id;meta.dataset |
ID_UCAC4 |
ravedr5Source |
RAVE |
UCAC4 identifier |
varchar |
11 |
|
|
meta.id |
ID_USNOB1 |
ravedr5Source |
RAVE |
USNOB-1 identifier |
varchar |
14 |
|
|
meta.id |
idCand |
rosat_bsc |
ROSAT |
number of identification candidates in the correlation catalogue |
smallint |
2 |
|
|
meta.number |
idCand |
rosat_fsc |
ROSAT |
number of identification candidates in the correlation catalogue |
tinyint |
1 |
|
|
meta.number |
idType |
iras_psc |
IRAS |
Type of Object |
tinyint |
1 |
|
|
src.class |
iEll |
atlasSource |
ATLASDR1 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
iEll |
atlasSource |
ATLASDR2 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
iEll |
atlasSource |
ATLASDR3 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity;em.opt.I |
iEll |
atlasSource |
ATLASDR4 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity;em.opt.I |
iEll |
atlasSource |
ATLASDR5 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity;em.opt.I |
iEll |
atlasSource |
ATLASv20131127 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
iEll |
atlasSource |
ATLASv20160425 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity;em.opt.I |
iEll |
atlasSource |
ATLASv20180209 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity;em.opt.I |
iEll |
vphasSource |
VPHASDR3 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity;em.opt.I |
iEll |
vphasSource |
VPHASv20160112 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity;em.opt.I |
iEll |
vphasSource |
VPHASv20170222 |
1-b/a, where a/b=semi-major/minor axes in I |
real |
4 |
|
-0.9999995e9 |
src.ellipticity;em.opt.I |
ieNum |
atlasMergeLog |
ATLASDR1 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.number |
ieNum |
atlasMergeLog |
ATLASDR2 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.number |
ieNum |
atlasMergeLog |
ATLASDR3 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.number;em.opt.I |
ieNum |
atlasMergeLog |
ATLASDR4 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.number;em.opt.I |
ieNum |
atlasMergeLog |
ATLASDR5 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.id;em.opt.I |
ieNum |
atlasMergeLog |
ATLASv20131127 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.number |
ieNum |
atlasMergeLog |
ATLASv20160425 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.number;em.opt.I |
ieNum |
atlasMergeLog |
ATLASv20180209 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.number;em.opt.I |
ieNum |
vphasMergeLog |
VPHASDR3 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.number;em.opt.I |
ieNum |
vphasMergeLog |
VPHASv20160112 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.number;em.opt.I |
ieNum |
vphasMergeLog |
VPHASv20170222 |
the extension number of this I frame |
tinyint |
1 |
|
|
meta.number;em.opt.I |
iErrBits |
atlasSource |
ATLASDR1 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iErrBits |
atlasSource |
ATLASDR2 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iErrBits |
atlasSource |
ATLASDR3 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code;em.opt.I |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iErrBits |
atlasSource |
ATLASDR4 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code;em.opt.I |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iErrBits |
atlasSource |
ATLASDR5 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code;em.opt.I |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iErrBits |
atlasSource |
ATLASv20131127 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iErrBits |
atlasSource |
ATLASv20160425 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code;em.opt.I |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iErrBits |
atlasSource |
ATLASv20180209 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code;em.opt.I |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iErrBits |
vphasSource |
VPHASDR3 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code;em.opt.I |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iErrBits |
vphasSource |
VPHASv20160112 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code;em.opt.I |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iErrBits |
vphasSource |
VPHASv20170222 |
processing warning/error bitwise flags in I |
int |
4 |
|
-99999999 |
meta.code;em.opt.I |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
iEta |
atlasSource |
ATLASDR1 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iEta |
atlasSource |
ATLASDR2 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iEta |
atlasSource |
ATLASDR3 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iEta |
atlasSource |
ATLASDR4 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iEta |
atlasSource |
ATLASDR5 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iEta |
atlasSource |
ATLASv20131127 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iEta |
atlasSource |
ATLASv20160425 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iEta |
atlasSource |
ATLASv20180209 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iEta |
vphasSource |
VPHASDR3 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iEta |
vphasSource |
VPHASv20160112 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iEta |
vphasSource |
VPHASv20170222 |
Offset of I detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iFlag |
rosat_bsc, rosat_fsc |
ROSAT |
broad band image available |
varchar |
1 |
|
|
meta.code |
iGausig |
atlasSource |
ATLASDR1 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param |
iGausig |
atlasSource |
ATLASDR2 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param |
iGausig |
atlasSource |
ATLASDR3 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param;em.opt.I |
iGausig |
atlasSource |
ATLASDR4 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param;em.opt.I |
iGausig |
atlasSource |
ATLASDR5 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param;em.opt.I |
iGausig |
atlasSource |
ATLASv20131127 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param |
iGausig |
atlasSource |
ATLASv20160425 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param;em.opt.I |
iGausig |
atlasSource |
ATLASv20180209 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param;em.opt.I |
iGausig |
vphasSource |
VPHASDR3 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param;em.opt.I |
iGausig |
vphasSource |
VPHASv20160112 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param;em.opt.I |
iGausig |
vphasSource |
VPHASv20170222 |
RMS of axes of ellipse fit in I |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param;em.opt.I |
iHlCorSMjRadAs |
atlasSource |
ATLASDR1 |
Seeing corrected half-light, semi-major axis in I band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize;src |
iHlCorSMjRadAs |
atlasSource |
ATLASDR2 |
Seeing corrected half-light, semi-major axis in I band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize;src |
iHlCorSMjRadAs |
atlasSource |
ATLASDR3 |
Seeing corrected half-light, semi-major axis in I band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize;em.opt.I |
iHlCorSMjRadAs |
atlasSource |
ATLASDR4 |
Seeing corrected half-light, semi-major axis in I band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize;em.opt.I |
iHlCorSMjRadAs |
atlasSource |
ATLASDR5 |
Seeing corrected half-light, semi-major axis in I band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize;em.opt.I |
iHlCorSMjRadAs |
atlasSource |
ATLASv20131127 |
Seeing corrected half-light, semi-major axis in I band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize;src |
iHlCorSMjRadAs |
atlasSource |
ATLASv20160425 |
Seeing corrected half-light, semi-major axis in I band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize;em.opt.I |
iHlCorSMjRadAs |
atlasSource |
ATLASv20180209 |
Seeing corrected half-light, semi-major axis in I band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize;em.opt.I |
iKronMag |
atlasSource |
ATLASDR4 |
Extended source I mag (Kron) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iKronMag |
atlasSource |
ATLASDR5 |
Extended source I mag (Kron) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iKronMag |
atlasSource |
ATLASv20180209 |
Extended source I mag (Kron) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iKronMagErr |
atlasSource |
ATLASDR4 |
Error in extended source I mag (Kron) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iKronMagErr |
atlasSource |
ATLASDR5 |
Error in extended source I mag (Kron) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iKronMagErr |
atlasSource |
ATLASv20180209 |
Error in extended source I mag (Kron) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
illumCorr |
atlasDetection |
ATLASDR1 |
illumination correction |
real |
4 |
|
0.0 |
|
illumCorr |
atlasDetection |
ATLASDR3 |
illumination correction |
real |
4 |
|
0.0 |
|
illumCorr |
atlasDetection |
ATLASDR4 |
illumination correction |
real |
4 |
|
0.0 |
|
illumCorr |
atlasDetection |
ATLASDR5 |
illumination correction |
real |
4 |
|
0.0 |
|
illumCorr |
atlasDetection |
ATLASv20131127 |
illumination correction |
real |
4 |
|
0.0 |
|
illumCorr |
atlasDetection |
ATLASv20160425 |
illumination correction |
real |
4 |
|
0.0 |
|
illumCorr |
atlasDetection |
ATLASv20180209 |
illumination correction |
real |
4 |
|
0.0 |
|
illumCorr |
atlasDetection, atlasDetectionUncorr |
ATLASDR2 |
illumination correction |
real |
4 |
|
0.0 |
|
illumCorr |
vphasDetection |
VPHASv20160112 |
illumination correction |
real |
4 |
|
0.0 |
|
illumCorr |
vphasDetection |
VPHASv20170222 |
illumination correction |
real |
4 |
|
0.0 |
|
illumCorr |
vphasDetection, vphasDetectionUncorr |
VPHASDR3 |
illumination correction |
real |
4 |
|
0.0 |
|
illumFile |
Multiframe |
ATLASDR1 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumFile |
Multiframe |
ATLASDR2 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumFile |
Multiframe |
ATLASDR3 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumFile |
Multiframe |
ATLASDR4 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumFile |
Multiframe |
ATLASDR5 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumFile |
Multiframe |
ATLASv20131127 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumFile |
Multiframe |
ATLASv20160425 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumFile |
Multiframe |
ATLASv20180209 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumFile |
Multiframe |
VPHASDR3 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumFile |
Multiframe |
VPHASv20160112 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumFile |
Multiframe |
VPHASv20170222 |
File name of CASU created photometric illumination correction used on catalogue data from this file |
varchar |
256 |
|
NONE |
|
illumMoon |
Multiframe |
ATLASDR1 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
illumMoon |
Multiframe |
ATLASDR2 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
illumMoon |
Multiframe |
ATLASDR3 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
illumMoon |
Multiframe |
ATLASDR4 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
illumMoon |
Multiframe |
ATLASDR5 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
illumMoon |
Multiframe |
ATLASv20131127 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
illumMoon |
Multiframe |
ATLASv20160425 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
illumMoon |
Multiframe |
ATLASv20180209 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
illumMoon |
Multiframe |
VPHASDR3 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
illumMoon |
Multiframe |
VPHASv20160112 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
illumMoon |
Multiframe |
VPHASv20170222 |
Illumination of the Moon |
float |
8 |
|
-0.9999995e9 |
?? |
im_nx |
twomass_xsc |
TWOMASS |
size of postage stamp image in pixels. |
smallint |
2 |
|
|
instr.fov;instr.pixel |
iMag |
ukirtFSstars |
ATLASDR1 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iMag |
ukirtFSstars |
ATLASDR2 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iMag |
ukirtFSstars |
ATLASDR3 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iMag |
ukirtFSstars |
ATLASDR4 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iMag |
ukirtFSstars |
ATLASDR5 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iMag |
ukirtFSstars |
ATLASv20131127 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iMag |
ukirtFSstars |
ATLASv20160425 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iMag |
ukirtFSstars |
ATLASv20180209 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iMag |
ukirtFSstars |
VPHASDR3 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iMag |
ukirtFSstars |
VPHASv20160112 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iMag |
ukirtFSstars |
VPHASv20170222 |
I band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
Imag_DENIS |
ravedr5Source |
RAVE |
Catalog I magnitude |
real |
4 |
mag |
|
phot.mag;em.opt.I |
Imag_USNOB1 |
ravedr5Source |
RAVE |
I magnitude USNOB1 |
real |
4 |
mag |
|
phot.mag;em.opt.I |
Image |
denisDR3Source |
DENIS |
DENIS image number; the image number is incremented at each image taken during the survey. In case a source results from the merging of two consecutive overlapping images (N and N+1) in the same strip (Flag_mult set to 1), the image number corresponds to the first image N. |
int |
4 |
|
|
|
imageExtent |
CurrentAstrometry |
ATLASDR1 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtent |
CurrentAstrometry |
ATLASDR2 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtent |
CurrentAstrometry |
ATLASDR3 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtent |
CurrentAstrometry |
ATLASDR4 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtent |
CurrentAstrometry |
ATLASDR5 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtent |
CurrentAstrometry |
ATLASv20131127 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtent |
CurrentAstrometry |
ATLASv20160425 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtent |
CurrentAstrometry |
ATLASv20180209 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtent |
CurrentAstrometry |
VPHASDR3 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtent |
CurrentAstrometry |
VPHASv20160112 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtent |
CurrentAstrometry |
VPHASv20170222 |
The maximum angular extent from the central position |
real |
4 |
Arcminutes |
-0.9999995e9 |
pos.angDistance |
imageExtType |
MultiframeDetector |
ATLASDR1 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageExtType |
MultiframeDetector |
ATLASDR2 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageExtType |
MultiframeDetector |
ATLASDR3 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageExtType |
MultiframeDetector |
ATLASDR4 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageExtType |
MultiframeDetector |
ATLASDR5 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageExtType |
MultiframeDetector |
ATLASv20131127 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageExtType |
MultiframeDetector |
ATLASv20160425 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageExtType |
MultiframeDetector |
ATLASv20180209 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageExtType |
MultiframeDetector |
VPHASDR3 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageExtType |
MultiframeDetector |
VPHASv20160112 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageExtType |
MultiframeDetector |
VPHASv20170222 |
Extension type in source FITS image file {image extension keyword: XTENSION} |
varchar |
16 |
|
NONE |
?? |
imageGcount |
MultiframeDetector |
ATLASDR1 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imageGcount |
MultiframeDetector |
ATLASDR2 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imageGcount |
MultiframeDetector |
ATLASDR3 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imageGcount |
MultiframeDetector |
ATLASDR4 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imageGcount |
MultiframeDetector |
ATLASDR5 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imageGcount |
MultiframeDetector |
ATLASv20131127 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imageGcount |
MultiframeDetector |
ATLASv20160425 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imageGcount |
MultiframeDetector |
ATLASv20180209 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imageGcount |
MultiframeDetector |
VPHASDR3 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imageGcount |
MultiframeDetector |
VPHASv20160112 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imageGcount |
MultiframeDetector |
VPHASv20170222 |
FITS image extension required keyword (always 1 for uncompressed images) {image extension keyword: GCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
ATLASDR1 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
ATLASDR2 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
ATLASDR3 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
ATLASDR4 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
ATLASDR5 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
ATLASv20131127 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
ATLASv20160425 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
ATLASv20180209 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
VPHASDR3 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
VPHASv20160112 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagePcount |
MultiframeDetector |
VPHASv20170222 |
FITS image extension required keyword (always 0 for uncompressed images) {image extension keyword: PCOUNT} |
int |
4 |
|
-99999999 |
meta.number |
imagesLocation |
ExternalSurvey |
ATLASDR1 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imagesLocation |
ExternalSurvey |
ATLASDR2 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imagesLocation |
ExternalSurvey |
ATLASDR3 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imagesLocation |
ExternalSurvey |
ATLASDR4 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imagesLocation |
ExternalSurvey |
ATLASDR5 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imagesLocation |
ExternalSurvey |
ATLASv20131127 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imagesLocation |
ExternalSurvey |
ATLASv20160425 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imagesLocation |
ExternalSurvey |
ATLASv20180209 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imagesLocation |
ExternalSurvey |
VPHASDR3 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imagesLocation |
ExternalSurvey |
VPHASv20160112 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imagesLocation |
ExternalSurvey |
VPHASv20170222 |
Pathname to the pixels (eg. for list-driven remeasurement) |
varchar |
256 |
|
|
?? |
imfID |
atlasMergeLog |
ATLASDR1 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
obs.field |
imfID |
atlasMergeLog |
ATLASDR2 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
obs.field |
imfID |
atlasMergeLog |
ATLASDR3 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
meta.id;obs.field;em.opt.I |
imfID |
atlasMergeLog |
ATLASDR4 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
meta.id;obs.field;em.opt.I |
imfID |
atlasMergeLog |
ATLASDR5 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
meta.id;obs.field;em.opt.I |
imfID |
atlasMergeLog |
ATLASv20131127 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
obs.field |
imfID |
atlasMergeLog |
ATLASv20160425 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
meta.id;obs.field;em.opt.I |
imfID |
atlasMergeLog |
ATLASv20180209 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
meta.id;obs.field;em.opt.I |
imfID |
vphasMergeLog |
VPHASDR3 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
meta.id;obs.field;em.opt.I |
imfID |
vphasMergeLog |
VPHASv20160112 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
meta.id;obs.field;em.opt.I |
imfID |
vphasMergeLog |
VPHASv20170222 |
the UID of the relevant I multiframe |
bigint |
8 |
|
|
meta.id;obs.field;em.opt.I |
iMjd |
atlasSource |
ATLASDR3 |
The mean Modified Julian Day of each detection |
float |
8 |
day |
-0.9999995e9 |
time.epoch |
iMjd |
atlasSource |
ATLASDR4 |
The mean Modified Julian Day of each detection |
float |
8 |
day |
-0.9999995e9 |
time.epoch;em.opt.I |
iMjd |
atlasSource |
ATLASDR5 |
The mean Modified Julian Day of each detection |
float |
8 |
day |
-0.9999995e9 |
time.epoch;em.opt.I |
iMjd |
atlasSource |
ATLASv20160425 |
The mean Modified Julian Day of each detection |
float |
8 |
day |
-0.9999995e9 |
time.epoch |
iMjd |
atlasSource |
ATLASv20180209 |
The mean Modified Julian Day of each detection |
float |
8 |
day |
-0.9999995e9 |
time.epoch;em.opt.I |
iMjd |
vphasSource |
VPHASDR3 |
The mean Modified Julian Day of each detection |
float |
8 |
day |
-0.9999995e9 |
time.epoch;em.opt.I |
iMjd |
vphasSource |
VPHASv20160112 |
The mean Modified Julian Day of each detection |
float |
8 |
day |
-0.9999995e9 |
time.epoch |
iMjd |
vphasSource |
VPHASv20170222 |
The mean Modified Julian Day of each detection |
float |
8 |
day |
-0.9999995e9 |
time.epoch |
imzExt |
atlasSource |
ATLASDR1 |
Extended source colour I-Z (using aperMagNoAperCorr3) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_COLOR |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExt |
atlasSource |
ATLASDR2 |
Extended source colour I-Z (using aperMagNoAperCorr3) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_COLOR |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExt |
atlasSource |
ATLASDR3 |
Extended source colour I-Z (using aperMagNoAperCorr3) |
real |
4 |
mag |
-0.9999995e9 |
phot.color;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExt |
atlasSource |
ATLASDR4 |
Extended source colour I-Z (using aperMagNoAperCorr3) |
real |
4 |
mag |
-0.9999995e9 |
phot.color;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExt |
atlasSource |
ATLASDR5 |
Extended source colour I-Z (using aperMagNoAperCorr3) |
real |
4 |
mag |
-0.9999995e9 |
phot.color;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExt |
atlasSource |
ATLASv20131127 |
Extended source colour I-Z (using aperMagNoAperCorr3) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_COLOR |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExt |
atlasSource |
ATLASv20160425 |
Extended source colour I-Z (using aperMagNoAperCorr3) |
real |
4 |
mag |
-0.9999995e9 |
phot.color;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExt |
atlasSource |
ATLASv20180209 |
Extended source colour I-Z (using aperMagNoAperCorr3) |
real |
4 |
mag |
-0.9999995e9 |
phot.color;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExtErr |
atlasSource |
ATLASDR1 |
Error on extended source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExtErr |
atlasSource |
ATLASDR2 |
Error on extended source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExtErr |
atlasSource |
ATLASDR3 |
Error on extended source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExtErr |
atlasSource |
ATLASDR4 |
Error on extended source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExtErr |
atlasSource |
ATLASDR5 |
Error on extended source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExtErr |
atlasSource |
ATLASv20131127 |
Error on extended source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExtErr |
atlasSource |
ATLASv20160425 |
Error on extended source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzExtErr |
atlasSource |
ATLASv20180209 |
Error on extended source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPnt |
atlasSource |
ATLASDR1 |
Point source colour I-Z (using aperMag3) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_COLOR |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPnt |
atlasSource |
ATLASDR2 |
Point source colour I-Z (using aperMag3) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_COLOR |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPnt |
atlasSource |
ATLASDR3 |
Point source colour I-Z (using aperMag3) |
real |
4 |
mag |
-0.9999995e9 |
phot.color;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPnt |
atlasSource |
ATLASDR4 |
Point source colour I-Z (using aperMag3) |
real |
4 |
mag |
-0.9999995e9 |
phot.color;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPnt |
atlasSource |
ATLASDR5 |
Point source colour I-Z (using aperMag3) |
real |
4 |
mag |
-0.9999995e9 |
phot.color;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPnt |
atlasSource |
ATLASv20131127 |
Point source colour I-Z (using aperMag3) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_COLOR |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPnt |
atlasSource |
ATLASv20160425 |
Point source colour I-Z (using aperMag3) |
real |
4 |
mag |
-0.9999995e9 |
phot.color;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPnt |
atlasSource |
ATLASv20180209 |
Point source colour I-Z (using aperMag3) |
real |
4 |
mag |
-0.9999995e9 |
phot.color;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPntErr |
atlasSource |
ATLASDR1 |
Error on point source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPntErr |
atlasSource |
ATLASDR2 |
Error on point source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPntErr |
atlasSource |
ATLASDR3 |
Error on point source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPntErr |
atlasSource |
ATLASDR4 |
Error on point source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPntErr |
atlasSource |
ATLASDR5 |
Error on point source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPntErr |
atlasSource |
ATLASv20131127 |
Error on point source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPntErr |
atlasSource |
ATLASv20160425 |
Error on point source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
imzPntErr |
atlasSource |
ATLASv20180209 |
Error on point source colour I-Z |
real |
4 |
mag |
-0.9999995e9 |
stat.error;em.opt.I;em.opt.I |
Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
INEXR |
mgcBrightSpec |
MGC |
Exclusion region flag (0 exclude/ 1 keep) |
tinyint |
1 |
|
|
|
inherit |
MultiframeDetector |
ATLASDR1 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
inherit |
MultiframeDetector |
ATLASDR2 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
inherit |
MultiframeDetector |
ATLASDR3 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
inherit |
MultiframeDetector |
ATLASDR4 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
inherit |
MultiframeDetector |
ATLASDR5 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
inherit |
MultiframeDetector |
ATLASv20131127 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
inherit |
MultiframeDetector |
ATLASv20160425 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
inherit |
MultiframeDetector |
ATLASv20180209 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
inherit |
MultiframeDetector |
VPHASDR3 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
inherit |
MultiframeDetector |
VPHASv20160112 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
inherit |
MultiframeDetector |
VPHASv20170222 |
denotes the INHERIT keyword convention {image extension keyword: INHERIT} |
tinyint |
1 |
|
0 |
|
insDate |
MultiframeEsoKeys |
ATLASDR1 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDate |
MultiframeEsoKeys |
ATLASDR2 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDate |
MultiframeEsoKeys |
ATLASDR3 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDate |
MultiframeEsoKeys |
ATLASDR4 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDate |
MultiframeEsoKeys |
ATLASDR5 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDate |
MultiframeEsoKeys |
ATLASv20131127 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDate |
MultiframeEsoKeys |
ATLASv20160425 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDate |
MultiframeEsoKeys |
ATLASv20180209 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDate |
MultiframeEsoKeys |
VPHASDR3 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDate |
MultiframeEsoKeys |
VPHASv20160112 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDate |
MultiframeEsoKeys |
VPHASv20170222 |
Instrument release date (yyyy-mm-dd) {image primary HDU keyword: HIERARCH ESO INS DATE} |
varchar |
16 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
ATLASDR1 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
ATLASDR2 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
ATLASDR3 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
ATLASDR4 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
ATLASDR5 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
ATLASv20131127 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
ATLASv20160425 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
ATLASv20180209 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
VPHASDR3 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
VPHASv20160112 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insDid |
MultiframeEsoKeys |
VPHASv20170222 |
Data dictionary {image primary HDU keyword: HIERARCH ESO INS DID} |
varchar |
32 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
ATLASDR1 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
ATLASDR2 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
ATLASDR3 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
ATLASDR4 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
ATLASDR5 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
ATLASv20131127 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
ATLASv20160425 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
ATLASv20180209 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
VPHASDR3 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
VPHASv20160112 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1ID |
MultiframeEsoKeys |
VPHASv20170222 |
Filter slot name {image primary HDU keyword: HIERARCH ESO INS FILT1 ID} |
varchar |
8 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
ATLASDR1 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
ATLASDR2 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
ATLASDR3 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
ATLASDR4 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
ATLASDR5 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
ATLASv20131127 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
ATLASv20160425 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
ATLASv20180209 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
VPHASDR3 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
VPHASv20160112 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1Name |
MultiframeEsoKeys |
VPHASv20170222 |
Filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
NONE |
|
insFilt1No |
MultiframeEsoKeys |
ATLASDR1 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1No |
MultiframeEsoKeys |
ATLASDR2 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1No |
MultiframeEsoKeys |
ATLASDR3 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1No |
MultiframeEsoKeys |
ATLASDR4 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1No |
MultiframeEsoKeys |
ATLASDR5 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1No |
MultiframeEsoKeys |
ATLASv20131127 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1No |
MultiframeEsoKeys |
ATLASv20160425 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1No |
MultiframeEsoKeys |
ATLASv20180209 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1No |
MultiframeEsoKeys |
VPHASDR3 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1No |
MultiframeEsoKeys |
VPHASv20160112 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1No |
MultiframeEsoKeys |
VPHASv20170222 |
Pos 1-6=Mag.A 7-12=Mag.B 0=NO Filter CASU** - Jim L? {image primary HDU keyword: HIERARCH ESO INS FILT1 NO} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
ATLASDR1 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
ATLASDR2 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
ATLASDR3 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
ATLASDR4 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
ATLASDR5 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
ATLASv20131127 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
ATLASv20160425 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
ATLASv20180209 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
VPHASDR3 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
VPHASv20160112 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insFilt1Swsim |
MultiframeEsoKeys |
VPHASv20170222 |
If T, function is software simulation {image primary HDU keyword: HIERARCH ESO INS FILT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insID |
MultiframeEsoKeys |
ATLASDR1 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insID |
MultiframeEsoKeys |
ATLASDR2 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insID |
MultiframeEsoKeys |
ATLASDR3 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insID |
MultiframeEsoKeys |
ATLASDR4 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insID |
MultiframeEsoKeys |
ATLASDR5 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insID |
MultiframeEsoKeys |
ATLASv20131127 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insID |
MultiframeEsoKeys |
ATLASv20160425 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insID |
MultiframeEsoKeys |
ATLASv20180209 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insID |
MultiframeEsoKeys |
VPHASDR3 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insID |
MultiframeEsoKeys |
VPHASv20160112 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insID |
MultiframeEsoKeys |
VPHASv20170222 |
Instrument ID {image primary HDU keyword: HIERARCH ESO INS ID} |
varchar |
16 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
ATLASDR1 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
ATLASDR2 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
ATLASDR3 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
ATLASDR4 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
ATLASDR5 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
ATLASv20131127 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
ATLASv20160425 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
ATLASv20180209 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
VPHASDR3 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
VPHASv20160112 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insMode |
MultiframeEsoKeys |
VPHASv20170222 |
Instrument mode used {image primary HDU keyword: HIERARCH ESO INS MODE} |
varchar |
8 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
ATLASDR1 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
ATLASDR2 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
ATLASDR3 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
ATLASDR4 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
ATLASDR5 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
ATLASv20131127 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
ATLASv20160425 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
ATLASv20180209 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
VPHASDR3 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
VPHASv20160112 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1ID |
MultiframeEsoKeys |
VPHASv20170222 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS1 ID} |
varchar |
4 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
ATLASDR1 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
ATLASDR2 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
ATLASDR3 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
ATLASDR4 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
ATLASDR5 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
ATLASv20131127 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
ATLASv20160425 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
ATLASv20180209 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
VPHASDR3 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
VPHASv20160112 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Name |
MultiframeEsoKeys |
VPHASv20170222 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS1 NAME} |
varchar |
16 |
|
NONE |
|
insSens1Val |
MultiframeEsoKeys |
ATLASDR1 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens1Val |
MultiframeEsoKeys |
ATLASDR2 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens1Val |
MultiframeEsoKeys |
ATLASDR3 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens1Val |
MultiframeEsoKeys |
ATLASDR4 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens1Val |
MultiframeEsoKeys |
ATLASDR5 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens1Val |
MultiframeEsoKeys |
ATLASv20131127 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens1Val |
MultiframeEsoKeys |
ATLASv20160425 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens1Val |
MultiframeEsoKeys |
ATLASv20180209 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens1Val |
MultiframeEsoKeys |
VPHASDR3 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens1Val |
MultiframeEsoKeys |
VPHASv20160112 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens1Val |
MultiframeEsoKeys |
VPHASv20170222 |
Calibration Lamps Current {image primary HDU keyword: HIERARCH ESO INS SENS1 VAL} |
real |
4 |
A |
-9.999995e+08 |
|
insSens2ID |
MultiframeEsoKeys |
ATLASDR1 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2ID |
MultiframeEsoKeys |
ATLASDR2 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2ID |
MultiframeEsoKeys |
ATLASDR3 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2ID |
MultiframeEsoKeys |
ATLASDR4 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2ID |
MultiframeEsoKeys |
ATLASDR5 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2ID |
MultiframeEsoKeys |
ATLASv20131127 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2ID |
MultiframeEsoKeys |
ATLASv20160425 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2ID |
MultiframeEsoKeys |
ATLASv20180209 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2ID |
MultiframeEsoKeys |
VPHASDR3 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2ID |
MultiframeEsoKeys |
VPHASv20160112 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2ID |
MultiframeEsoKeys |
VPHASv20170222 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS2 ID} |
varchar |
8 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
ATLASDR1 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
ATLASDR2 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
ATLASDR3 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
ATLASDR4 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
ATLASDR5 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
ATLASv20131127 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
ATLASv20160425 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
ATLASv20180209 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
VPHASDR3 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
VPHASv20160112 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Name |
MultiframeEsoKeys |
VPHASv20170222 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS2 NAME} |
varchar |
32 |
|
NONE |
|
insSens2Val |
MultiframeEsoKeys |
ATLASDR1 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens2Val |
MultiframeEsoKeys |
ATLASDR2 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens2Val |
MultiframeEsoKeys |
ATLASDR3 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens2Val |
MultiframeEsoKeys |
ATLASDR4 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens2Val |
MultiframeEsoKeys |
ATLASDR5 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens2Val |
MultiframeEsoKeys |
ATLASv20131127 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens2Val |
MultiframeEsoKeys |
ATLASv20160425 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens2Val |
MultiframeEsoKeys |
ATLASv20180209 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens2Val |
MultiframeEsoKeys |
VPHASDR3 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens2Val |
MultiframeEsoKeys |
VPHASv20160112 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens2Val |
MultiframeEsoKeys |
VPHASv20170222 |
Instr Cool. Fluid Flow IN {image primary HDU keyword: HIERARCH ESO INS SENS2 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3ID |
MultiframeEsoKeys |
ATLASDR1 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3ID |
MultiframeEsoKeys |
ATLASDR2 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3ID |
MultiframeEsoKeys |
ATLASDR3 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3ID |
MultiframeEsoKeys |
ATLASDR4 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3ID |
MultiframeEsoKeys |
ATLASDR5 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3ID |
MultiframeEsoKeys |
ATLASv20131127 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3ID |
MultiframeEsoKeys |
ATLASv20160425 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3ID |
MultiframeEsoKeys |
ATLASv20180209 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3ID |
MultiframeEsoKeys |
VPHASDR3 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3ID |
MultiframeEsoKeys |
VPHASv20160112 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3ID |
MultiframeEsoKeys |
VPHASv20170222 |
sensor ID {image primary HDU keyword: HIERARCH ESO INS SENS3 ID} |
varchar |
8 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
ATLASDR1 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
ATLASDR2 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
ATLASDR3 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
ATLASDR4 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
ATLASDR5 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
ATLASv20131127 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
ATLASv20160425 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
ATLASv20180209 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
VPHASDR3 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
VPHASv20160112 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Name |
MultiframeEsoKeys |
VPHASv20170222 |
Sensor common name {image primary HDU keyword: HIERARCH ESO INS SENS3 NAME} |
varchar |
32 |
|
NONE |
|
insSens3Val |
MultiframeEsoKeys |
ATLASDR1 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3Val |
MultiframeEsoKeys |
ATLASDR2 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3Val |
MultiframeEsoKeys |
ATLASDR3 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3Val |
MultiframeEsoKeys |
ATLASDR4 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3Val |
MultiframeEsoKeys |
ATLASDR5 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3Val |
MultiframeEsoKeys |
ATLASv20131127 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3Val |
MultiframeEsoKeys |
ATLASv20160425 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3Val |
MultiframeEsoKeys |
ATLASv20180209 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3Val |
MultiframeEsoKeys |
VPHASDR3 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3Val |
MultiframeEsoKeys |
VPHASv20160112 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insSens3Val |
MultiframeEsoKeys |
VPHASv20170222 |
Instr Cool. Fluid Flow DIF {image primary HDU keyword: HIERARCH ESO INS SENS3 VAL} |
real |
4 |
l/min |
-9.999995e+08 |
|
insShut1Swsim |
MultiframeEsoKeys |
ATLASDR1 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insShut1Swsim |
MultiframeEsoKeys |
ATLASDR2 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insShut1Swsim |
MultiframeEsoKeys |
ATLASDR3 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insShut1Swsim |
MultiframeEsoKeys |
ATLASDR4 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insShut1Swsim |
MultiframeEsoKeys |
ATLASDR5 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insShut1Swsim |
MultiframeEsoKeys |
ATLASv20131127 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insShut1Swsim |
MultiframeEsoKeys |
ATLASv20160425 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insShut1Swsim |
MultiframeEsoKeys |
ATLASv20180209 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insShut1Swsim |
MultiframeEsoKeys |
VPHASDR3 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insShut1Swsim |
MultiframeEsoKeys |
VPHASv20160112 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insShut1Swsim |
MultiframeEsoKeys |
VPHASv20170222 |
If T, function is software simulat {image primary HDU keyword: HIERARCH ESO INS SHUT1 SWSIM} |
tinyint |
1 |
|
0 |
|
insSwsim |
MultiframeEsoKeys |
ATLASDR1 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insSwsim |
MultiframeEsoKeys |
ATLASDR2 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insSwsim |
MultiframeEsoKeys |
ATLASDR3 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insSwsim |
MultiframeEsoKeys |
ATLASDR4 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insSwsim |
MultiframeEsoKeys |
ATLASDR5 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insSwsim |
MultiframeEsoKeys |
ATLASv20131127 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insSwsim |
MultiframeEsoKeys |
ATLASv20160425 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insSwsim |
MultiframeEsoKeys |
ATLASv20180209 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insSwsim |
MultiframeEsoKeys |
VPHASDR3 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insSwsim |
MultiframeEsoKeys |
VPHASv20160112 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insSwsim |
MultiframeEsoKeys |
VPHASv20170222 |
Software simulation {image primary HDU keyword: HIERARCH ESO INS SWSIM} |
varchar |
8 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
ATLASDR1 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
ATLASDR2 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
ATLASDR3 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
ATLASDR4 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
ATLASDR5 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
ATLASv20131127 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
ATLASv20160425 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
ATLASv20180209 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
VPHASDR3 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
VPHASv20160112 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11ID |
MultiframeEsoKeys |
VPHASv20170222 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP11 ID} |
varchar |
4 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
ATLASDR1 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
ATLASDR2 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
ATLASDR3 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
ATLASDR4 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
ATLASDR5 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
ATLASv20131127 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
ATLASv20160425 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
ATLASv20180209 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
VPHASDR3 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
VPHASv20160112 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Name |
MultiframeEsoKeys |
VPHASv20170222 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP11 NAME} |
varchar |
32 |
|
NONE |
|
insTemp11Val |
MultiframeEsoKeys |
ATLASDR1 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp11Val |
MultiframeEsoKeys |
ATLASDR2 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp11Val |
MultiframeEsoKeys |
ATLASDR3 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp11Val |
MultiframeEsoKeys |
ATLASDR4 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp11Val |
MultiframeEsoKeys |
ATLASDR5 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp11Val |
MultiframeEsoKeys |
ATLASv20131127 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp11Val |
MultiframeEsoKeys |
ATLASv20160425 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp11Val |
MultiframeEsoKeys |
ATLASv20180209 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp11Val |
MultiframeEsoKeys |
VPHASDR3 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp11Val |
MultiframeEsoKeys |
VPHASv20160112 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp11Val |
MultiframeEsoKeys |
VPHASv20170222 |
Filter system temperature {image primary HDU keyword: HIERARCH ESO INS TEMP11 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12ID |
MultiframeEsoKeys |
ATLASDR1 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12ID |
MultiframeEsoKeys |
ATLASDR2 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12ID |
MultiframeEsoKeys |
ATLASDR3 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12ID |
MultiframeEsoKeys |
ATLASDR4 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12ID |
MultiframeEsoKeys |
ATLASDR5 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12ID |
MultiframeEsoKeys |
ATLASv20131127 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12ID |
MultiframeEsoKeys |
ATLASv20160425 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12ID |
MultiframeEsoKeys |
ATLASv20180209 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12ID |
MultiframeEsoKeys |
VPHASDR3 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12ID |
MultiframeEsoKeys |
VPHASv20160112 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12ID |
MultiframeEsoKeys |
VPHASv20170222 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP12 ID} |
varchar |
8 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
ATLASDR1 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
ATLASDR2 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
ATLASDR3 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
ATLASDR4 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
ATLASDR5 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
ATLASv20131127 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
ATLASv20160425 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
ATLASv20180209 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
VPHASDR3 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
VPHASv20160112 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Name |
MultiframeEsoKeys |
VPHASv20170222 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP12 NAME} |
varchar |
32 |
|
NONE |
|
insTemp12Val |
MultiframeEsoKeys |
ATLASDR1 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12Val |
MultiframeEsoKeys |
ATLASDR2 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12Val |
MultiframeEsoKeys |
ATLASDR3 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12Val |
MultiframeEsoKeys |
ATLASDR4 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12Val |
MultiframeEsoKeys |
ATLASDR5 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12Val |
MultiframeEsoKeys |
ATLASv20131127 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12Val |
MultiframeEsoKeys |
ATLASv20160425 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12Val |
MultiframeEsoKeys |
ATLASv20180209 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12Val |
MultiframeEsoKeys |
VPHASDR3 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12Val |
MultiframeEsoKeys |
VPHASv20160112 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp12Val |
MultiframeEsoKeys |
VPHASv20170222 |
FIERA Cooling Liquid IN temperature {image primary HDU keyword: HIERARCH ESO INS TEMP12 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13ID |
MultiframeEsoKeys |
ATLASDR1 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13ID |
MultiframeEsoKeys |
ATLASDR2 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13ID |
MultiframeEsoKeys |
ATLASDR3 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13ID |
MultiframeEsoKeys |
ATLASDR4 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13ID |
MultiframeEsoKeys |
ATLASDR5 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13ID |
MultiframeEsoKeys |
ATLASv20131127 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13ID |
MultiframeEsoKeys |
ATLASv20160425 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13ID |
MultiframeEsoKeys |
ATLASv20180209 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13ID |
MultiframeEsoKeys |
VPHASDR3 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13ID |
MultiframeEsoKeys |
VPHASv20160112 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13ID |
MultiframeEsoKeys |
VPHASv20170222 |
Temperature sensor ID {image primary HDU keyword: HIERARCH ESO INS TEMP13 ID} |
varchar |
8 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
ATLASDR1 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
ATLASDR2 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
ATLASDR3 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
ATLASDR4 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
ATLASDR5 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
ATLASv20131127 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
ATLASv20160425 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
ATLASv20180209 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
VPHASDR3 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
VPHASv20160112 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Name |
MultiframeEsoKeys |
VPHASv20170222 |
Temperature sensor name {image primary HDU keyword: HIERARCH ESO INS TEMP13 NAME} |
varchar |
32 |
|
NONE |
|
insTemp13Val |
MultiframeEsoKeys |
ATLASDR1 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13Val |
MultiframeEsoKeys |
ATLASDR2 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13Val |
MultiframeEsoKeys |
ATLASDR3 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13Val |
MultiframeEsoKeys |
ATLASDR4 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13Val |
MultiframeEsoKeys |
ATLASDR5 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13Val |
MultiframeEsoKeys |
ATLASv20131127 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13Val |
MultiframeEsoKeys |
ATLASv20160425 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13Val |
MultiframeEsoKeys |
ATLASv20180209 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13Val |
MultiframeEsoKeys |
VPHASDR3 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13Val |
MultiframeEsoKeys |
VPHASv20160112 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
insTemp13Val |
MultiframeEsoKeys |
VPHASv20170222 |
FIERA Cooling Liquid OUT temperature {image primary HDU keyword: HIERARCH ESO INS TEMP13 VAL} |
real |
4 |
degC |
-9.999995e+08 |
|
institution |
ExternalProduct |
ATLASDR2 |
Name of the institution that created the product |
varchar |
256 |
|
|
?? |
institution |
ExternalProduct |
ATLASDR3 |
Name of the institution that created the product |
varchar |
256 |
|
|
?? |
institution |
ExternalProduct |
ATLASDR4 |
Name of the institution that created the product |
varchar |
256 |
|
|
?? |
institution |
ExternalProduct |
ATLASDR5 |
Name of the institution that created the product |
varchar |
256 |
|
|
?? |
institution |
ExternalProduct |
ATLASv20131127 |
Name of the institution that created the product |
varchar |
256 |
|
|
?? |
institution |
ExternalProduct |
ATLASv20160425 |
Name of the institution that created the product |
varchar |
256 |
|
|
?? |
institution |
ExternalProduct |
ATLASv20180209 |
Name of the institution that created the product |
varchar |
256 |
|
|
?? |
institution |
ExternalProduct |
VPHASDR3 |
Name of the institution that created the product |
varchar |
256 |
|
|
?? |
institution |
ExternalProduct |
VPHASv20160112 |
Name of the institution that created the product |
varchar |
256 |
|
|
?? |
institution |
ExternalProduct |
VPHASv20170222 |
Name of the institution that created the product |
varchar |
256 |
|
|
?? |
instrument |
Multiframe |
ATLASDR1 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
instrument |
Multiframe |
ATLASDR2 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
instrument |
Multiframe |
ATLASDR3 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
instrument |
Multiframe |
ATLASDR4 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
instrument |
Multiframe |
ATLASDR5 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
instrument |
Multiframe |
ATLASv20131127 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
instrument |
Multiframe |
ATLASv20160425 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
instrument |
Multiframe |
ATLASv20180209 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
instrument |
Multiframe |
VPHASDR3 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
instrument |
Multiframe |
VPHASv20160112 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
instrument |
Multiframe |
VPHASv20170222 |
Instrument name {image primary HDU keyword: INSTRUME} |
varchar |
8 |
|
NONE |
|
int_average_g |
cepheid, rrlyrae |
GAIADR1 |
Intensity-averaged magnitude in the G band |
float |
8 |
mag |
|
phot.mag;em.opt |
int_average_g_error |
cepheid, rrlyrae |
GAIADR1 |
Uncertainty on the intensity-averaged magnitude in the G band |
float |
8 |
mag |
|
stat.error;phot.mag;em.opt |
intProdType |
ProductLinks |
ATLASDR1 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProdType |
ProductLinks |
ATLASDR2 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProdType |
ProductLinks |
ATLASDR3 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProdType |
ProductLinks |
ATLASDR4 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProdType |
ProductLinks |
ATLASDR5 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProdType |
ProductLinks |
ATLASv20131127 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProdType |
ProductLinks |
ATLASv20160425 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProdType |
ProductLinks |
ATLASv20180209 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProdType |
ProductLinks |
VPHASDR3 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProdType |
ProductLinks |
VPHASv20160112 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProdType |
ProductLinks |
VPHASv20170222 |
Type (stack,tile,mosaic) of intermediate frame |
varchar |
8 |
|
|
?? |
intProductID |
ProductLinks |
ATLASDR1 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
intProductID |
ProductLinks |
ATLASDR2 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
intProductID |
ProductLinks |
ATLASDR3 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
intProductID |
ProductLinks |
ATLASDR4 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
intProductID |
ProductLinks |
ATLASDR5 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
intProductID |
ProductLinks |
ATLASv20131127 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
intProductID |
ProductLinks |
ATLASv20160425 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
intProductID |
ProductLinks |
ATLASv20180209 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
intProductID |
ProductLinks |
VPHASDR3 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
intProductID |
ProductLinks |
VPHASv20160112 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
intProductID |
ProductLinks |
VPHASv20170222 |
Product ID of intermediate frame |
int |
4 |
|
|
?? |
iPA |
atlasSource |
ATLASDR1 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng |
iPA |
atlasSource |
ATLASDR2 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng |
iPA |
atlasSource |
ATLASDR3 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng;em.opt.I |
iPA |
atlasSource |
ATLASDR4 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng;em.opt.I |
iPA |
atlasSource |
ATLASDR5 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng;em.opt.I |
iPA |
atlasSource |
ATLASv20131127 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng |
iPA |
atlasSource |
ATLASv20160425 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng;em.opt.I |
iPA |
atlasSource |
ATLASv20180209 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng;em.opt.I |
iPA |
vphasSource |
VPHASDR3 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng;em.opt.I |
iPA |
vphasSource |
VPHASv20160112 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng;em.opt.I |
iPA |
vphasSource |
VPHASv20170222 |
ellipse fit celestial orientation in I |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng;em.opt.I |
iPetroMag |
atlasSource |
ATLASDR1 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iPetroMag |
atlasSource |
ATLASDR2 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iPetroMag |
atlasSource |
ATLASDR3 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPetroMag |
atlasSource |
ATLASDR4 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPetroMag |
atlasSource |
ATLASDR5 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPetroMag |
atlasSource |
ATLASv20131127 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iPetroMag |
atlasSource |
ATLASv20160425 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPetroMag |
atlasSource |
ATLASv20180209 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPetroMag |
vphasSource |
VPHASDR3 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPetroMag |
vphasSource |
VPHASv20160112 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPetroMag |
vphasSource |
VPHASv20170222 |
Extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPetroMagErr |
atlasSource |
ATLASDR1 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iPetroMagErr |
atlasSource |
ATLASDR2 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iPetroMagErr |
atlasSource |
ATLASDR3 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPetroMagErr |
atlasSource |
ATLASDR4 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPetroMagErr |
atlasSource |
ATLASDR5 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPetroMagErr |
atlasSource |
ATLASv20131127 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iPetroMagErr |
atlasSource |
ATLASv20160425 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPetroMagErr |
atlasSource |
ATLASv20180209 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPetroMagErr |
vphasSource |
VPHASDR3 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPetroMagErr |
vphasSource |
VPHASv20160112 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPetroMagErr |
vphasSource |
VPHASv20170222 |
Error in extended source I mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
ipmag_APASSDR9 |
ravedr5Source |
RAVE |
i' magnitude from APASSDR9 |
real |
4 |
mag |
|
phot.mag;em.opt |
ippErrBits |
atlasSource |
ATLASDR1 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
ippErrBits |
atlasSource |
ATLASDR2 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
ippErrBits |
atlasSource |
ATLASDR3 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code;em.opt.I |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
ippErrBits |
atlasSource |
ATLASDR4 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code;em.opt.I |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
ippErrBits |
atlasSource |
ATLASDR5 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code;em.opt.I |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
ippErrBits |
atlasSource |
ATLASv20131127 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
ippErrBits |
atlasSource |
ATLASv20160425 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code;em.opt.I |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
ippErrBits |
atlasSource |
ATLASv20180209 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code;em.opt.I |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
ippErrBits |
vphasSource |
VPHASDR3 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code;em.opt.I |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
ippErrBits |
vphasSource |
VPHASv20160112 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code;em.opt.I |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
ippErrBits |
vphasSource |
VPHASv20170222 |
additional WFAU post-processing error bits in I |
int |
4 |
|
0 |
meta.code;em.opt.I |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
iPsfMag |
atlasSource |
ATLASDR1 |
Point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iPsfMag |
atlasSource |
ATLASDR2 |
Point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iPsfMag |
atlasSource |
ATLASDR3 |
Point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPsfMag |
atlasSource |
ATLASv20131127 |
Point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iPsfMag |
atlasSource |
ATLASv20160425 |
Point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPsfMag |
vphasSource |
VPHASDR3 |
Point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPsfMag |
vphasSource |
VPHASv20160112 |
Point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPsfMag |
vphasSource |
VPHASv20170222 |
Point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iPsfMagErr |
atlasSource |
ATLASDR1 |
Error in point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iPsfMagErr |
atlasSource |
ATLASDR2 |
Error in point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iPsfMagErr |
atlasSource |
ATLASDR3 |
Error in point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPsfMagErr |
atlasSource |
ATLASv20131127 |
Error in point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iPsfMagErr |
atlasSource |
ATLASv20160425 |
Error in point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPsfMagErr |
vphasSource |
VPHASDR3 |
Error in point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPsfMagErr |
vphasSource |
VPHASv20160112 |
Error in point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iPsfMagErr |
vphasSource |
VPHASv20170222 |
Error in point source profile-fitted I mag |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iqr |
phot_variable_time_series_g_fov_statistical_parameters |
GAIADR1 |
Inter-quartile range of the G-band time series values |
float |
8 |
mag |
|
phot.mag;stat.value |
IR_direct |
ravedr5Source |
RAVE |
Infrared flux method flag (Note 5, DR5) |
varchar |
6 |
|
|
meta.code |
isApassCal |
atlasDetection |
ATLASDR3 |
Code for a APASS calibrated (=1) or standard calibrated (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isApassCal |
atlasDetection |
ATLASDR4 |
Code for a APASS calibrated (=1) or standard calibrated (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isApassCal |
atlasDetection |
ATLASDR5 |
Code for a APASS calibrated (=1) or standard calibrated (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isApassCal |
atlasDetection |
ATLASv20160425 |
Code for a APASS calibrated (=1) or standard calibrated (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isApassCal |
atlasDetection |
ATLASv20180209 |
Code for a APASS calibrated (=1) or standard calibrated (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isApassCal |
atlasDetection, atlasDetectionUncorr |
ATLASDR2 |
Code for a APASS calibrated (=1) or standard calibrated (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isApassCal |
vphasDetection |
VPHASv20160112 |
Code for a APASS calibrated (=1) or standard calibrated (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isApassCal |
vphasDetection |
VPHASv20170222 |
Code for a APASS calibrated (=1) or standard calibrated (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isApassCal |
vphasDetection, vphasDetectionUncorr |
VPHASDR3 |
Code for a APASS calibrated (=1) or standard calibrated (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isComplete |
atlasAstrometricInfo |
ATLASDR4 |
Level of completeness: 0 redo both parts 1; halfspace calculation complete; 2 Astrometric correction complete; 3 All complete |
tinyint |
1 |
|
0 |
meta.code.qual |
isComplete |
atlasAstrometricInfo |
ATLASDR5 |
Level of completeness: 0 redo both parts 1; halfspace calculation complete; 2 Astrometric correction complete; 3 All complete |
tinyint |
1 |
|
0 |
meta.code.qual |
isComplete |
atlasAstrometricInfo |
ATLASv20180209 |
Level of completeness: 0 redo both parts 1; halfspace calculation complete; 2 Astrometric correction complete; 3 All complete |
tinyint |
1 |
|
0 |
meta.code.qual |
isComplete |
vphasAstrometricInfo |
VPHASDR3 |
Level of completeness: 0 redo both parts 1; halfspace calculation complete; 2 Astrometric correction complete; 3 All complete |
tinyint |
1 |
|
0 |
meta.code.qual |
isComplete |
vphasAstrometricInfo |
VPHASv20170222 |
Level of completeness: 0 redo both parts 1; halfspace calculation complete; 2 Astrometric correction complete; 3 All complete |
tinyint |
1 |
|
0 |
meta.code.qual |
iSeqNum |
atlasSource |
ATLASDR1 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.id |
iSeqNum |
atlasSource |
ATLASDR2 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.id |
iSeqNum |
atlasSource |
ATLASDR3 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.number;em.opt.I |
iSeqNum |
atlasSource |
ATLASDR4 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.number;em.opt.I |
iSeqNum |
atlasSource |
ATLASDR5 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.id;em.opt.I |
iSeqNum |
atlasSource |
ATLASv20131127 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.id |
iSeqNum |
atlasSource |
ATLASv20160425 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.number;em.opt.I |
iSeqNum |
atlasSource |
ATLASv20180209 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.number;em.opt.I |
iSeqNum |
vphasSource |
VPHASDR3 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.number;em.opt.I |
iSeqNum |
vphasSource |
VPHASv20160112 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.number;em.opt.I |
iSeqNum |
vphasSource |
VPHASv20170222 |
the running number of the I detection |
int |
4 |
|
-99999999 |
meta.number;em.opt.I |
iSerMag2D |
atlasSource |
ATLASDR1 |
Extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iSerMag2D |
atlasSource |
ATLASDR2 |
Extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iSerMag2D |
atlasSource |
ATLASDR3 |
Extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iSerMag2D |
atlasSource |
ATLASv20131127 |
Extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
iSerMag2D |
atlasSource |
ATLASv20160425 |
Extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iSerMag2D |
vphasSource |
VPHASDR3 |
Extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iSerMag2D |
vphasSource |
VPHASv20160112 |
Extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iSerMag2D |
vphasSource |
VPHASv20170222 |
Extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;em.opt.I |
iSerMag2DErr |
atlasSource |
ATLASDR1 |
Error in extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iSerMag2DErr |
atlasSource |
ATLASDR2 |
Error in extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iSerMag2DErr |
atlasSource |
ATLASDR3 |
Error in extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iSerMag2DErr |
atlasSource |
ATLASv20131127 |
Error in extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
iSerMag2DErr |
atlasSource |
ATLASv20160425 |
Error in extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iSerMag2DErr |
vphasSource |
VPHASDR3 |
Error in extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iSerMag2DErr |
vphasSource |
VPHASv20160112 |
Error in extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
iSerMag2DErr |
vphasSource |
VPHASv20170222 |
Error in extended source I mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag;em.opt.I |
isIllumCorr |
atlasDetection |
ATLASDR3 |
Code for a illumination corrected (=1) or not illumination corrected (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isIllumCorr |
atlasDetection |
ATLASDR4 |
Code for a illumination corrected (=1) or not illumination corrected (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isIllumCorr |
atlasDetection |
ATLASDR5 |
Code for a illumination corrected (=1) or not illumination corrected (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isIllumCorr |
atlasDetection |
ATLASv20160425 |
Code for a illumination corrected (=1) or not illumination corrected (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isIllumCorr |
atlasDetection |
ATLASv20180209 |
Code for a illumination corrected (=1) or not illumination corrected (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isIllumCorr |
atlasDetection, atlasDetectionUncorr |
ATLASDR2 |
Code for a illumination corrected (=1) or not illumination corrected (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isIllumCorr |
vphasDetection |
VPHASv20160112 |
Code for a illumination corrected (=1) or not illumination corrected (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isIllumCorr |
vphasDetection |
VPHASv20170222 |
Code for a illumination corrected (=1) or not illumination corrected (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isIllumCorr |
vphasDetection, vphasDetectionUncorr |
VPHASDR3 |
Code for a illumination corrected (=1) or not illumination corrected (=0) detection |
tinyint |
1 |
|
0 |
meta.code |
isLowGalacticLat |
Programme |
ATLASDR1 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
isLowGalacticLat |
Programme |
ATLASDR2 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
isLowGalacticLat |
Programme |
ATLASDR3 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
isLowGalacticLat |
Programme |
ATLASDR4 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
isLowGalacticLat |
Programme |
ATLASDR5 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
isLowGalacticLat |
Programme |
ATLASv20131127 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
isLowGalacticLat |
Programme |
ATLASv20160425 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
isLowGalacticLat |
Programme |
ATLASv20180209 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
isLowGalacticLat |
Programme |
VPHASDR3 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
isLowGalacticLat |
Programme |
VPHASv20160112 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
isLowGalacticLat |
Programme |
VPHASv20170222 |
Is this a low Galactic latitude field where Schlegel maps don't work (No=0/Yes=1) |
tinyint |
1 |
|
0 |
|
ISOAREA_IMAGE |
mgcDetection |
MGC |
Isophotal area above analysis threshold |
int |
4 |
pixel^2 |
|
|
ISOAREA_WORLD |
mgcDetection |
MGC |
Isophotal area above analysis threshold |
real |
4 |
deg^2 |
|
|
isoFlux |
atlasDetection |
ATLASDR1 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoFlux |
atlasDetection |
ATLASDR3 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoFlux |
atlasDetection |
ATLASDR4 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoFlux |
atlasDetection |
ATLASDR5 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoFlux |
atlasDetection |
ATLASv20131127 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoFlux |
atlasDetection |
ATLASv20160425 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoFlux |
atlasDetection |
ATLASv20180209 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoFlux |
atlasDetection, atlasDetectionUncorr |
ATLASDR2 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoFlux |
vphasDetection |
VPHASv20160112 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoFlux |
vphasDetection |
VPHASv20170222 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoFlux |
vphasDetection, vphasDetectionUncorr |
VPHASDR3 |
Instrumental isophotal flux counts {catalogue TType keyword: Isophotal_flux} |
real |
4 |
ADU |
|
phot.count;em.opt |
Standard definition of summed flux within detection isophote, apart from detection filter is used to define pixel connectivity and hence which pixels to include. This helps to reduce edge effects for all isophotally derived parameters. |
isoMag |
atlasDetection |
ATLASDR1 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isoMag |
atlasDetection |
ATLASDR3 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isoMag |
atlasDetection |
ATLASDR4 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isoMag |
atlasDetection |
ATLASDR5 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isoMag |
atlasDetection |
ATLASv20131127 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isoMag |
atlasDetection |
ATLASv20160425 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isoMag |
atlasDetection |
ATLASv20180209 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isoMag |
atlasDetection, atlasDetectionUncorr |
ATLASDR2 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isoMag |
vphasDetection |
VPHASv20160112 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isoMag |
vphasDetection |
VPHASv20170222 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isoMag |
vphasDetection, vphasDetectionUncorr |
VPHASDR3 |
Calibrated isophotal magnitude |
real |
4 |
mag |
|
phot.mag |
isSectioned |
Filter |
ATLASDR1 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSectioned |
Filter |
ATLASDR2 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSectioned |
Filter |
ATLASDR3 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSectioned |
Filter |
ATLASDR4 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSectioned |
Filter |
ATLASDR5 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSectioned |
Filter |
ATLASv20131127 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSectioned |
Filter |
ATLASv20160425 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSectioned |
Filter |
ATLASv20180209 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSectioned |
Filter |
VPHASDR3 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSectioned |
Filter |
VPHASv20160112 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSectioned |
Filter |
VPHASv20170222 |
Is the focal plane sectioned into different filters, 0 No, 1 Yes. If so, data for each section in FilterSections and SectionDetectors |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
ATLASDR1 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
ATLASDR2 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
ATLASDR3 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
ATLASDR4 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
ATLASDR5 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
ATLASv20131127 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
ATLASv20160425 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
ATLASv20180209 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
VPHASDR3 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
VPHASv20160112 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
isSynoptic |
RequiredFilters |
VPHASv20170222 |
is the band observed multiple times for variability measurements (0 FALSE, 1 TRUE) |
tinyint |
1 |
|
0 |
|
itb |
rosat_fsc |
ROSAT |
start time of observation (MM-DD-YYYY HH:MM:SS) |
datetime |
8 |
mm-dd-yyyy hh:mm:ss |
|
time.epoch |
ite |
rosat_fsc |
ROSAT |
end time of observation (MM-DD-YYYY HH:MM:SS) |
datetime |
8 |
mm-dd-yyyy hh:mm:ss |
|
time.epoch |
iXi |
atlasSource |
ATLASDR1 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iXi |
atlasSource |
ATLASDR2 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iXi |
atlasSource |
ATLASDR3 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iXi |
atlasSource |
ATLASDR4 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iXi |
atlasSource |
ATLASDR5 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iXi |
atlasSource |
ATLASv20131127 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iXi |
atlasSource |
ATLASv20160425 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iXi |
atlasSource |
ATLASv20180209 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iXi |
vphasSource |
VPHASDR3 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iXi |
vphasSource |
VPHASv20160112 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
iXi |
vphasSource |
VPHASv20170222 |
Offset of I detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff;em.opt.I |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |