E |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
e_Ap35mag_I |
denisDR3Source |
DENIS |
Error in I band mag from 3.5" aperture |
float |
8 |
mag |
|
|
e_Ap35mag_J |
denisDR3Source |
DENIS |
Error in J band mag from 3.5" aperture |
float |
8 |
mag |
|
|
e_Ap35mag_K |
denisDR3Source |
DENIS |
Error in K band mag from 3.5" aperture |
float |
8 |
mag |
|
|
e_Ap45mag_I |
denisDR3Source |
DENIS |
Error in I band mag from 4.5" aperture |
float |
8 |
mag |
|
|
e_Ap45mag_J |
denisDR3Source |
DENIS |
Error in J band mag from 4.5" aperture |
float |
8 |
mag |
|
|
e_Ap45mag_K |
denisDR3Source |
DENIS |
Error in K band mag from 4.5" aperture |
float |
8 |
mag |
|
|
e_Ap55mag_I |
denisDR3Source |
DENIS |
Error in I band mag from 5.5" aperture |
float |
8 |
mag |
|
|
e_Ap55mag_J |
denisDR3Source |
DENIS |
Error in J band mag from 5.5" aperture |
float |
8 |
mag |
|
|
e_Ap55mag_K |
denisDR3Source |
DENIS |
Error in K band mag from 5.5" aperture |
float |
8 |
mag |
|
|
e_Apc15mag_I |
denisDR3Source |
DENIS |
I band mag error in 1.5" corr. aperture |
float |
8 |
mag |
|
|
e_Apc15mag_J |
denisDR3Source |
DENIS |
J band mag error in 1.5" corr. aperture |
float |
8 |
mag |
|
|
e_Apc15mag_K |
denisDR3Source |
DENIS |
K band mag error in 1.5" corr. aperture |
float |
8 |
mag |
|
|
e_Apc25mag_I |
denisDR3Source |
DENIS |
I band mag error in 2.5" corr. aperture |
float |
8 |
mag |
|
|
e_Apc25mag_J |
denisDR3Source |
DENIS |
J band mag error in 2.5" corr. aperture |
float |
8 |
mag |
|
|
e_Apc25mag_K |
denisDR3Source |
DENIS |
K band mag error in 2.5" corr. aperture |
float |
8 |
mag |
|
|
e_Apc35mag_I |
denisDR3Source |
DENIS |
I band mag error in 3.5" corr. aperture |
float |
8 |
mag |
|
|
e_Apc35mag_J |
denisDR3Source |
DENIS |
J band mag error in 3.5" corr. aperture |
float |
8 |
mag |
|
|
e_Apc35mag_K |
denisDR3Source |
DENIS |
K band mag error in 3.5" corr. aperture |
float |
8 |
mag |
|
|
e_b_v |
hipparcos_new_reduction |
GAIADR1 |
Formal error on B-V colour index |
float |
8 |
mag |
|
em.opt;phot.colour;stat.error |
e_bp_min_rp_percentile_lower |
gaia_source |
GAIADR2 |
Lower uncertainty on e_bp_min_rp_val |
real |
4 |
mag |
|
|
e_bp_min_rp_percentile_Upper |
gaia_source |
GAIADR2 |
Upper uncertainty on e_bp_min_rp_val |
real |
4 |
mag |
|
|
e_bp_min_rp_val |
gaia_source |
GAIADR2 |
Line-of-sight reddening E(BP-RP) |
real |
4 |
mag |
|
|
e_bt_mag |
tycho2 |
GAIADR1 |
Standard error on BT |
real |
4 |
mag |
|
stat.error |
e_de_deg |
tycho2 |
GAIADR1 |
Standard error of observed Tycho2 Dec |
float |
8 |
milliarcsec |
|
stat.error |
e_de_m_deg |
tycho2 |
GAIADR1 |
Standard error of mean Tycho2 Dec |
float |
8 |
milliarcsec |
|
stat.error |
e_de_rad |
hipparcos_new_reduction |
GAIADR1 |
Formal error on de_rad |
float |
8 |
milliarcsec |
|
pos.eq.dec;stat.error |
e_DEcs |
nvssSource |
NVSS |
Mean error on Dec |
real |
4 |
arcsec |
|
stat.error |
e_Fitmag_I |
denisDR3Source |
DENIS |
Magnitude error in I band from PSF fit |
float |
8 |
mag |
|
|
e_Fitmag_J |
denisDR3Source |
DENIS |
Magnitude error in J band from PSF fit |
float |
8 |
mag |
|
|
e_Fitmag_K |
denisDR3Source |
DENIS |
Magnitude error in K band from PSF fit |
float |
8 |
mag |
|
|
e_hp_mag |
hipparcos_new_reduction |
GAIADR1 |
Error on mean Hipparcos magnitude |
float |
8 |
mag |
|
em.opt.V;phot.mag;stat.error |
e_majAxis |
nvssSource |
NVSS |
Mean error on majAxis |
real |
4 |
arcsec |
|
stat.error |
e_minAxis |
nvssSource |
NVSS |
Mean error on minAxis |
real |
4 |
arcsec |
|
stat.error |
e_PA |
nvssSource |
NVSS |
Mean error on PA |
real |
4 |
degrees |
|
stat.error |
e_plx |
hipparcos_new_reduction |
GAIADR1 |
Formal error on parallax |
float |
8 |
milliarcsec |
|
pos.parallax;stat.error |
e_pm_de |
hipparcos_new_reduction |
GAIADR1 |
Formal error on pm_de |
float |
8 |
milliarcsec/year |
|
pos.eq.dec;pos.pm;stat.error |
e_pm_de |
tycho2 |
GAIADR1 |
Standard error of Dec proper motion |
real |
4 |
milliarcsec/year |
|
stat.error |
e_pm_ra |
hipparcos_new_reduction |
GAIADR1 |
Formal error on pm_ra |
float |
8 |
milliarcsec/year |
|
pos.eq.ra;pos.pm;stat.error |
e_pm_ra |
tycho2 |
GAIADR1 |
Standard error in RA*cos(Dec) of RA proper motion |
real |
4 |
milliarcsec/year |
|
stat.error |
e_polFlux |
nvssSource |
NVSS |
Mean error on polFlux |
real |
4 |
mJy |
|
stat.error |
e_polPA |
nvssSource |
NVSS |
Mean error on polPA |
real |
4 |
mJy |
|
stat.error |
e_ra_deg |
tycho2 |
GAIADR1 |
Standard error in RA*cos(Dec) of observed Tycho2 RA |
float |
8 |
milliarcsec |
|
stat.error |
e_ra_m_deg |
tycho2 |
GAIADR1 |
Standard error in RA*cos(Dec) of mean Tycho2 RA |
float |
8 |
milliarcsec |
|
stat.error |
e_ra_rad |
hipparcos_new_reduction |
GAIADR1 |
Formal error on ra_rad |
float |
8 |
milliarcsec |
|
pos.eq.ra;stat.error |
e_RAs |
nvssSource |
NVSS |
Mean error on RA |
real |
4 |
s |
|
stat.error |
e_S14 |
nvssSource |
NVSS |
Mean error on S14 |
real |
4 |
mJy |
|
stat.error |
e_score |
twomass_xsc |
TWOMASS |
extended score: 1(extended) < e_score < 2(point-like). |
real |
4 |
|
|
meta.code |
e_vt_mag |
tycho2 |
GAIADR1 |
Standard error on VT |
real |
4 |
mag |
|
stat.error |
eBmag_APASSDR9 |
ravedr5Source |
RAVE |
error B magnitude from APASSDR9 |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt.B |
ebmvMed |
MultiframeDetector |
ATLASDR1 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
ATLASDR2 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
ATLASDR3 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
ATLASDR4 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
ATLASDR5 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
ATLASv20131127 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
ATLASv20160425 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
ATLASv20180209 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VPHASDR3 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VPHASv20160112 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VPHASv20170222 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
eBTmag_TYCHO2 |
ravedr5Source |
RAVE |
Error of BT magnitude from TYCHO2 |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt.B |
eBV |
atlasSource |
ATLASDR1 |
The galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. This uses the correction given in Bonifacio, Monai & Beers (2000). This correction reduces the extinction value in regions of high extinction (E(B-V)>0.1) |
real |
4 |
|
-0.9999995e9 |
|
eBV |
atlasSource |
ATLASDR2 |
The galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. This uses the correction given in Bonifacio, Monai & Beers (2000). This correction reduces the extinction value in regions of high extinction (E(B-V)>0.1) |
real |
4 |
|
-0.9999995e9 |
|
eBV |
atlasSource |
ATLASDR3 |
The galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. This uses the correction given in Bonifacio, Monai & Beers (2000). This correction reduces the extinction value in regions of high extinction (E(B-V)>0.1) |
real |
4 |
|
-0.9999995e9 |
phys.absorption.gal |
eBV |
atlasSource |
ATLASDR4 |
The galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. This uses the correction given in Bonifacio, Monai & Beers (2000). This correction reduces the extinction value in regions of high extinction (E(B-V)>0.1) |
real |
4 |
|
-0.9999995e9 |
phys.absorption.gal |
eBV |
atlasSource |
ATLASDR5 |
The galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. This uses the correction given in Bonifacio, Monai & Beers (2000). This correction reduces the extinction value in regions of high extinction (E(B-V)>0.1) |
real |
4 |
|
-0.9999995e9 |
phys.absorption.gal |
eBV |
atlasSource |
ATLASv20131127 |
The galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. This uses the correction given in Bonifacio, Monai & Beers (2000). This correction reduces the extinction value in regions of high extinction (E(B-V)>0.1) |
real |
4 |
|
-0.9999995e9 |
|
eBV |
atlasSource |
ATLASv20160425 |
The galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. This uses the correction given in Bonifacio, Monai & Beers (2000). This correction reduces the extinction value in regions of high extinction (E(B-V)>0.1) |
real |
4 |
|
-0.9999995e9 |
phys.absorption.gal |
eBV |
atlasSource |
ATLASv20180209 |
The galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. This uses the correction given in Bonifacio, Monai & Beers (2000). This correction reduces the extinction value in regions of high extinction (E(B-V)>0.1) |
real |
4 |
|
-0.9999995e9 |
phys.absorption.gal |
ebv |
twompzPhotoz |
TWOMPZ |
The Galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. {image primary HDU keyword: EBV} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
ecl_lat |
gaia_source |
GAIADR2 |
Ecliptic latitude |
float |
8 |
degrees |
|
pos.ecliptic.lat |
ecl_lat |
gaia_source, tgas_source |
GAIADR1 |
Ecliptic latitude |
float |
8 |
degrees |
|
pos.ecliptic.lat |
ecl_lon |
gaia_source |
GAIADR2 |
Ecliptic longitude |
float |
8 |
degrees |
|
pos.ecliptic.lon |
ecl_lon |
gaia_source, tgas_source |
GAIADR1 |
Ecliptic longitude |
float |
8 |
degrees |
|
pos.ecliptic.lon |
ecliptic_lat |
igsl_source |
GAIADR1 |
Ecliptic latitude |
real |
4 |
degrees |
|
pos.ecliptic.lat |
ecliptic_lon |
igsl_source |
GAIADR1 |
Ecliptic longitude |
real |
4 |
degrees |
|
pos.ecliptic.lon |
edistance |
ravedr5Source |
RAVE |
Error of spectrophotometric Distance (Binney et al. 2014) |
real |
4 |
pc |
|
pos.distance |
eDistanceModulus_Binney |
ravedr5Source |
RAVE |
Error of distance Modulus from Binney et al. 2014 |
real |
4 |
mag |
|
phot.mag.distMod |
eFlag |
rosat_bsc, rosat_fsc |
ROSAT |
source extended beyond SASS extraction radius |
varchar |
1 |
|
|
meta.code |
egpmag_APASSDR9 |
ravedr5Source |
RAVE |
g' magnitude from APASSDR9 |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt |
eHmag_2MASS |
ravedr5Source |
RAVE |
error 2MASS H magnitude |
real |
4 |
mag |
|
stat.error;phot.mag;em.IR.H |
eHRV |
ravedr5Source |
RAVE |
Error of Heliocentric radial velocity stat.error |
real |
4 |
km/s |
|
stat.error;spect.dopplerVeloc;pos.heliocentric |
eImag_DENIS |
ravedr5Source |
RAVE |
error DENIS I magnitude |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt.I |
eipmag_APASSDR9 |
ravedr5Source |
RAVE |
i' magnitude from APASSDR9 |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt |
eJmag_2MASS |
ravedr5Source |
RAVE |
error 2MASS J magnitude |
real |
4 |
mag |
|
stat.error;phot.mag;em.IR.J |
eJmag_DENIS |
ravedr5Source |
RAVE |
error DENIS J magnitude |
real |
4 |
mag |
|
stat.error;phot.mag;em.IR.J |
eKmag_2MASS |
ravedr5Source |
RAVE |
error 2MASS K magnitude |
real |
4 |
mag |
|
stat.error;phot.mag;em.IR.K |
eKmag_DENIS |
ravedr5Source |
RAVE |
error DENIS K magnitude |
real |
4 |
mag |
|
stat.error;phot.mag;em.IR.K |
elat |
allwise_sc |
WISE |
Ecliptic latitude computed from the non-moving source fit equatorial position. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
deg |
|
|
elat |
catwise_2020, catwise_prelim |
WISE |
ecliptic latitude |
float |
8 |
deg |
|
|
elat |
wise_allskysc |
WISE |
Ecliptic latitude. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
degrees |
|
|
elat |
wise_prelimsc |
WISE |
Ecliptic latitude. CAUTION: This coordinate should not be used as an astrometric reference |
float |
8 |
degrees |
|
|
elat_avg |
catwise_2020, catwise_prelim |
WISE |
averaged ecliptic latitude |
float |
8 |
deg |
|
|
elatSig |
catwise_2020, catwise_prelim |
WISE |
one-sigma uncertainty in elat |
real |
4 |
arcsec |
|
|
ell |
atlasDetection |
ATLASDR1 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
atlasDetection |
ATLASDR3 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
atlasDetection |
ATLASDR4 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
atlasDetection |
ATLASDR5 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
atlasDetection |
ATLASv20131127 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
atlasDetection |
ATLASv20160425 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
atlasDetection |
ATLASv20180209 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
atlasDetection, atlasDetectionUncorr |
ATLASDR2 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vphasDetection |
VPHASv20160112 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vphasDetection |
VPHASv20170222 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vphasDetection, vphasDetectionUncorr |
VPHASDR3 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ellfit_flg |
twomass_xsc |
TWOMASS |
ellipse fitting contamination flag. |
smallint |
2 |
|
|
meta.code |
ELLIPTICITY |
mgcDetection |
MGC |
1 - B_IMAGE/A_IMAGE |
real |
4 |
|
|
|
elog_Av |
ravedr5Source |
RAVE |
Error of log_10(Av) optical extinction, see p4 ff, Mon. Not. R. Astron. Soc. 000, 1-8 (2012) |
real |
4 |
|
|
stat.error;phys.absorption |
elogg_K |
ravedr5Source |
RAVE |
Log gravity (Note 2, DR5) |
float |
8 |
dex |
|
phys.gravity |
elon |
allwise_sc |
WISE |
Ecliptic longitude computed from the non-moving source fit equatorial position. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
deg |
|
|
elon |
catwise_2020, catwise_prelim |
WISE |
ecliptic longitude |
float |
8 |
deg |
|
|
elon |
wise_allskysc |
WISE |
Ecliptic longitude. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
degrees |
|
|
elon |
wise_prelimsc |
WISE |
Ecliptic longitude. CAUTION: This coordinate should not be used as an astrometric reference |
float |
8 |
degrees |
|
|
elon_avg |
catwise_2020, catwise_prelim |
WISE |
averaged ecliptic longitude |
float |
8 |
deg |
|
|
elonSig |
catwise_2020, catwise_prelim |
WISE |
one-sigma uncertainty in elon |
real |
4 |
arcsec |
|
|
eMet_K |
ravedr5Source |
RAVE |
Error of [m/H] |
float |
8 |
dex |
|
phys.abund.Z |
endDate |
AstrCalVers |
ATLASDR1 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
ATLASDR2 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
ATLASDR3 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
ATLASDR4 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
ATLASDR5 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
ATLASv20131127 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
ATLASv20160425 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
ATLASv20180209 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VPHASDR3 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VPHASv20160112 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VPHASv20170222 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
PhotCalVers |
ATLASDR1 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
endDate |
PhotCalVers |
ATLASDR2 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
endDate |
PhotCalVers |
ATLASDR3 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
endDate |
PhotCalVers |
ATLASDR4 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
endDate |
PhotCalVers |
ATLASDR5 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
endDate |
PhotCalVers |
ATLASv20131127 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
endDate |
PhotCalVers |
ATLASv20160425 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
endDate |
PhotCalVers |
ATLASv20180209 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
endDate |
PhotCalVers |
VPHASDR3 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
endDate |
PhotCalVers |
VPHASv20160112 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
endDate |
PhotCalVers |
VPHASv20170222 |
Date time of end time for this version of the calibration (MM-DD-YYYY) |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
EP_1_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 1 flux |
real |
4 |
erg/cm**2/s |
|
|
EP_1_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 1 flux error EP_1_FLUX_ERR = SQRT ( 1.0 / SUM ( 1 / ca_1_FLUX_ERR2 )), where ca = PN, M1, M2 |
real |
4 |
erg/cm**2/s |
|
|
EP_2_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 2 flux |
real |
4 |
erg/cm**2/s |
|
|
EP_2_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 2 flux error EP_2_FLUX_ERR = SQRT ( 1.0 / SUM ( 1 / ca_2_FLUX_ERR2 )), where ca = PN, M1, M2 |
real |
4 |
erg/cm**2/s |
|
|
EP_3_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 3 flux |
real |
4 |
erg/cm**2/s |
|
|
EP_3_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 3 flux error EP_3_FLUX_ERR = SQRT ( 1.0 / SUM ( 1 / ca_3_FLUX_ERR2 )), where ca = PN, M1, M2 |
real |
4 |
erg/cm**2/s |
|
|
EP_4_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 4 flux |
real |
4 |
erg/cm**2/s |
|
|
EP_4_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 4 flux error EP_4_FLUX_ERR = SQRT ( 1.0 / SUM ( 1 / ca_4_FLUX_ERR2 )), where ca = PN, M1, M2 |
real |
4 |
erg/cm**2/s |
|
|
EP_5_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 5 flux |
real |
4 |
erg/cm**2/s |
|
|
EP_5_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 5 flux error EP_5_FLUX_ERR = SQRT ( 1.0 / SUM ( 1 / ca_5_FLUX_ERR2 )), where ca = PN, M1, M2 |
real |
4 |
erg/cm**2/s |
|
|
EP_8_CTS |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Combined band source counts |
real |
4 |
counts |
|
|
EP_8_CTS_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Combined band source counts 1 σ error |
real |
4 |
counts |
|
|
EP_8_DET_ML |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 8 Maximum likelihood |
real |
4 |
|
|
|
EP_8_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 8 flux |
real |
4 |
erg/cm**2/s |
|
|
EP_8_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 8 flux error EP_8_FLUX_ERR = SQRT ( 1.0 / SUM ( 1 / ca_8_FLUX_ERR2 )), where ca = PN, M1, M2 |
real |
4 |
erg/cm**2/s |
|
|
EP_8_RATE |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 8 Count rates |
real |
4 |
counts/s |
|
|
EP_8_RATE_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 8 Count rates error |
real |
4 |
counts/s |
|
|
EP_9_DET_ML |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 9 Maximum likelihood |
real |
4 |
|
|
|
EP_9_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 9 flux |
real |
4 |
erg/cm**2/s |
|
|
EP_9_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 9 flux error EP_9_FLUX_ERR = SQRT ( 1.0 / SUM ( 1 / ca_9_FLUX_ERR2 )), where ca = PN, M1, M2 |
real |
4 |
erg/cm**2/s |
|
|
EP_9_RATE |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 9 Count rates |
real |
4 |
counts/s |
|
|
EP_9_RATE_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
EP band 9 Count rates error |
real |
4 |
counts/s |
|
|
EP_CHI2PROB |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
XMM |
The Chi² probability (based on the null hypothesis) that the source as detected by any of the cameras, is constant. The minimum value of the available camera probabilities (PN_CHI2PROB, M1_CHI2PROB, M2_CHI2PROB) is given. |
real |
4 |
|
|
|
EP_CHI2PROB |
xmm3dr4 |
XMM |
The Chi² probability (based on the null hypothesis) that the source as detected by any of the cameras, is constant. The minimum value of the available camera probabilities (PN_CHI2PROB, M1_CHI2PROB, M2_CHI2PROB) is given. |
float |
8 |
|
|
|
ep_de1990 |
tycho2 |
GAIADR1 |
Epoch - 1990 of de_deg |
real |
4 |
years |
|
time.epoch |
ep_de_m |
tycho2 |
GAIADR1 |
Mean epoch of dec (Julian years) |
real |
4 |
years |
|
time.epoch |
EP_DIST_NN |
twoxmmi_dr3_v1_0 |
XMM |
The distance to the nearest neighbouring detection. An internal threshold of 6 arseconds (before positional fitting) is used for splitting a source into two. |
real |
4 |
arcsec |
|
|
EP_EXTENT |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The Extent radius of a source detected as extended. |
real |
4 |
arcsec |
|
|
EP_EXTENT_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The Extent error of a source detected as extended. |
real |
4 |
arcsec |
|
|
EP_EXTENT_ML |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The extent likelihood is the likelihood of the detection being extended as given by P = - ln (EXTENT_ML) , where P is the probability the extent occurring by chance. |
real |
4 |
|
|
|
EP_FLAG |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
XMM |
EPIC flag string made of the flags 1 - 12 (counted from left to right), where flag 10 is not used: it combines the PN, M1, and M2 flags, that is, a flag is set in EP_FLAG if at least one of the camera-dependent flags is set. |
varchar |
12 |
|
|
|
EP_FLAG |
xmm3dr4 |
XMM |
EPIC flag string made of the flags 1 - 12 (counted from left to right), where flag 10 is not used: it combines the PN, M1, and M2 flags, that is, a flag is set in EP_FLAG if at least one of the camera-dependent flags is set. |
varchar |
50 |
|
|
|
EP_HR1 |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The EP hardness ratio between the bands 1 & 2 In the case where the rate in one band is 0.0 (i.e., too faint to be detected in this band) the hardness ratio will be -1 or +1 which is only a lower or upper limit, respectively. |
real |
4 |
|
|
|
EP_HR1_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The 1 σ error of the EP hardness ratio between the bands 1 & 2 |
real |
4 |
|
|
|
EP_HR2 |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The EP hardness ratio between the bands 2 & 3 In the case where the rate in one band is 0.0 (i.e., too faint to be detected in this band) the hardness ratio will be -1 or +1 which is only a lower or upper limit, respectively. |
real |
4 |
|
|
|
EP_HR2_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The 1 σ error of the EP hardness ratio between the bands 2 & 3 |
real |
4 |
|
|
|
EP_HR3 |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The EP hardness ratio between the bands 3 & 4 In the case where the rate in one band is 0.0 (i.e., too faint to be detected in this band) the hardness ratio will be -1 or +1 which is only a lower or upper limit, respectively. |
real |
4 |
|
|
|
EP_HR3_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The 1 σ error of the EP hardness ratio between the bands 3 & 4 |
real |
4 |
|
|
|
EP_HR4 |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The EP hardness ratio between the bands 4 & 5 In the case where the rate in one band is 0.0 (i.e., too faint to be detected in this band) the hardness ratio will be -1 or +1 which is only a lower or upper limit, respectively. |
real |
4 |
|
|
|
EP_HR4_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The 1 σ error of the EP hardness ratio between the bands 4 & 5 |
real |
4 |
|
|
|
EP_OFFAX |
twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The EP offaxis angle (the distance between the detection position and the onaxis position on the respective detector). The offaxis angle for a camera can be larger than 15 arcminutes when the detection is located outside the FOV of that camera. |
real |
4 |
arcmin |
|
|
EP_ONTIME |
twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The EP ontime value (the total good exposure time (after GTI filtering) of the CCD where the detection is positioned). If a source position falls into CCD gaps or outside of the detector it will have a NULL given. |
real |
4 |
s |
|
|
ep_ra1990 |
tycho2 |
GAIADR1 |
Epoch - 1990 of ra_deg |
real |
4 |
years |
|
time.epoch |
ep_ra_m |
tycho2 |
GAIADR1 |
Mean epoch of ra (Julian years) |
real |
4 |
years |
|
time.epoch |
eparallax |
ravedr5Source |
RAVE |
Error of spectrophotometric Parallax (Binney et al. 2014) |
real |
4 |
mas |
|
stat.error;pos.parallax |
epmDE_PPMXL |
ravedr5Source |
RAVE |
Proper Motion error (Declination) |
real |
4 |
mas/yr |
|
stat.error;pos.pm;pos.eq.dec |
epmDE_TYCHO2 |
ravedr5Source |
RAVE |
Proper Motion error (Declination) |
real |
4 |
mas/yr |
|
stat.error;pos.pm;pos.eq.dec |
epmDE_UCAC4 |
ravedr5Source |
RAVE |
Proper Motion error (Declination) |
real |
4 |
mas/yr |
|
stat.error;pos.pm;pos.eq.dec |
epmDE_USNOB1 |
ravedr5Source |
RAVE |
Proper Motion error (Declination) |
real |
4 |
mas/yr |
|
stat.error;pos.pm;pos.eq.dec |
epmRA_PPMXL |
ravedr5Source |
RAVE |
Proper Motion error (Right Ascension) |
real |
4 |
mas/yr |
|
stat.error;pos.pm;pos.eq.ra |
epmRA_TYCHO2 |
ravedr5Source |
RAVE |
Proper Motion error (Right Ascension) |
real |
4 |
mas/yr |
|
stat.error;pos.pm;pos.eq.ra |
epmRA_UCAC4 |
ravedr5Source |
RAVE |
Proper Motion error (Right Ascension) |
real |
4 |
mas/yr |
|
stat.error;pos.pm.pos.eq.ra |
epmRA_USNOB1 |
ravedr5Source |
RAVE |
Proper Motion error (Right Ascension) |
real |
4 |
mas/yr |
|
stat.error;pos.pm;pos.eq.ra |
Epoch |
denisDR3Source |
DENIS |
Epoch of USNOA2.0 nearest match |
float |
8 |
yr |
|
|
epoch |
RequiredMergeLogMultiEpoch |
ATLASDR3 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
ATLASDR4 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
ATLASDR5 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
ATLASv20160425 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
ATLASv20180209 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VPHASDR3 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VPHASv20160112 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VPHASv20170222 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
ukirtFSstars |
ATLASDR1 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
ATLASDR2 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
ATLASDR3 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
ATLASDR4 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
ATLASDR5 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
ATLASv20131127 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
ATLASv20160425 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
ATLASv20180209 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
VPHASDR3 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
VPHASv20160112 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
VPHASv20170222 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
vphasSource |
VPHASDR3 |
Epoch of position measurement |
float |
8 |
Years |
|
time.epoch |
epoch |
vphasSource |
VPHASv20160112 |
Epoch of position measurement |
float |
8 |
Years |
|
time.epoch |
epoch |
vphasSource |
VPHASv20170222 |
Epoch of position measurement |
float |
8 |
Years |
|
time.epoch |
epoch_g |
cepheid, rrlyrae |
GAIADR1 |
Epoch of the maximum of the light curve in the G band |
float |
8 |
Barycentric JD in TCB - 2455197.5 days |
|
time.epoch;stat.max |
epoch_g_error |
cepheid, rrlyrae |
GAIADR1 |
Uncertainty on epoch of the maximum of the light curve in the G band |
float |
8 |
days |
|
stat.error;time.epoch |
epochFrameType |
Programme |
ATLASDR1 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
ATLASDR2 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
ATLASDR3 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
ATLASDR4 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
ATLASDR5 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
ATLASv20131127 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
ATLASv20160425 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
ATLASv20180209 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VPHASDR3 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VPHASv20160112 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VPHASv20170222 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochTolerance |
Programme |
ATLASDR3 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
ATLASDR4 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
ATLASDR5 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
ATLASv20160425 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
ATLASv20180209 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VPHASDR3 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VPHASv20160112 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VPHASv20170222 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
equinox |
Multiframe |
ATLASDR1 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
equinox |
Multiframe |
ATLASDR2 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
equinox |
Multiframe |
ATLASDR3 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
equinox |
Multiframe |
ATLASDR4 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
equinox |
Multiframe |
ATLASDR5 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
equinox |
Multiframe |
ATLASv20131127 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
equinox |
Multiframe |
ATLASv20160425 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
equinox |
Multiframe |
ATLASv20180209 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
equinox |
Multiframe |
VPHASDR3 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
equinox |
Multiframe |
VPHASv20160112 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
equinox |
Multiframe |
VPHASv20170222 |
Standard FK5 {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-9.999995e+08 |
|
erpmag_APASSDR9 |
ravedr5Source |
RAVE |
r' magnitude from APASSDR9 |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt |
err_ang |
twomass_psc |
TWOMASS |
Position angle on the sky of the semi-major axis of the position uncertainty ellipse (East of North) |
smallint |
2 |
degrees |
|
pos.posAng |
err_ang |
twomass_sixx2_psc |
TWOMASS |
angle of error ellipse major axis (E of N) |
smallint |
2 |
deg |
|
|
err_maj |
twomass_psc |
TWOMASS |
Semi-major axis length of the one sigma position uncertainty ellipse |
real |
4 |
arcsec |
|
phys.angSize;src |
err_maj |
twomass_sixx2_psc |
TWOMASS |
major axis of 1-sigma error ellipse |
real |
4 |
arcsec |
|
|
err_min |
twomass_psc |
TWOMASS |
Semi-minor axis length of the one sigma position uncertainty ellipse |
real |
4 |
arcsec |
|
phys.angSize;src |
err_min |
twomass_sixx2_psc |
TWOMASS |
minor axis of 1-sigma error ellipse |
real |
4 |
arcsec |
|
|
ERRA_IMAGE |
mgcDetection |
MGC |
Position error along major axis |
real |
4 |
pixel |
|
|
ERRB_IMAGE |
mgcDetection |
MGC |
Position error along minor axis |
real |
4 |
pixel |
|
|
errBits |
atlasDetection |
ATLASDR1 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errBits |
atlasDetection |
ATLASDR3 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errBits |
atlasDetection |
ATLASDR4 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errBits |
atlasDetection |
ATLASDR5 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errBits |
atlasDetection |
ATLASv20131127 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errBits |
atlasDetection |
ATLASv20160425 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errBits |
atlasDetection |
ATLASv20180209 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errBits |
atlasDetection, atlasDetectionUncorr |
ATLASDR2 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errBits |
vphasDetection |
VPHASv20160112 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errBits |
vphasDetection |
VPHASv20170222 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errBits |
vphasDetection, vphasDetectionUncorr |
VPHASDR3 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
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. |
errHr1 |
rosat_bsc, rosat_fsc |
ROSAT |
error of hardness ratio 1 |
float |
8 |
|
|
stat.error |
errHr2 |
rosat_bsc, rosat_fsc |
ROSAT |
error of hardness ratio 2 |
float |
8 |
|
|
stat.error |
errP |
rosat_bsc |
ROSAT |
total positional error (1-sigma-radius; including 6" systematic error) |
tinyint |
1 |
arcsec |
|
stat.error |
errP |
rosat_fsc |
ROSAT |
total positional error (1-sigma-radius; including 6" systematic error) |
smallint |
2 |
arcsec |
|
stat.error |
errSrcCps |
rosat_bsc, rosat_fsc |
ROSAT |
error of source countrate, vignetting corrected |
real |
4 |
counts/s |
|
stat.error |
esoDecMoon |
Multiframe |
ATLASDR1 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoDecMoon |
Multiframe |
ATLASDR2 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoDecMoon |
Multiframe |
ATLASDR3 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoDecMoon |
Multiframe |
ATLASDR4 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoDecMoon |
Multiframe |
ATLASDR5 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoDecMoon |
Multiframe |
ATLASv20131127 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoDecMoon |
Multiframe |
ATLASv20160425 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoDecMoon |
Multiframe |
ATLASv20180209 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoDecMoon |
Multiframe |
VPHASDR3 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoDecMoon |
Multiframe |
VPHASv20160112 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoDecMoon |
Multiframe |
VPHASv20170222 |
Declination of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON DEC} |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoGrade |
Multiframe |
ATLASDR1 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
ATLASDR2 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
ATLASDR3 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
ATLASDR4 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
ATLASDR5 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
ATLASv20131127 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
ATLASv20160425 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
ATLASv20180209 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VPHASDR3 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VPHASv20160112 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VPHASv20170222 |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoRaMoon |
Multiframe |
ATLASDR1 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
esoRaMoon |
Multiframe |
ATLASDR2 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
esoRaMoon |
Multiframe |
ATLASDR3 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
esoRaMoon |
Multiframe |
ATLASDR4 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
esoRaMoon |
Multiframe |
ATLASDR5 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
esoRaMoon |
Multiframe |
ATLASv20131127 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
esoRaMoon |
Multiframe |
ATLASv20160425 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
esoRaMoon |
Multiframe |
ATLASv20180209 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
esoRaMoon |
Multiframe |
VPHASDR3 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
esoRaMoon |
Multiframe |
VPHASv20160112 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
esoRaMoon |
Multiframe |
VPHASv20170222 |
Right ascension of the Moon (J2000) (deg) {image primary HDU keyword: HIERARCH ESO TEL MOON RA} |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
eta |
CurrentAstrometry |
ATLASDR1 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
ATLASDR2 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
ATLASDR3 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
ATLASDR4 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
ATLASDR5 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
ATLASv20131127 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
ATLASv20160425 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
ATLASv20180209 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VPHASDR3 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VPHASv20160112 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VPHASv20170222 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
atlasDetection |
ATLASDR3 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
atlasDetection |
ATLASDR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
atlasDetection |
ATLASDR5 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
atlasDetection |
ATLASv20131127 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
atlasDetection |
ATLASv20160425 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
atlasDetection |
ATLASv20180209 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
atlasDetection, atlasDetectionUncorr |
ATLASDR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
atlasDetection, atlasSource |
ATLASDR1 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vphasDetection |
VPHASv20160112 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vphasDetection |
VPHASv20170222 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vphasDetection, vphasDetectionUncorr, vphasSource |
VPHASDR3 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
ETA_TYPE |
mgcGalaxyStruct |
MGC |
2dFGRS Eta type |
real |
4 |
|
-99.9 |
|
eTeff_IR |
ravedr5Source |
RAVE |
Error of effective temperature from infrared flux method |
real |
4 |
K |
|
stat.error;phys.temperature.effective |
eTeff_K |
ravedr5Source |
RAVE |
Effective Temperature error |
float |
8 |
K |
|
stat.error;phys.temperature.effective |
eVmag_APASSDR9 |
ravedr5Source |
RAVE |
error V magnitude from APASSDR9 |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt.V |
eVTmag_TYCHO2 |
ravedr5Source |
RAVE |
Error of VT magnitude from TYCHO2 |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt.V |
eW1mag_ALLWISE |
ravedr5Source |
RAVE |
Error W1 magnitude from ALLWISE |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt |
eW2mag_ALLWISE |
ravedr5Source |
RAVE |
Error W2 magnitude from ALLWISE |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt |
eW3mag_ALLWISE |
ravedr5Source |
RAVE |
Error W3 magnitude from ALLWISE |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt |
eW4mag_ALLWISE |
ravedr5Source |
RAVE |
Error W4 magnitude from ALLWISE |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt |
expTime |
Multiframe |
ATLASDR1 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
Multiframe |
ATLASDR2 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
Multiframe |
ATLASDR3 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
Multiframe |
ATLASDR4 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
Multiframe |
ATLASDR5 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
Multiframe |
ATLASv20131127 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
Multiframe |
ATLASv20160425 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
Multiframe |
ATLASv20180209 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
Multiframe |
VPHASDR3 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
Multiframe |
VPHASv20160112 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
Multiframe |
VPHASv20170222 |
Total integration time {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-9.999995e+08 |
|
expTime |
rosat_bsc |
ROSAT |
exposure time |
smallint |
2 |
sec |
|
time.duration;obs.exposure |
expTime |
rosat_fsc |
ROSAT |
exposure time |
int |
4 |
sec |
|
time.duration;obs.exposure |
ext |
rosat_bsc, rosat_fsc |
ROSAT |
source extent |
smallint |
2 |
arcsec |
|
phys.angSize |
ext_cat_solution_type |
gaia_hip_tycho2_match |
GAIADR1 |
Type of solution in the Hipparcos/Tycho2 catalogue |
varchar |
1 |
|
|
meta.code |
ext_flg |
allwise_sc |
WISE |
Extended source flag. This is an integer flag, the value of which indicates whether or not the morphology of a source is consistent with the WISE point spread function in any band, or whether the source is associated with or superimposed on a previously known extended object from the 2MASS Extended Source Catalog (XSC). CAUTION: WISE profile-fit (w?mpro) and standard aperture (w?mag) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has ext_flg>0, you may wish to examine the large aperture photometry, or the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies. |
int |
4 |
|
|
|
The values of the ext_flg indicate the following conditions: - 0 - The source shape is consistent with a point-source and the source is not associated with or superimposed on a 2MASS XSC source
- 1 - The profile-fit photometry goodness-of-fit, w?rchi2, is >3.0 in one or more bands.
- 2 - The source falls within the extrapolated isophotal footprint of a 2MASS XSC source.
- 3 - The profile-fit photometry goodness-of-fit,w?rchi2, is >3.0 in one or more bands, and the source falls within the extrapolated isophotal footprint of a 2MASS XSC source.
- 4 - The source position falls within 5" of a 2MASS XSC source.
- 5 - The profile-fit photometry goodness-of-fit,w?rchi2, is >3.0 in one or more bands, and the source position falls within 5" of a 2MASS XSC source.
|
ext_flg |
wise_allskysc |
WISE |
Extended source flag. This flag indicates whether or not the morphology of a source is consistent with the WISE point spread function in any band or whether the source is associated with or superimposed on a previously known extended object from the 2MASS Extended Source Catalog (XSC): 0 - The source shape is consistent with a point-source; 1 - The source shape is not consistent with a point-source; 2 - The source falls within the extrapolated isophotal footprint of a 2MASS XSC source; 3 - The profile-fit photometry goodness-of-fit, w?rchi2, is >3.0 in one or more bands, and The source falls within the extrapolated isophotal footprint of a 2MASS XSC source; 4 - The source position falls within 5" of a 2MASS XSC source; 5 - The profile-fit photometry goodness-of-fit, w?rchi2, is >3.0 in one or more bands, and the source position falls within 5" of a 2MASS XSC source. CAUTION: WISE profile-fit (w?mpro) and standard aperture (w?mag) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. |
tinyint |
1 |
|
|
|
ext_flg |
wise_prelimsc |
WISE |
Extended source flag This flag indicates whether or not the morphology of a source is consistent with the WISE point spread function in any band: 0 - The source shape is consistent with a point-source; 1 - The source shape is not consistent with a point-source |
tinyint |
1 |
|
|
|
ext_flg_ALLWISE |
ravedr5Source |
RAVE |
probability source morphology is not consistent with single PSF |
int |
4 |
|
|
meta.code |
ext_key |
twomass_psc |
TWOMASS |
Unique identification number of the record in the XSC that corresponds to this point source. |
int |
4 |
|
|
meta.id |
ext_key |
twomass_xsc |
TWOMASS |
entry counter (key) number (unique within table). |
int |
4 |
|
|
meta.id |
extinctionCat |
MultiframeDetector |
ATLASDR1 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionCat |
MultiframeDetector |
ATLASDR2 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionCat |
MultiframeDetector |
ATLASDR3 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionCat |
MultiframeDetector |
ATLASDR4 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionCat |
MultiframeDetector |
ATLASDR5 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionCat |
MultiframeDetector |
ATLASv20131127 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionCat |
MultiframeDetector |
ATLASv20160425 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionCat |
MultiframeDetector |
ATLASv20180209 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionCat |
MultiframeDetector |
VPHASDR3 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionCat |
MultiframeDetector |
VPHASv20160112 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionCat |
MultiframeDetector |
VPHASv20170222 |
Extinction coefficient for the catalogue data {catalogue extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
ATLASDR1 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
ATLASDR2 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
ATLASDR3 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
ATLASDR4 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
ATLASDR5 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
ATLASv20131127 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
ATLASv20160425 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
ATLASv20180209 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
VPHASDR3 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
VPHASv20160112 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionExt |
MultiframeDetector |
VPHASv20170222 |
Extinction coefficient of the detector {image extension keyword: EXTINCT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
These are currently set to a constant clear night level, which within the current measuring error is the same for all passbands. Note that the frame-by-frame derived ZP from 2MASS automatically corrects for extinction variations, assuming they are uniform across the field of view. |
extinctionMapList |
Programme |
ATLASDR3 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
ATLASDR4 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
ATLASDR5 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
ATLASv20160425 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
ATLASv20180209 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VPHASDR3 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VPHASv20160112 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VPHASv20170222 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extl |
rosat_bsc, rosat_fsc |
ROSAT |
likelihood of source extent |
smallint |
2 |
|
|
stat.likelihood |
extMapID |
vphasSourceExtinction |
VPHASDR3 |
UID of 3D extinction map used |
tinyint |
1 |
|
0 |
|
extMapID |
vphasSourceExtinction |
VPHASv20160112 |
UID of 3D extinction map used |
tinyint |
1 |
|
0 |
|
extMapID |
vphasSourceExtinction |
VPHASv20170222 |
UID of 3D extinction map used |
tinyint |
1 |
|
0 |
|
extName |
MultiframeDetector |
ATLASDR1 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extName |
MultiframeDetector |
ATLASDR2 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extName |
MultiframeDetector |
ATLASDR3 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extName |
MultiframeDetector |
ATLASDR4 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extName |
MultiframeDetector |
ATLASDR5 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extName |
MultiframeDetector |
ATLASv20131127 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extName |
MultiframeDetector |
ATLASv20160425 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extName |
MultiframeDetector |
ATLASv20180209 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extName |
MultiframeDetector |
VPHASDR3 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extName |
MultiframeDetector |
VPHASv20160112 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extName |
MultiframeDetector |
VPHASv20170222 |
Extension name {image extension keyword: EXTNAME} |
varchar |
16 |
|
NONE |
|
extNum |
CurrentAstrometry |
ATLASDR2 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
ATLASDR3 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
ATLASDR5 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
ATLASv20131127 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
ATLASv20160425 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
ATLASv20180209 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VPHASDR3 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VPHASv20160112 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VPHASv20170222 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry, EpochFrameStatus |
ATLASDR4 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry, MultiframeDetector, MultiframeDetectorEsoKeys |
ATLASDR1 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
PreviousMFDZP |
ATLASDR3 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
ATLASDR5 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
ATLASv20131127 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
ATLASv20160425 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
ATLASv20180209 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VPHASv20160112 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VPHASv20170222 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
atlasAstrometricInfo, PreviousMFDZP |
ATLASDR4 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
atlasDetection, PreviousMFDZP |
ATLASDR1 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
atlasDetectionUncorr, PreviousMFDZP |
ATLASDR2 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, vphasAstrometricInfo, vphasDetection, vphasDetectionUncorr |
VPHASDR3 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extPixelID |
vphasSourceExtinction |
VPHASDR3 |
Pixel ID from 3D extinction map that matches source position |
int |
4 |
|
-99999999 |
|
extPixelID |
vphasSourceExtinction |
VPHASv20160112 |
Pixel ID from 3D extinction map that matches source position |
int |
4 |
|
-99999999 |
|
extPixelID |
vphasSourceExtinction |
VPHASv20170222 |
Pixel ID from 3D extinction map that matches source position |
int |
4 |
|
-99999999 |
|
extProgID |
RequiredNeighbours |
ATLASDR1 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
ATLASDR2 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
ATLASDR3 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
ATLASDR4 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
ATLASDR5 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
ATLASv20131127 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
ATLASv20160425 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
ATLASv20180209 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VPHASDR3 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VPHASv20160112 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VPHASv20170222 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extr |
rosat_bsc, rosat_fsc |
ROSAT |
extraction radius |
smallint |
2 |
arcsec |
|
stat.fit.param |
extractTool |
Programme |
ATLASDR1 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
ATLASDR2 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
ATLASDR3 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
ATLASDR4 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
ATLASDR5 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
ATLASv20131127 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
ATLASv20160425 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
ATLASv20180209 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VPHASDR3 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VPHASv20160112 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VPHASv20170222 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extTableID |
ExternalSurveyTable |
ATLASDR2 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
ATLASDR3 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
ATLASDR4 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
ATLASDR5 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
ATLASv20131127 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
ATLASv20160425 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
ATLASv20180209 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VPHASDR3 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VPHASv20160112 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VPHASv20170222 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable, RequiredNeighbours |
ATLASDR1 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableName |
ExternalSurveyTable |
ATLASDR1 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
ATLASDR2 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
ATLASDR3 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
ATLASDR4 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
ATLASDR5 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
ATLASv20131127 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
ATLASv20160425 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
ATLASv20180209 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VPHASDR3 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VPHASv20160112 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VPHASv20170222 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |