E |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
E24umMag |
spitzer_smcSource |
SPITZER |
The SPITZER E24μm band magnitude. |
real |
4 |
mag |
|
|
E3_6umMag |
spitzer_smcSource |
SPITZER |
The SPITZER E3.6μm band magnitude. |
real |
4 |
mag |
|
|
E4_5umMag |
spitzer_smcSource |
SPITZER |
The SPITZER E4.5μm band magnitude. |
real |
4 |
mag |
|
|
E5_8umMag |
spitzer_smcSource |
SPITZER |
The SPITZER E5.8μm band magnitude. |
real |
4 |
mag |
|
|
E70umMag |
spitzer_smcSource |
SPITZER |
The SPITZER E70μm band magnitude. |
real |
4 |
mag |
|
|
E8_0umMag |
spitzer_smcSource |
SPITZER |
The SPITZER E8.0μm band magnitude. |
real |
4 |
mag |
|
|
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_BbMag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of BbMag |
real |
4 |
mag |
|
|
e_BF_D |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of BF_D |
float |
8 |
|
|
|
e_BF_F |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of BF_F |
float |
8 |
|
|
|
e_BF_S |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of BF_S |
float |
8 |
|
|
|
e_BjMag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of BjMag |
real |
4 |
mag |
|
|
e_Bmag |
mcps_lmcSource, mcps_smcSource |
MCPS |
The 1σ error in Bmag |
real |
4 |
|
|
|
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_dej2000 |
masterDR2 |
SKYMAPPER |
RMS variation around the mean Declination, in milliarcseconds |
int |
4 |
mas |
|
stat.stdev;pos.eq.dec |
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_g_petro |
masterDR2 |
SKYMAPPER |
Error in g-band Petrosian magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
e_g_psf |
masterDR2 |
SKYMAPPER |
Error in g-band PSF magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
e_gsMag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of gsMag |
real |
4 |
mag |
|
|
e_Hmag |
mcps_lmcSource, mcps_smcSource |
MCPS |
The 1σ error in Hmag |
real |
4 |
|
|
|
e_hp_mag |
hipparcos_new_reduction |
GAIADR1 |
Error on mean Hipparcos magnitude |
float |
8 |
mag |
|
em.opt.V;phot.mag;stat.error |
e_i_petro |
masterDR2 |
SKYMAPPER |
Error in i-band Petrosian magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
e_i_psf |
masterDR2 |
SKYMAPPER |
Error in i-band PSF magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
e_IF_D |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of IF_D |
float |
8 |
|
|
|
e_Imag |
mcps_lmcSource, mcps_smcSource |
MCPS |
The 1σ error in Imag magnitude |
real |
4 |
|
|
|
e_Jmag |
mcps_lmcSource, mcps_smcSource |
MCPS |
The 1σ error in Jmag |
real |
4 |
|
|
|
e_Kmag |
mcps_lmcSource, mcps_smcSource |
MCPS |
The 1σ error in Kmag |
real |
4 |
|
|
|
e_majAxis |
nvssSource |
NVSS |
Mean error on majAxis |
real |
4 |
arcsec |
|
stat.error |
e_MC_z |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of MC_z |
real |
4 |
|
|
|
e_MC_z2 |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of MC_z2 |
real |
4 |
|
|
|
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_r_petro |
masterDR2 |
SKYMAPPER |
Error in r-band Petrosian magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
e_r_psf |
masterDR2 |
SKYMAPPER |
Error in r-band PSF magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
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_raj2000 |
masterDR2 |
SKYMAPPER |
RMS variation around the mean Right Ascension, in milliarcseconds |
int |
4 |
mas |
|
stat.stdev;pos.eq.ra |
e_RAs |
nvssSource |
NVSS |
Mean error on RA |
real |
4 |
s |
|
stat.error |
e_RF_D |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of RF_D |
float |
8 |
|
|
|
e_RF_E |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of RF_E |
float |
8 |
|
|
|
e_RF_F |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of RF_F |
float |
8 |
|
|
|
e_RF_G |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of RF_G |
float |
8 |
|
|
|
e_RF_S |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of RF_S |
float |
8 |
|
|
|
e_Rmag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of Rmag |
real |
4 |
mag |
|
|
e_rsMag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of rsMag |
real |
4 |
mag |
|
|
e_S14 |
nvssSource |
NVSS |
Mean error on S14 |
real |
4 |
mJy |
|
stat.error |
e_S145Mag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of S145Mag |
real |
4 |
mag |
|
|
e_S280Mag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of S280Mag |
real |
4 |
mag |
|
|
e_score |
twomass_xsc |
TWOMASS |
extended score: 1(extended) < e_score < 2(point-like). |
real |
4 |
|
|
meta.code |
e_u_petro |
masterDR2 |
SKYMAPPER |
Error in u-band Petrosian magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
e_u_psf |
masterDR2 |
SKYMAPPER |
Error in u-band PSF magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
e_UbMag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of UbMag |
real |
4 |
mag |
|
|
e_UF_F |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of UF_F |
float |
8 |
|
|
|
e_UF_G |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of UF_G |
float |
8 |
|
|
|
e_UF_S |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of UF_S |
float |
8 |
|
|
|
e_UjMag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of UjMag |
real |
4 |
mag |
|
|
e_Umag |
mcps_lmcSource, mcps_smcSource |
MCPS |
The 1σ error in Umag |
real |
4 |
|
|
|
e_usMag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of usMag |
real |
4 |
mag |
|
|
e_v_petro |
masterDR2 |
SKYMAPPER |
Error in v-band Petrosian magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
e_v_psf |
masterDR2 |
SKYMAPPER |
Error in v-band PSF magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
e_VbMag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of VbMag |
real |
4 |
mag |
|
|
e_VF_D |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of VF_D |
float |
8 |
|
|
|
e_VjMag |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of VjMag |
real |
4 |
mag |
|
|
e_Vmag |
mcps_lmcSource, mcps_smcSource |
MCPS |
The 1σ error in Vmag |
real |
4 |
|
|
|
e_vt_mag |
tycho2 |
GAIADR1 |
Standard error on VT |
real |
4 |
mag |
|
stat.error |
e_W420F_E |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W420F_E |
float |
8 |
|
|
|
e_W462F_E |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W462F_E |
float |
8 |
|
|
|
e_W485F_D |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W485F_D |
float |
8 |
|
|
|
e_W518F_E |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W518F_E |
float |
8 |
|
|
|
e_W571F_D |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W571F_D |
float |
8 |
|
|
|
e_W571F_E |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W571F_E |
float |
8 |
|
|
|
e_W571F_S |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W571F_S |
float |
8 |
|
|
|
e_W604F_E |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W604F_E |
float |
8 |
|
|
|
e_W646F_D |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W646F_D |
float |
8 |
|
|
|
e_W696F_E |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W696F_E |
float |
8 |
|
|
|
e_W753F_E |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W753F_E |
float |
8 |
|
|
|
e_W815F_E |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W815F_E |
float |
8 |
|
|
|
e_W815F_G |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W815F_G |
float |
8 |
|
|
|
e_W815F_S |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W815F_S |
float |
8 |
|
|
|
e_W856F_D |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W856F_D |
float |
8 |
|
|
|
e_W914F_D |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W914F_D |
float |
8 |
|
|
|
e_W914F_E |
combo17CDFSSource |
COMBO17 |
mean error (1-sigma) of W914F_E |
float |
8 |
|
|
|
e_z_petro |
masterDR2 |
SKYMAPPER |
Error in z-band Petrosian magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
e_z_psf |
masterDR2 |
SKYMAPPER |
Error in z-band PSF magnitude |
real |
4 |
mag |
|
stat.error;phot.mag |
eBmag_APASSDR9 |
ravedr5Source |
RAVE |
error B magnitude from APASSDR9 |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt.B |
ebmv_sfd |
masterDR2 |
SKYMAPPER |
E(B-V) from Schlegel+1998 extinction maps at the ICRS coordinates |
real |
4 |
mag |
|
phot.color.excess;phys.absorption |
ebmvMed |
MultiframeDetector |
SHARKSv20210222 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
SHARKSv20210421 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
ULTRAVISTADR4 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSDR1 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSDR2 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSDR3 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSDR4 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSDR5 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSDR6 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20120926 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20130417 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20140409 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20150108 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20160114 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20160507 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20170630 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20180419 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20201209 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20231101 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VHSv20240731 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIDEODR2 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIDEODR3 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIDEODR4 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIDEODR5 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIDEOv20111208 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGDR2 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGDR3 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGDR4 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGv20110714 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGv20111019 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGv20130417 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGv20140402 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGv20150421 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGv20151230 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGv20160406 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGv20161202 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VIKINGv20170715 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCDEEPv20230713 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCDEEPv20240506 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCDR1 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCDR2 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCDR3 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCDR4 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCDR5 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20110816 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20110909 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20120126 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20121128 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20130304 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20130805 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20140428 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20140903 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20150309 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20151218 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20160311 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20160822 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20170109 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20170411 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20171101 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20180702 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20181120 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20191212 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20210708 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20230816 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VMCv20240226 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VVVDR1 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VVVDR2 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VVVDR5 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VVVXDR1 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
MultiframeDetector |
VVVv20110718 |
Median modified E(B-V) {catalogue extension keyword: EBMVMED} |
real |
4 |
|
-0.9999995e9 |
|
ebmvMed |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Median modified E(B-V) |
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 |
sharksSource |
SHARKSv20210222 |
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 |
sharksSource |
SHARKSv20210421 |
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 |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
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 |
vhsSource |
VHSDR1 |
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 |
vhsSource |
VHSDR2 |
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 |
vhsSource |
VHSDR3 |
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 |
vhsSource |
VHSDR4 |
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 |
vhsSource |
VHSDR5 |
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 |
vhsSource |
VHSDR6 |
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 |
vhsSource |
VHSv20120926 |
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 |
vhsSource |
VHSv20130417 |
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 |
vhsSource |
VHSv20140409 |
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 |
vhsSource |
VHSv20150108 |
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 |
vhsSource |
VHSv20160114 |
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 |
vhsSource |
VHSv20160507 |
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 |
vhsSource |
VHSv20170630 |
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 |
vhsSource |
VHSv20180419 |
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 |
vhsSource |
VHSv20201209 |
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 |
vhsSource |
VHSv20231101 |
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 |
vhsSource |
VHSv20240731 |
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 |
videoSource |
VIDEODR2 |
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 |
videoSource |
VIDEODR3 |
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 |
videoSource |
VIDEODR4 |
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 |
videoSource |
VIDEODR5 |
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 |
videoSource |
VIDEOv20100513 |
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 |
videoSource |
VIDEOv20111208 |
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 |
vikingSource |
VIKINGDR2 |
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 |
vikingSource |
VIKINGDR3 |
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 |
vikingSource |
VIKINGDR4 |
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 |
vikingSource |
VIKINGv20110714 |
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 |
vikingSource |
VIKINGv20111019 |
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 |
vikingSource |
VIKINGv20130417 |
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 |
vikingSource |
VIKINGv20140402 |
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 |
vikingSource |
VIKINGv20150421 |
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 |
vikingSource |
VIKINGv20151230 |
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 |
vikingSource |
VIKINGv20160406 |
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 |
vikingSource |
VIKINGv20161202 |
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 |
vikingSource |
VIKINGv20170715 |
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 |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
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 |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
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 |
smashdr2_deep, smashdr2_object |
SMASH |
Median SFD E(B-V) across frame |
real |
4 |
|
|
|
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 |
ebv |
wiseScosPhotoz, wiseScosPhotozRejects, wiseScosSvm |
WISExSCOSPZ |
The Galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. {image primary HDU keyword: Ebmv} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
ECCENT |
grs_ngpSource, grs_ranSource, grs_sgpSource |
TWODFGRS |
Eccentricity (e) e*200 = 200*(((sxx-syy)**2 + 4sxy**2)**0.5)/(sxx + syy) |
real |
4 |
|
|
|
ecl_lat |
gaia_source |
GAIADR2 |
Ecliptic latitude |
float |
8 |
degrees |
|
pos.ecliptic.lat |
ecl_lat |
gaia_source |
GAIAEDR3 |
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 |
GAIAEDR3 |
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 |
eD |
vvvVivaCatalogue |
VVVDR5 |
Even dispersion parameter of Ks pawprint data {catalogue TType keyword: ED} |
float |
8 |
mag |
-9.999995e8 |
|
edepm |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Error on Dec component of proper motion {catalogue TType keyword: edepm} |
float |
8 |
mas/yr |
-999999500.0 |
|
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 |
eHKs |
vvvBulge3DExtinctVals |
EXTINCT |
E(H-Ks) calculated from the stellar population model at distance r |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
eHKsErr |
vvvBulge3DExtinctVals |
EXTINCT |
Error on E(H-Ks) calculated from the stellar population model at distance r |
real |
4 |
mag |
-0.9999995e9 |
star.error |
eHmag |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Error on VVV DR4 H photometry. {catalogue TType keyword: eHmag} |
real |
4 |
mag |
-999999500.0 |
|
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 |
eJ |
vvvPsfDaophotJKsSource |
VVVDR5 |
The fitted (4th-degree polynomial) adjusted Median Absolute Deviation (MAD; so that 1-MAD = 1-sigma in the traditional sense) per J bin of the simulations, of the Jin-Jout (Kin - Kout) difference {catalogue TType keyword: ej} |
real |
4 |
|
-0.9999995e9 |
|
eJKs |
vvvBulge3DExtinctVals |
EXTINCT |
E(J-Ks) calculated from the stellar population model at distance r |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
eJKs |
vvvPsfDaophotJKsSource |
VVVDR5 |
The galactic dust extinction value measured from Gonzalez et al. (201?) to the. {catalogue TType keyword: ejk} |
real |
4 |
|
-0.9999995e9 |
phys.absorption.gal |
eJKs |
vvvVivaCatalogue |
VVVDR5 |
Extinction computed from Gonzalez et al. 2012 (Galactic bulge) and Minniti-2018 (Galactic disk) {catalogue TType keyword: EJKs} |
real |
4 |
|
-9.999995e8 |
|
eJKsErr |
vvvBulge3DExtinctVals |
EXTINCT |
Error on E(J-Ks) calculated from the stellar population model at distance r |
real |
4 |
mag |
-0.9999995e9 |
star.error |
eJKsErr |
vvvPsfDaophotJKsSource |
VVVDR5 |
The error on the galactic dust extinction value measured from Gonzalez et al. (201?). {catalogue TType keyword: ejk_err} |
real |
4 |
|
-0.9999995e9 |
stat.error;phys.absorption.gal |
eJKsErr |
vvvVivaCatalogue |
VVVDR5 |
Rms related with the three nearest EJKs estimations (Galactic disk) {catalogue TType keyword: EJKsErr} |
real |
4 |
|
-9.999995e8 |
|
eJmag |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Error on VVV DR4 J photometry. {catalogue TType keyword: eJmag} |
real |
4 |
mag |
-999999500.0 |
|
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 |
eKs |
vvvPsfDaophotJKsSource |
VVVDR5 |
The fitted (4th-degree polynomial) adjusted Median Absolute Deviation (MAD; so that 1-MAD = 1-sigma in the traditional sense) per Ks bin of the simulations, of the Jin-Jout (Kin - Kout) difference {catalogue TType keyword: ek} |
real |
4 |
|
-0.9999995e9 |
|
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 |
smashdr2_deep, smashdr2_object |
SMASH |
Ecliptic latitude |
float |
8 |
|
|
|
elat |
smashdr2_source |
SMASH |
Ecliptic Latitude |
float |
8 |
|
|
|
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 |
sharksDetection |
SHARKSv20210222 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
sharksDetection |
SHARKSv20210421 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged 1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSDR2 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSDR3 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSDR4 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSDR5 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSDR6 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20120926 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20130417 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20140409 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20150108 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20160114 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20160507 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20170630 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20180419 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20201209 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20231101 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection |
VHSv20240731 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
videoDetection |
VIDEODR2 |
1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
videoDetection |
VIDEODR3 |
1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
videoDetection |
VIDEODR4 |
1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
videoDetection |
VIDEODR5 |
1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
videoDetection |
VIDEOv20100513 |
1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
videoDetection |
VIDEOv20111208 |
1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
videoListRemeasurement |
VIDEOv20100513 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGDR2 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGDR3 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGDR4 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGv20111019 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGv20130417 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGv20140402 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGv20150421 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGv20151230 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGv20160406 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGv20161202 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection |
VIKINGv20170715 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged 1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) |
real |
4 |
|
|
src.ellipticity |
ell |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged 1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) |
real |
4 |
|
|
src.ellipticity |
ell |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
1-b/a, where a/b=semi-major/minor axes (SE: THETA_IMAGE) {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCDR1 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCDR2 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCDR3 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCDR4 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCDR5 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20110909 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20120126 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20121128 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20130304 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20130805 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20140428 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20140903 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20150309 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20151218 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20160311 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20160822 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20170109 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20170411 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20171101 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20180702 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20181120 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20191212 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20210708 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20230816 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection |
VMCv20240226 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcdeepDetection |
VMCDEEPv20230713 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vmcdeepDetection |
VMCDEEPv20240506 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vvvDetection |
VVVDR1 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vvvDetection |
VVVDR2 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
1-b/a, where a/b=semi-major/minor axes {catalogue TType keyword: Ellipticity} |
real |
4 |
|
|
src.ellipticity |
ell |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Mean Ks band ellipticity across all observations of this source in every pawprint set. {catalogue TType keyword: ell} |
real |
4 |
|
-999999500.0 |
|
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 |
smashdr2_deep, smashdr2_object |
SMASH |
Ecliptic longitude |
float |
8 |
|
|
|
elon |
smashdr2_source |
SMASH |
Ecliptic Longitude |
float |
8 |
|
|
|
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 |
|
|
emag |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Median absolute deviation of Ks band aperMag2 measurements from all epochs in the pawprint set {catalogue TType keyword: emag} |
real |
4 |
|
-999999500.0 |
|
eMet_K |
ravedr5Source |
RAVE |
Error of [m/H] |
float |
8 |
dex |
|
phys.abund.Z |
endDate |
AstrCalVers |
SHARKSv20210222 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
SHARKSv20210421 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
ULTRAVISTADR4 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSDR1 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSDR2 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSDR3 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSDR4 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSDR5 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSDR6 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSv20120926 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSv20130417 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSv20150108 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSv20160114 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSv20160507 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSv20170630 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSv20180419 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSv20201209 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSv20231101 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VHSv20240731 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIDEODR2 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIDEODR3 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIDEODR4 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIDEODR5 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIDEOv20100513 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIDEOv20111208 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGDR2 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGDR3 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGDR4 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGv20110714 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGv20111019 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGv20130417 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGv20150421 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGv20151230 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGv20160406 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGv20161202 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VIKINGv20170715 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCDEEPv20230713 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCDEEPv20240506 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCDR1 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCDR3 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCDR4 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCDR5 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20110816 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20110909 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20120126 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20121128 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20130304 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20130805 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20140428 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20140903 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20150309 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20151218 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20160311 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20160822 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20170109 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20170411 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20171101 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20180702 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20181120 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20191212 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20210708 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20230816 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VMCv20240226 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VVVDR1 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VVVDR2 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VVVDR5 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VVVXDR1 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VVVv20100531 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
AstrCalVers |
VVVv20110718 |
MJD of the end time for this version of the calibration |
float |
8 |
Julian days |
|
time.epoch |
endDate |
PhotCalVers |
SHARKSv20210222 |
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 |
SHARKSv20210421 |
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 |
ULTRAVISTADR4 |
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 |
VHSDR1 |
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 |
VHSDR2 |
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 |
VHSDR3 |
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 |
VHSDR4 |
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 |
VHSDR5 |
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 |
VHSDR6 |
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 |
VHSv20120926 |
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 |
VHSv20130417 |
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 |
VHSv20150108 |
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 |
VHSv20160114 |
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 |
VHSv20160507 |
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 |
VHSv20170630 |
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 |
VHSv20180419 |
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 |
VHSv20201209 |
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 |
VHSv20231101 |
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 |
VHSv20240731 |
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 |
VIDEODR2 |
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 |
VIDEODR3 |
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 |
VIDEODR4 |
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 |
VIDEODR5 |
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 |
VIDEOv20100513 |
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 |
VIDEOv20111208 |
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 |
VIKINGDR2 |
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 |
VIKINGDR3 |
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 |
VIKINGDR4 |
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 |
VIKINGv20110714 |
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 |
VIKINGv20111019 |
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 |
VIKINGv20130417 |
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 |
VIKINGv20150421 |
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 |
VIKINGv20151230 |
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 |
VIKINGv20160406 |
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 |
VIKINGv20161202 |
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 |
VIKINGv20170715 |
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 |
VMCDEEPv20230713 |
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 |
VMCDEEPv20240506 |
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 |
VMCDR1 |
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 |
VMCDR3 |
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 |
VMCDR4 |
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 |
VMCDR5 |
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 |
VMCv20110816 |
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 |
VMCv20110909 |
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 |
VMCv20120126 |
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 |
VMCv20121128 |
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 |
VMCv20130304 |
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 |
VMCv20130805 |
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 |
VMCv20140428 |
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 |
VMCv20140903 |
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 |
VMCv20150309 |
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 |
VMCv20151218 |
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 |
VMCv20160311 |
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 |
VMCv20160822 |
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 |
VMCv20170109 |
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 |
VMCv20170411 |
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 |
VMCv20171101 |
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 |
VMCv20180702 |
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 |
VMCv20181120 |
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 |
VMCv20191212 |
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 |
VMCv20210708 |
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 |
VMCv20230816 |
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 |
VMCv20240226 |
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 |
VVVDR1 |
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 |
VVVDR2 |
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 |
VVVDR5 |
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 |
VVVXDR1 |
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 |
VVVv20100531 |
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 |
VVVv20110718 |
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 |
eplx |
vvvParallaxCatalogue |
VVVDR5 |
Error on parallax. These are inverse variance weighted averages across their measured values in both equatorial tangent plane dimensions and from all pawprint sets. {catalogue TType keyword: eplx} |
float |
8 |
mas |
-999999500.0 |
|
epm |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Error on total proper motion {catalogue TType keyword: epm} |
float |
8 |
mas/yr |
-999999500.0 |
|
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 |
SHARKSv20210222 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
SHARKSv20210421 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
ULTRAVISTADR4 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VHSDR5 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VHSDR6 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VHSv20160114 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VHSv20160507 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VHSv20170630 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VHSv20180419 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VHSv20201209 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VHSv20231101 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VHSv20240731 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VIKINGv20151230 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VIKINGv20160406 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VIKINGv20161202 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VIKINGv20170715 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCDEEPv20230713 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCDEEPv20240506 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCDR4 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCDR5 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20151218 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20160311 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20160822 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20170109 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20170411 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20171101 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20180702 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20181120 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20191212 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20210708 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20230816 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VMCv20240226 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VVVDR5 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
RequiredMergeLogMultiEpoch |
VVVXDR1 |
Epoch number in MergeLog table |
tinyint |
1 |
|
|
|
epoch |
sage_lmcIracSource, sage_lmcMips160Source, sage_lmcMips24Source, sage_lmcMips70Source |
SPITZER |
Character string identifier for epoch of source |
varchar |
16 |
|
|
|
epoch |
sage_smcIRACv1_5Source |
SPITZER |
Character string identifier for the epoch of the observation of the source, i.e. "epoch 1", "epoch 2", "epoch 1+2",... |
varchar |
16 |
|
|
|
epoch |
sharksVariability |
SHARKSv20210222 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
sharksVariability |
SHARKSv20210421 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
ukirtFSstars |
VIDEOv20100513 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
VIKINGv20110714 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ukirtFSstars |
VVVv20100531 |
The epoch of columns ra and dec |
real |
4 |
years |
-0.9999995e9 |
|
epoch |
ultravistaVariability |
ULTRAVISTADR4 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vhsSourceRemeasurement |
VHSDR1 |
Epoch of position measurement |
float |
8 |
Years |
-0.9999995e9 |
time.epoch |
epoch |
videoSourceRemeasurement |
VIDEOv20100513 |
Epoch of position measurement |
float |
8 |
Years |
-0.9999995e9 |
time.epoch |
epoch |
videoVariability |
VIDEODR2 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
videoVariability |
VIDEODR3 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
videoVariability |
VIDEODR4 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
videoVariability |
VIDEODR5 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
videoVariability |
VIDEOv20100513 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
videoVariability |
VIDEOv20111208 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingSourceRemeasurement |
VIKINGv20110714 |
Epoch of position measurement |
float |
8 |
Years |
-0.9999995e9 |
time.epoch |
epoch |
vikingSourceRemeasurement |
VIKINGv20111019 |
Epoch of position measurement |
float |
8 |
Years |
-0.9999995e9 |
time.epoch |
epoch |
vikingVariability |
VIKINGDR2 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGDR3 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGDR4 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGv20110714 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGv20111019 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGv20130417 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGv20140402 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGv20150421 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGv20151230 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGv20160406 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGv20161202 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vikingVariability |
VIKINGv20170715 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcSourceRemeasurement |
VMCv20110816 |
Epoch of position measurement |
float |
8 |
Years |
-0.9999995e9 |
time.epoch |
epoch |
vmcSourceRemeasurement |
VMCv20110909 |
Epoch of position measurement |
float |
8 |
Years |
-0.9999995e9 |
time.epoch |
epoch |
vmcVariability |
VMCDR1 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCDR2 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCDR3 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCDR4 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCDR5 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20110816 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20110909 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20120126 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20121128 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20130304 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20130805 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20140428 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20140903 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20150309 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20151218 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20160311 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20160822 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20170109 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20170411 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20171101 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20180702 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20181120 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20191212 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20210708 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20230816 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcVariability |
VMCv20240226 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcdeepVariability |
VMCDEEPv20230713 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vmcdeepVariability |
VMCDEEPv20240506 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vvvSourceRemeasurement |
VVVv20100531 |
Epoch of position measurement |
float |
8 |
Years |
-0.9999995e9 |
time.epoch |
epoch |
vvvSourceRemeasurement |
VVVv20110718 |
Epoch of position measurement |
float |
8 |
Years |
-0.9999995e9 |
time.epoch |
epoch |
vvvVariability |
VVVDR1 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vvvVariability |
VVVDR2 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vvvVariability |
VVVDR5 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vvvVariability |
VVVv20100531 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vvvVariability |
VVVv20110718 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
epoch |
vvvxVariability |
VVVXDR1 |
Epoch of measurement |
float |
8 |
Years |
|
time.epoch |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
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 |
SHARKSv20210222 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
SHARKSv20210421 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
ULTRAVISTADR4 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSDR1 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSDR2 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSDR3 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSDR4 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSDR5 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSDR6 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSv20120926 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSv20130417 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSv20150108 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSv20160114 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSv20160507 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSv20170630 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSv20180419 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSv20201209 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSv20231101 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VHSv20240731 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIDEODR2 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIDEODR3 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIDEODR4 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIDEODR5 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIDEOv20100513 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIDEOv20111208 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGDR2 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGDR3 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGDR4 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGv20110714 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGv20111019 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGv20130417 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGv20150421 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGv20151230 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGv20160406 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGv20161202 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VIKINGv20170715 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCDEEPv20230713 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCDEEPv20240506 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCDR1 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCDR3 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCDR4 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCDR5 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20110816 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20110909 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20120126 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20121128 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20130304 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20130805 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20140428 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20140903 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20150309 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20151218 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20160311 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20160822 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20170109 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20170411 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20171101 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20180702 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20181120 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20191212 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20210708 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20230816 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VMCv20240226 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VSAQC |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VVVDR1 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VVVDR2 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VVVDR5 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VVVXDR1 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VVVv20100531 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochFrameType |
Programme |
VVVv20110718 |
The frame type to be used for each epoch (stack, tile) |
varchar |
16 |
|
NONE |
|
epochMax |
ogle4CepLmcSource, ogle4CepSmcSource, ogle4RRLyrLmcSource, ogle4RRLyrSmcSource |
OGLE |
Time of maximum brightness (HJD-2450000) |
float |
8 |
days |
|
time.epoch |
epochMax |
vmcRRLyraeVariables |
VMCv20240226 |
Epoch of maximum light; EROS, (HJD-2,456,000 for sources, HJD-2455197.5 for Gaia DR2 sources). {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMax |
vmcRRlyraeVariables |
VMCDR4 |
Epoch of maximum light; EROS, (HJD-2,450,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMax |
vmcRRlyraeVariables |
VMCv20160822 |
Epoch of maximum light; EROS, (HJD-2,450,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMax |
vmcRRlyraeVariables |
VMCv20170109 |
Epoch of maximum light; EROS, (HJD-2,450,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMax |
vmcRRlyraeVariables |
VMCv20170411 |
Epoch of maximum light; EROS, (HJD-2,450,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMax |
vmcRRlyraeVariables |
VMCv20171101 |
Epoch of maximum light; EROS, (HJD-2,450,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMax |
vmcRRlyraeVariables |
VMCv20180702 |
Epoch of maximum light; EROS, (HJD-2,450,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMax |
vmcRRlyraeVariables |
VMCv20181120 |
Epoch of maximum light; EROS, (HJD-2,450,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMax |
vmcRRlyraeVariables |
VMCv20191212 |
Epoch of maximum light; EROS, (HJD-2,450,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMax |
vmcRRlyraeVariables |
VMCv20210708 |
Epoch of maximum light; EROS, (HJD-2,450,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMax |
vmcRRlyraeVariables |
VMCv20230816 |
Epoch of maximum light; EROS, (HJD-2,450,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MAX} |
real |
4 |
day |
|
time.epoch |
epochMean |
ObjectThin |
PS1DR2 |
Modified Julian Date of the mean epoch corresponding to raMean, decMean (equinox J2000). Note that Gaia DR1 data is sometimes included in the mean position; in those cases, the epochMean value is near the Gaia DR1 epoch 2015.5 = MJD 15023. As a result, epochMean is not necessarily near the mean value of the PS1 measurement dates. |
float |
8 |
days |
-999 |
|
epochmean |
decapsSource |
DECAPS |
Mean MJD {catalogue TType keyword: epochmean} |
float |
8 |
day |
-9.999995e8 |
stat.mean;time.epoch |
epochmean_ok |
decapsSource |
DECAPS |
Mean good MJD {catalogue TType keyword: epochmean_ok} |
float |
8 |
day |
-9.999995e8 |
stat.mean;time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCDR4 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20140903 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20150309 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20151218 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20160311 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20160822 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20170109 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20170411 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20171101 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20180702 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20181120 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20191212 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20210708 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20230816 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochMin |
vmcEclipsingBinaryVariables |
VMCv20240226 |
Epoch of minimum light; EROS, (HJD-2,400,000) determined by GRATIS in EROS R passband; OGLE (JD-2,400,000) from the OGLE III catalogue. {catalogue TType keyword: EPOCH_MIN} |
real |
4 |
day |
|
time.epoch |
epochrange |
decapsSource |
DECAPS |
MJD difference between first and last detection {catalogue TType keyword: epochrange} |
float |
8 |
day |
-9.999995e8 |
time.interval |
epochrange_ok |
decapsSource |
DECAPS |
MJD difference between first and last good detection {catalogue TType keyword: epochrange_ok} |
float |
8 |
day |
-9.999995e8 |
time.interval |
epochs |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
the total number of epochs across all pawprint sets used by the VIRAC pipeline {catalogue TType keyword: epochs} |
int |
4 |
|
-99999999 |
|
epochTolerance |
Programme |
SHARKSv20210222 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
SHARKSv20210421 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
ULTRAVISTADR4 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VHSDR5 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VHSDR6 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VHSv20160114 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VHSv20160507 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VHSv20170630 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VHSv20180419 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VHSv20201209 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VHSv20231101 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VHSv20240731 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VIKINGv20151230 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VIKINGv20160406 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VIKINGv20161202 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VIKINGv20170715 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCDEEPv20230713 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCDEEPv20240506 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCDR4 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCDR5 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20151218 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20160311 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20160822 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20170109 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20170411 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20171101 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20180702 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20181120 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20191212 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20210708 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20230816 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VMCv20240226 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VSAQC |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VVVDR5 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
epochTolerance |
Programme |
VVVXDR1 |
Minimum separation of epochs for proper motion calculation |
real |
4 |
days |
-0.9999995e9 |
?? |
equinox |
Multiframe |
SHARKSv20210222 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
SHARKSv20210421 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
ULTRAVISTADR4 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSDR1 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSDR2 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSDR3 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSDR4 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSDR5 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSDR6 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20120926 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20130417 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20140409 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20150108 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20160114 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20160507 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20170630 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20180419 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20201209 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20231101 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VHSv20240731 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIDEODR2 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIDEODR3 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIDEODR4 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIDEODR5 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIDEOv20100513 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIDEOv20111208 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGDR2 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGDR3 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGDR4 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGv20110714 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGv20111019 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGv20130417 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGv20140402 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGv20150421 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGv20151230 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGv20160406 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGv20161202 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VIKINGv20170715 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCDEEPv20230713 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCDEEPv20240506 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCDR1 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCDR2 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCDR3 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCDR4 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCDR5 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20110816 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20110909 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20120126 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20121128 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20130304 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20130805 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20140428 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20140903 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20150309 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20151218 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20160311 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20160822 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20170109 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20170411 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20171101 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20180702 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20181120 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20191212 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20210708 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20230816 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VMCv20240226 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VVVDR1 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VVVDR2 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VVVDR5 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VVVXDR1 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VVVv20100531 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
Multiframe |
VVVv20110718 |
Equinox of object position (Standard FK5) {image primary HDU keyword: EQUINOX} |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
equinox |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Equinox of object position (Standard FK5) |
real |
4 |
years |
-0.9999995e9 |
time.equinox |
erapm |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Error on RA (cosDec) component of proper motion {catalogue TType keyword: erapm} |
float |
8 |
mas/yr |
-999999500.0 |
|
erosid |
eros2LMCSource, eros2SMCSource, erosLMCSource, erosSMCSource |
EROS |
EROS star identification |
varchar |
24 |
|
|
|
erpmag_APASSDR9 |
ravedr5Source |
RAVE |
r' magnitude from APASSDR9 |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt |
err |
smashdr2_source |
SMASH |
Uncertainty of MAG |
real |
4 |
|
|
|
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 |
sharksDetection |
SHARKSv20210222 |
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 |
sharksDetection |
SHARKSv20210421 |
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 |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
errBits |
vhsDetection |
VHSDR1 |
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 |
vhsDetection |
VHSDR2 |
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 |
vhsDetection |
VHSDR3 |
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 |
vhsDetection |
VHSDR4 |
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 |
vhsDetection |
VHSDR5 |
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 |
vhsDetection |
VHSDR6 |
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 |
vhsDetection |
VHSv20120926 |
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 |
vhsDetection |
VHSv20130417 |
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 |
vhsDetection |
VHSv20140409 |
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 |
vhsDetection |
VHSv20150108 |
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 |
vhsDetection |
VHSv20160114 |
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 |
vhsDetection |
VHSv20160507 |
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 |
vhsDetection |
VHSv20170630 |
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 |
vhsDetection |
VHSv20180419 |
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 |
vhsDetection |
VHSv20201209 |
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 |
vhsDetection |
VHSv20231101 |
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 |
vhsDetection |
VHSv20240731 |
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 |
vhsListRemeasurement |
VHSDR1 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
errBits |
videoDetection |
VIDEODR2 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
errBits |
videoDetection |
VIDEODR3 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
errBits |
videoDetection |
VIDEODR4 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
errBits |
videoDetection |
VIDEODR5 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
errBits |
videoDetection |
VIDEOv20100513 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
errBits |
videoDetection |
VIDEOv20111208 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
errBits |
videoListRemeasurement |
VIDEOv20100513 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
errBits |
vikingDetection |
VIKINGDR2 |
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 |
vikingDetection |
VIKINGDR3 |
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 |
vikingDetection |
VIKINGDR4 |
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 |
vikingDetection |
VIKINGv20110714 |
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 |
vikingDetection |
VIKINGv20111019 |
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 |
vikingDetection |
VIKINGv20130417 |
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 |
vikingDetection |
VIKINGv20140402 |
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 |
vikingDetection |
VIKINGv20150421 |
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 |
vikingDetection |
VIKINGv20151230 |
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 |
vikingDetection |
VIKINGv20160406 |
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 |
vikingDetection |
VIKINGv20161202 |
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 |
vikingDetection |
VIKINGv20170715 |
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 |
vikingListRemeasurement |
VIKINGv20110714 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
errBits |
vikingListRemeasurement |
VIKINGv20111019 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
errBits |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
errBits |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
errBits |
vmcDetection |
VMCDR1 |
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 |
vmcDetection |
VMCDR2 |
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 |
vmcDetection |
VMCDR3 |
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 |
vmcDetection |
VMCDR4 |
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 |
vmcDetection |
VMCDR5 |
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 |
vmcDetection |
VMCv20110816 |
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 |
vmcDetection |
VMCv20110909 |
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 |
vmcDetection |
VMCv20120126 |
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 |
vmcDetection |
VMCv20121128 |
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 |
vmcDetection |
VMCv20130304 |
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 |
vmcDetection |
VMCv20130805 |
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 |
vmcDetection |
VMCv20140428 |
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 |
vmcDetection |
VMCv20140903 |
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 |
vmcDetection |
VMCv20150309 |
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 |
vmcDetection |
VMCv20151218 |
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 |
vmcDetection |
VMCv20160311 |
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 |
vmcDetection |
VMCv20160822 |
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 |
vmcDetection |
VMCv20170109 |
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 |
vmcDetection |
VMCv20170411 |
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 |
vmcDetection |
VMCv20171101 |
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 |
vmcDetection |
VMCv20180702 |
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 |
vmcDetection |
VMCv20181120 |
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 |
vmcDetection |
VMCv20191212 |
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 |
vmcDetection |
VMCv20210708 |
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 |
vmcDetection |
VMCv20230816 |
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 |
vmcDetection |
VMCv20240226 |
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 |
vmcListRemeasurement |
VMCv20110816 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
errBits |
vmcListRemeasurement |
VMCv20110909 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
errBits |
vmcdeepDetection |
VMCDEEPv20230713 |
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 |
vmcdeepDetection |
VMCDEEPv20240506 |
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 |
vvvDetection |
VVVDR1 |
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 |
vvvDetection |
VVVDR2 |
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 |
vvvDetection |
VVVv20100531 |
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 |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
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 |
vvvListRemeasurement |
VVVv20100531 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
errBits |
vvvListRemeasurement |
VVVv20110718 |
processing warning/error bitwise flags {catalogue TType keyword: Error_bit_flag} |
int |
4 |
|
|
meta.code |
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 |
ErrMB |
eros2LMCSource, eros2SMCSource, erosLMCSource, erosSMCSource |
EROS |
Error of mean magnitude in blue channel |
real |
4 |
|
|
|
ErrMR |
eros2LMCSource, eros2SMCSource, erosLMCSource, erosSMCSource |
EROS |
Error of mean magnitude in red channel |
real |
4 |
|
|
|
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 |
SHARKSv20210222 |
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 |
SHARKSv20210421 |
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 |
ULTRAVISTADR4 |
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 |
VHSDR1 |
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 |
VHSDR2 |
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 |
VHSDR3 |
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 |
VHSDR4 |
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 |
VHSDR5 |
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 |
VHSDR6 |
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 |
VHSv20120926 |
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 |
VHSv20130417 |
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 |
VHSv20140409 |
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 |
VHSv20150108 |
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 |
VHSv20160114 |
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 |
VHSv20160507 |
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 |
VHSv20170630 |
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 |
VHSv20180419 |
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 |
VHSv20201209 |
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 |
VHSv20231101 |
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 |
VHSv20240731 |
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 |
VIDEODR2 |
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 |
VIDEODR3 |
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 |
VIDEODR4 |
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 |
VIDEODR5 |
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 |
VIDEOv20100513 |
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 |
VIDEOv20111208 |
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 |
VIKINGDR2 |
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 |
VIKINGDR3 |
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 |
VIKINGDR4 |
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 |
VIKINGv20110714 |
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 |
VIKINGv20111019 |
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 |
VIKINGv20130417 |
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 |
VIKINGv20140402 |
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 |
VIKINGv20150421 |
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 |
VIKINGv20151230 |
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 |
VIKINGv20160406 |
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 |
VIKINGv20161202 |
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 |
VIKINGv20170715 |
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 |
VMCDEEPv20230713 |
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 |
VMCDEEPv20240506 |
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 |
VMCDR1 |
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 |
VMCDR2 |
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 |
VMCDR3 |
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 |
VMCDR4 |
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 |
VMCDR5 |
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 |
VMCv20110816 |
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 |
VMCv20110909 |
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 |
VMCv20120126 |
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 |
VMCv20121128 |
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 |
VMCv20130304 |
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 |
VMCv20130805 |
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 |
VMCv20140428 |
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 |
VMCv20140903 |
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 |
VMCv20150309 |
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 |
VMCv20151218 |
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 |
VMCv20160311 |
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 |
VMCv20160822 |
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 |
VMCv20170109 |
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 |
VMCv20170411 |
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 |
VMCv20171101 |
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 |
VMCv20180702 |
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 |
VMCv20181120 |
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 |
VMCv20191212 |
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 |
VMCv20210708 |
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 |
VMCv20230816 |
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 |
VMCv20240226 |
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 |
VVVDR1 |
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 |
VVVDR2 |
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 |
VVVDR5 |
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 |
VVVXDR1 |
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 |
VVVv20100531 |
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 |
VVVv20110718 |
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 |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Declination of the Moon (J2000) (deg) |
float |
8 |
|
-0.9999995e9 |
pos.eq.dec;meta.main |
esoGrade |
Multiframe |
SHARKSv20210222 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
SHARKSv20210421 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
ULTRAVISTADR4 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSDR1 |
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 |
VHSDR2 |
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 |
VHSDR3 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSDR4 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSDR5 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSDR6 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSv20120926 |
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 |
VHSv20130417 |
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 |
VHSv20140409 |
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 |
VHSv20150108 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSv20160114 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSv20160507 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSv20170630 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSv20180419 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSv20201209 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSv20231101 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VHSv20240731 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VIDEODR2 |
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 |
VIDEODR3 |
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 |
VIDEODR4 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VIDEODR5 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VIDEOv20111208 |
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 |
VIKINGDR2 |
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 |
VIKINGDR3 |
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 |
VIKINGDR4 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VIKINGv20110714 |
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 |
VIKINGv20111019 |
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 |
VIKINGv20130417 |
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 |
VIKINGv20140402 |
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 |
VIKINGv20150421 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VIKINGv20151230 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VIKINGv20160406 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VIKINGv20161202 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VIKINGv20170715 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCDEEPv20230713 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCDEEPv20240506 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCDR1 |
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 |
VMCDR2 |
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 |
VMCDR3 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCDR4 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCDR5 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20110816 |
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 |
VMCv20110909 |
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 |
VMCv20120126 |
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 |
VMCv20121128 |
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 |
VMCv20130304 |
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 |
VMCv20130805 |
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 |
VMCv20140428 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20140903 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20150309 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20151218 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20160311 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20160822 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20170109 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20170411 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20171101 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20180702 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20181120 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20191212 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20210708 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20230816 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VMCv20240226 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VVVDR1 |
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 |
VVVDR2 |
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 |
VVVDR5 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VVVXDR1 |
ESO QC grade: 'A' if fully under constraints, 'B' if mostly (90%) under constraints, 'C' if out of constraints and 'R' rejected. {image primary HDU keyword: ESOGRADE} |
varchar |
4 |
|
NONE |
?? |
esoGrade |
Multiframe |
VVVv20110718 |
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 |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
ESO QC grade: 'A' if fully under constrains, 'B' if mostly (90%) under constrains, 'C' if out of constrains and 'R' rejected. |
varchar |
4 |
|
NONE |
?? |
esoRaMoon |
Multiframe |
SHARKSv20210222 |
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 |
SHARKSv20210421 |
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 |
ULTRAVISTADR4 |
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 |
VHSDR1 |
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 |
VHSDR2 |
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 |
VHSDR3 |
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 |
VHSDR4 |
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 |
VHSDR5 |
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 |
VHSDR6 |
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 |
VHSv20120926 |
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 |
VHSv20130417 |
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 |
VHSv20140409 |
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 |
VHSv20150108 |
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 |
VHSv20160114 |
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 |
VHSv20160507 |
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 |
VHSv20170630 |
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 |
VHSv20180419 |
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 |
VHSv20201209 |
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 |
VHSv20231101 |
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 |
VHSv20240731 |
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 |
VIDEODR2 |
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 |
VIDEODR3 |
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 |
VIDEODR4 |
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 |
VIDEODR5 |
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 |
VIDEOv20100513 |
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 |
VIDEOv20111208 |
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 |
VIKINGDR2 |
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 |
VIKINGDR3 |
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 |
VIKINGDR4 |
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 |
VIKINGv20110714 |
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 |
VIKINGv20111019 |
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 |
VIKINGv20130417 |
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 |
VIKINGv20140402 |
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 |
VIKINGv20150421 |
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 |
VIKINGv20151230 |
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 |
VIKINGv20160406 |
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 |
VIKINGv20161202 |
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 |
VIKINGv20170715 |
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 |
VMCDEEPv20230713 |
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 |
VMCDEEPv20240506 |
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 |
VMCDR1 |
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 |
VMCDR2 |
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 |
VMCDR3 |
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 |
VMCDR4 |
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 |
VMCDR5 |
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 |
VMCv20110816 |
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 |
VMCv20110909 |
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 |
VMCv20120126 |
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 |
VMCv20121128 |
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 |
VMCv20130304 |
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 |
VMCv20130805 |
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 |
VMCv20140428 |
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 |
VMCv20140903 |
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 |
VMCv20150309 |
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 |
VMCv20151218 |
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 |
VMCv20160311 |
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 |
VMCv20160822 |
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 |
VMCv20170109 |
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 |
VMCv20170411 |
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 |
VMCv20171101 |
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 |
VMCv20180702 |
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 |
VMCv20181120 |
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 |
VMCv20191212 |
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 |
VMCv20210708 |
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 |
VMCv20230816 |
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 |
VMCv20240226 |
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 |
VVVDR1 |
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 |
VVVDR2 |
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 |
VVVDR5 |
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 |
VVVXDR1 |
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 |
VVVv20100531 |
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 |
VVVv20110718 |
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 |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Right ascension of the Moon (J2000) (deg) |
float |
8 |
|
-0.9999995e9 |
pos.eq.ra;meta.main |
eta |
CurrentAstrometry |
SHARKSv20210222 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
SHARKSv20210421 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
ULTRAVISTADR4 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSDR1 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSDR2 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSDR3 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSDR4 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSDR5 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSDR6 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20120926 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20130417 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20140409 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20150108 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20160114 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20160507 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20170630 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20180419 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20201209 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20231101 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VHSv20240731 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIDEODR2 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIDEODR3 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIDEODR4 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIDEODR5 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIDEOv20100513 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIDEOv20111208 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGDR2 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGDR3 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGDR4 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGv20110714 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGv20111019 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGv20130417 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGv20140402 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGv20150421 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGv20151230 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGv20160406 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGv20161202 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VIKINGv20170715 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCDEEPv20230713 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCDEEPv20240506 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCDR1 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCDR2 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCDR3 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCDR4 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCDR5 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20110816 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20110909 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20120126 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20121128 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20130304 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20130805 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20140428 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20140903 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20150309 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20151218 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20160311 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20160822 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20170109 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20170411 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20171101 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20180702 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20181120 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20191212 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20210708 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20230816 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VMCv20240226 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VVVDR1 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VVVDR2 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VVVDR5 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VVVXDR1 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VVVv20100531 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
CurrentAstrometry |
VVVv20110718 |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos |
eta |
gaiaxwise_matches |
GAIAXWISE |
Photometric logarithmic likelihood ratio of Gaia-WISE match, as described by equation 37 of Wilson & Naylor (2018a, MNRAS, 473, 5570). |
float |
8 |
dimensionless |
|
|
eta |
sharksCurrentAstrometry, ultravistaCurrentAstrometry, vhsCurrentAstrometry, videoCurrentAstrometry, vikingCurrentAstrometry, vmcCurrentAstrometry, vvvCurrentAstrometry |
VSAQC |
SDSS system spherical co-ordinate 2 of device centre |
float |
8 |
Degrees |
|
pos |
eta |
sharksDetection |
SHARKSv20210421 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
sharksDetection, sharksSource, sharksTilePawPrints |
SHARKSv20210222 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
sharksTilePawTDOnly |
SHARKSv20210222 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
sharksTilePawTDOnly |
SHARKSv20210421 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
ultravistaDetection, ultravistaMapRemeasAver, ultravistaMapRemeasurement, ultravistaSource, ultravistaTilePawPrints |
ULTRAVISTADR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
SDSS system spherical co-ordinate 2 of aperture |
float |
8 |
Degrees |
|
pos |
eta |
ultravistaTilePawTDOnly |
ULTRAVISTADR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSDR3 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSDR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSDR5 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSDR6 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20120926 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20130417 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20140409 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20150108 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20160114 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20160507 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20170630 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20180419 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20201209 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20231101 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection |
VHSv20240731 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection, vhsListRemeasurement, vhsSource, vhsSourceRemeasurement, vhsTilePawPrints |
VHSDR1 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsDetection, vhsSource, vhsTilePawPrints |
VHSDR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSDR1 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSDR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSDR3 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSDR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSDR5 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSDR6 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20120926 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20130417 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20140409 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20150108 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20160114 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20160507 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20170630 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20180419 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20201209 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20231101 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vhsTilePawTDOnly |
VHSv20240731 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoDetection |
VIDEODR3 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoDetection |
VIDEODR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoDetection |
VIDEODR5 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoDetection |
VIDEOv20111208 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoDetection, videoListRemeasurement, videoSourceRemeasurement |
VIDEOv20100513 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoDetection, videoSource, videoTilePawPrints |
VIDEODR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoTilePawTDOnly |
VIDEODR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoTilePawTDOnly |
VIDEODR3 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoTilePawTDOnly |
VIDEODR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoTilePawTDOnly |
VIDEODR5 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
videoTilePawTDOnly |
VIDEOv20111208 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection |
VIKINGDR3 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection |
VIKINGDR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection |
VIKINGv20111019 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection |
VIKINGv20130417 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection |
VIKINGv20140402 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection |
VIKINGv20150421 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection |
VIKINGv20151230 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection |
VIKINGv20160406 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection |
VIKINGv20161202 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection |
VIKINGv20170715 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection, vikingListRemeasurement, vikingSourceRemeasurement |
VIKINGv20110714 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingDetection, vikingSource, vikingTilePawPrints |
VIKINGDR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingMapRemeasAver, vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGDR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGDR3 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGDR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGv20111019 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGv20130417 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGv20140402 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGv20150421 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGv20151230 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGv20160406 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGv20161202 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingTilePawTDOnly |
VIKINGv20170715 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
SDSS system spherical co-ordinate 2 of aperture |
float |
8 |
Degrees |
|
pos |
eta |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
SDSS system spherical co-ordinate 2 of aperture |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCDR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCDR3 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCDR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCDR5 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20110909 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20120126 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20121128 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20130304 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20130805 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20140428 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20140903 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20150309 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20151218 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20160311 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20160822 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20170109 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20170411 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20171101 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20180702 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20181120 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20191212 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20210708 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20230816 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection |
VMCv20240226 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection, vmcListRemeasurement, vmcSourceRemeasurement |
VMCv20110816 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcDetection, vmcSource, vmcSynopticSource, vmcTilePawPrints |
VMCDR1 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCDR1 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCDR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCDR3 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCDR4 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCDR5 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20110816 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20110909 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20120126 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20121128 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20130304 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20130805 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20140428 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20140903 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20150309 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20151218 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20160311 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20160822 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20170109 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20170411 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20171101 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20180702 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20181120 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20191212 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20210708 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20230816 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcTilePawTDOnly |
VMCv20240226 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcdeepDetection |
VMCDEEPv20240506 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcdeepDetection, vmcdeepSource, vmcdeepSynopticSource, vmcdeepTilePawPrints |
VMCDEEPv20230713 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcdeepTilePawTDOnly |
VMCDEEPv20230713 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vmcdeepTilePawTDOnly |
VMCDEEPv20240506 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vvvDetection |
VVVDR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vvvDetection, vvvListRemeasurement, vvvSourceRemeasurement |
VVVv20100531 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vvvDetection, vvvSource, vvvSynopticSource, vvvTilePawPrints |
VVVDR1 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vvvTilePawTDOnly |
VVVDR1 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vvvTilePawTDOnly |
VVVDR2 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vvvTilePawTDOnly |
VVVDR5 |
SDSS system spherical co-ordinate 2 |
float |
8 |
Degrees |
|
pos |
eta |
vvvxSource |
VVVXDR1 |
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 |
evi |
vmcCepheidVariables |
VMCDR3 |
The dust extinction value E(V-I) {catalogue TType keyword: E(V-I)} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
evi |
vmcCepheidVariables |
VMCv20121128 |
The dust extinction value E(V-I) {catalogue TType keyword: E(V-I)} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
evi |
vmcCepheidVariables |
VMCv20140428 |
The dust extinction value E(V-I) {catalogue TType keyword: E(V-I)} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
evi |
vmcCepheidVariables |
VMCv20140903 |
The dust extinction value E(V-I) {catalogue TType keyword: E(V-I)} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
evi |
vmcCepheidVariables |
VMCv20150309 |
The dust extinction value E(V-I) {catalogue TType keyword: E(V-I)} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
evi |
vmcCepheidVariables |
VMCv20151218 |
The dust extinction value E(V-I) {catalogue TType keyword: E(V-I)} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
evi |
vmcCepheidVariables |
VMCv20160311 |
The dust extinction value E(V-I) {catalogue TType keyword: E(V-I)} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
evi |
vmcCepheidVariables |
VMCv20160822 |
The dust extinction value E(V-I) {catalogue TType keyword: E(V-I)} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
evi |
vmcCepheidVariables, vmcRRlyraeVariables |
VMCDR4 |
The dust extinction value E(V-I) {catalogue TType keyword: E(V-I)} |
real |
4 |
mag |
-0.9999995e9 |
phys.absorption.gal |
eVmag_APASSDR9 |
ravedr5Source |
RAVE |
error V magnitude from APASSDR9 |
real |
4 |
mag |
|
stat.error;phot.mag;em.opt.V |
evolStatus |
ogle3LpvLmcSource, ogle3LpvSmcSource |
OGLE |
Evolutionary status (RGB, AGB) |
varchar |
3 |
|
|
meta.code.status;time.age |
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 |
EXP_R |
spectra |
SIXDF |
R reference frame exposure time seconds |
real |
4 |
seconds |
|
|
EXP_V |
spectra |
SIXDF |
V reference frame exposure time seconds |
real |
4 |
seconds |
|
|
expAstErr |
sharksVariability |
SHARKSv20210222 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
sharksVariability |
SHARKSv20210421 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
ultravistaVariability |
ULTRAVISTADR4 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
videoVariability |
VIDEODR2 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
videoVariability |
VIDEODR3 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
videoVariability |
VIDEODR4 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
videoVariability |
VIDEODR5 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
videoVariability |
VIDEOv20100513 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
videoVariability |
VIDEOv20111208 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGDR2 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGDR3 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGDR4 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGv20110714 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGv20111019 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGv20130417 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGv20140402 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGv20150421 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGv20151230 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGv20160406 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGv20161202 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vikingVariability |
VIKINGv20170715 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCDR1 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCDR2 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCDR3 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCDR4 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCDR5 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20110816 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20110909 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20120126 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20121128 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20130304 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20130805 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20140428 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20140903 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20150309 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20151218 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20160311 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20160822 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20170109 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20170411 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20171101 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20180702 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20181120 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20191212 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20210708 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20230816 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcVariability |
VMCv20240226 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcdeepVariability |
VMCDEEPv20230713 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vmcdeepVariability |
VMCDEEPv20240506 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vvvVariability |
VVVDR1 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vvvVariability |
VVVDR2 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vvvVariability |
VVVDR5 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vvvVariability |
VVVv20100531 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vvvVariability |
VVVv20110718 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expAstErr |
vvvxVariability |
VVVXDR1 |
Rms calculated from polynomial fit to minimum astrometric RMS as a function of magnitude |
real |
4 |
arcsec |
-0.9999995e9 |
stat.error |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
expnum |
smashdr2_source |
SMASH |
Eight-digit exposure number |
varchar |
8 |
|
|
|
expRMSNoise |
vvvVivaCatalogue |
VVVDR5 |
Expected noise value for even dispersion parameter of Ks pawprint data {catalogue TType keyword: ExpRmsNoise} |
float |
8 |
mag |
-9.999995e8 |
|
expTime |
Detection |
PS1DR2 |
Exposure time of the frame/exposure. Necessary for converting listed fluxes and magnitudes back to measured ADU counts. |
real |
4 |
seconds |
-999 |
|
expTime |
Multiframe |
SHARKSv20210222 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
SHARKSv20210421 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
ULTRAVISTADR4 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSDR1 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSDR2 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSDR3 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSDR4 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSDR5 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSDR6 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20120926 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20130417 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20140409 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20150108 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20160114 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20160507 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20170630 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20180419 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20201209 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20231101 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VHSv20240731 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIDEODR2 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIDEODR3 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIDEODR4 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIDEODR5 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIDEOv20100513 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIDEOv20111208 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGDR2 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGDR3 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGDR4 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGv20110714 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGv20111019 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGv20130417 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGv20140402 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGv20150421 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGv20151230 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGv20160406 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGv20161202 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VIKINGv20170715 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCDEEPv20230713 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCDEEPv20240506 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCDR1 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCDR2 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCDR3 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCDR4 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCDR5 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20110816 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20110909 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20120126 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20121128 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20130304 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20130805 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20140428 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20140903 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20150309 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20151218 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20160311 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20160822 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20170109 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20170411 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20171101 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20180702 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20181120 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20191212 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20210708 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20230816 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VMCv20240226 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VVVDR1 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VVVDR2 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VVVDR5 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VVVXDR1 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VVVv20100531 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
expTime |
Multiframe |
VVVv20110718 |
Integration time per exposure (corrected to ndit = 1) {image primary HDU keyword: EXPTIME} |
real |
4 |
seconds |
-0.9999995e9 |
time.duration;obs.exposure |
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 |
expTime |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Integration time per exposure (corrected to ndit = 1) |
real |
4 |
seconds |
-0.9999995e9 |
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 |
externalID |
vmcCepheidVariables |
VMCDR4 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20160311 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20160822 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20170109 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20170411 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20171101 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20180702 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20181120 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20191212 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20210708 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20230816 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcCepheidVariables |
VMCv20240226 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
'NONE' |
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20140903 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20150309 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20151218 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20160311 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20160822 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20170109 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20170411 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20171101 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20180702 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20181120 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20191212 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20210708 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20230816 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables |
VMCv20240226 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
externalID |
vmcEclipsingBinaryVariables, vmcRRlyraeVariables |
VMCDR4 |
EROS-2/OGLE III ID: Identification from the EROS-2 or OGLE III catalogues. {catalogue TType keyword: EXT_ID} |
varchar |
32 |
|
|
meta.id |
extID |
vmcRRLyraeVariables |
VMCv20240226 |
UID: External OGLE IV if 5 digits or Gaia DR2 >9 digits {catalogue TType keyword: ext_id} |
bigint |
8 |
|
|
meta.id |
extID |
vvvBulge3DExtinctVals |
EXTINCT |
UID of the 3D spatial position |
bigint |
8 |
|
|
meta.id;meta.main |
extinctionCat |
MultiframeDetector |
SHARKSv20210222 |
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 |
SHARKSv20210421 |
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 |
ULTRAVISTADR4 |
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 |
VHSDR1 |
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 |
VHSDR2 |
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 |
VHSDR3 |
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 |
VHSDR4 |
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 |
VHSDR5 |
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 |
VHSDR6 |
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 |
VHSv20120926 |
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 |
VHSv20130417 |
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 |
VHSv20140409 |
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 |
VHSv20150108 |
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 |
VHSv20160114 |
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 |
VHSv20160507 |
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 |
VHSv20170630 |
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 |
VHSv20180419 |
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 |
VHSv20201209 |
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 |
VHSv20231101 |
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 |
VHSv20240731 |
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 |
VIDEODR2 |
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 |
VIDEODR3 |
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 |
VIDEODR4 |
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 |
VIDEODR5 |
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 |
VIDEOv20100513 |
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 |
VIDEOv20111208 |
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 |
VIKINGDR2 |
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 |
VIKINGDR3 |
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 |
VIKINGDR4 |
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 |
VIKINGv20110714 |
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 |
VIKINGv20111019 |
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 |
VIKINGv20130417 |
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 |
VIKINGv20140402 |
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 |
VIKINGv20150421 |
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 |
VIKINGv20151230 |
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 |
VIKINGv20160406 |
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 |
VIKINGv20161202 |
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 |
VIKINGv20170715 |
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 |
VMCDEEPv20230713 |
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 |
VMCDEEPv20240506 |
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 |
VMCDR1 |
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 |
VMCDR2 |
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 |
VMCDR3 |
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 |
VMCDR4 |
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 |
VMCDR5 |
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 |
VMCv20110816 |
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 |
VMCv20110909 |
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 |
VMCv20120126 |
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 |
VMCv20121128 |
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 |
VMCv20130304 |
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 |
VMCv20130805 |
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 |
VMCv20140428 |
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 |
VMCv20140903 |
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 |
VMCv20150309 |
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 |
VMCv20151218 |
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 |
VMCv20160311 |
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 |
VMCv20160822 |
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 |
VMCv20170109 |
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 |
VMCv20170411 |
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 |
VMCv20171101 |
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 |
VMCv20180702 |
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 |
VMCv20181120 |
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 |
VMCv20191212 |
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 |
VMCv20210708 |
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 |
VMCv20230816 |
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 |
VMCv20240226 |
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 |
VVVDR1 |
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 |
VVVDR2 |
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 |
VVVDR5 |
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 |
VVVXDR1 |
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 |
VVVv20100531 |
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 |
VVVv20110718 |
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 |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Extinction coefficient for the catalogue data |
real |
4 |
mags |
-0.9999995e9 |
?? |
extinctionExt |
MultiframeDetector |
SHARKSv20210222 |
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 |
SHARKSv20210421 |
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 |
ULTRAVISTADR4 |
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 |
VHSDR1 |
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 |
VHSDR2 |
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 |
VHSDR3 |
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 |
VHSDR4 |
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 |
VHSDR5 |
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 |
VHSDR6 |
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 |
VHSv20120926 |
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 |
VHSv20130417 |
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 |
VHSv20140409 |
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 |
VHSv20150108 |
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 |
VHSv20160114 |
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 |
VHSv20160507 |
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 |
VHSv20170630 |
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 |
VHSv20180419 |
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 |
VHSv20201209 |
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 |
VHSv20231101 |
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 |
VHSv20240731 |
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 |
VIDEODR2 |
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 |
VIDEODR3 |
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 |
VIDEODR4 |
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 |
VIDEODR5 |
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 |
VIDEOv20100513 |
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 |
VIDEOv20111208 |
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 |
VIKINGDR2 |
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 |
VIKINGDR3 |
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 |
VIKINGDR4 |
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 |
VIKINGv20110714 |
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 |
VIKINGv20111019 |
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 |
VIKINGv20130417 |
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 |
VIKINGv20140402 |
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 |
VIKINGv20150421 |
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 |
VIKINGv20151230 |
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 |
VIKINGv20160406 |
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 |
VIKINGv20161202 |
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 |
VIKINGv20170715 |
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 |
VMCDEEPv20230713 |
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 |
VMCDEEPv20240506 |
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 |
VMCDR1 |
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 |
VMCDR2 |
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 |
VMCDR3 |
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 |
VMCDR4 |
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 |
VMCDR5 |
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 |
VMCv20110816 |
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 |
VMCv20110909 |
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 |
VMCv20120126 |
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 |
VMCv20121128 |
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 |
VMCv20130304 |
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 |
VMCv20130805 |
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 |
VMCv20140428 |
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 |
VMCv20140903 |
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 |
VMCv20150309 |
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 |
VMCv20151218 |
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 |
VMCv20160311 |
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 |
VMCv20160822 |
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 |
VMCv20170109 |
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 |
VMCv20170411 |
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 |
VMCv20171101 |
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 |
VMCv20180702 |
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 |
VMCv20181120 |
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 |
VMCv20191212 |
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 |
VMCv20210708 |
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 |
VMCv20230816 |
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 |
VMCv20240226 |
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 |
VVVDR1 |
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 |
VVVDR2 |
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 |
VVVDR5 |
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 |
VVVXDR1 |
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 |
VVVv20100531 |
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 |
VVVv20110718 |
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 |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Extinction coefficient of the detector |
real |
4 |
mags |
-0.9999995e9 |
?? |
extinctionMapList |
Programme |
SHARKSv20210222 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
SHARKSv20210421 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
ULTRAVISTADR4 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VHSDR4 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VHSDR5 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VHSDR6 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VHSv20160114 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VHSv20160507 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VHSv20170630 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VHSv20180419 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VHSv20201209 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VHSv20231101 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VHSv20240731 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VIDEODR5 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VIKINGv20150421 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VIKINGv20151230 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VIKINGv20160406 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VIKINGv20161202 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VIKINGv20170715 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCDEEPv20230713 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCDEEPv20240506 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCDR4 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCDR5 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20150309 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20151218 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20160311 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20160822 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20170109 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20170411 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20171101 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20180702 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20181120 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20191212 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20210708 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20230816 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VMCv20240226 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VSAQC |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VVVDR5 |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
extinctionMapList |
Programme |
VVVXDR1 |
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 |
vvvSourceExtinction |
VVVDR5 |
UID of 3D extinction map used |
tinyint |
1 |
|
0 |
|
extMapID |
vvvxSourceExtinction |
VVVXDR1 |
UID of 3D extinction map used |
tinyint |
1 |
|
0 |
|
extNSigma |
Detection |
PS1DR2 |
An extendedness measure based on the deviation between PSF and Kron (1980) magnitudes, normalized by the PSF magnitude uncertainty. |
real |
4 |
|
0 |
|
extNum |
CurrentAstrometry |
SHARKSv20210421 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
ULTRAVISTADR4 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSDR1 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSDR2 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSDR3 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSDR4 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSDR5 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSDR6 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20120926 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20130417 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20140409 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20150108 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20160114 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20160507 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20170630 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20180419 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20201209 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20231101 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VHSv20240731 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIDEODR2 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIDEODR3 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIDEODR4 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIDEODR5 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIDEOv20100513 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIDEOv20111208 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGDR2 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGDR3 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGDR4 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGv20110714 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGv20111019 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGv20130417 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGv20140402 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGv20150421 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGv20151230 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGv20160406 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGv20161202 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VIKINGv20170715 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCDEEPv20230713 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCDEEPv20240506 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCDR1 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCDR2 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCDR3 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCDR4 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCDR5 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20110816 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20110909 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20120126 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20121128 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20130304 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20130805 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20140428 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20140903 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20150309 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20151218 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20160311 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20160822 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20170109 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20170411 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20171101 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20180702 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20181120 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20191212 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20210708 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20230816 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VMCv20240226 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VVVDR1 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VVVDR2 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VVVDR5 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VVVXDR1 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VVVv20100531 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry |
VVVv20110718 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
CurrentAstrometry, EpochFrameStatus, MapCatalogueDetector, MultiframeDetector, MultiframeDetectorEsoKeys |
SHARKSv20210222 |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
extNum |
PreviousMFDZP |
SHARKSv20210421 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSDR2 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSDR3 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSDR4 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSDR5 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20120926 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20130417 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20140409 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20150108 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20160114 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20160507 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20170630 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20180419 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20201209 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20231101 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VHSv20240731 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIDEODR3 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIDEODR4 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIDEODR5 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIDEOv20111208 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIKINGDR3 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIKINGDR4 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIKINGv20111019 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIKINGv20130417 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIKINGv20140402 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIKINGv20150421 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIKINGv20151230 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIKINGv20160406 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIKINGv20161202 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VIKINGv20170715 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCDEEPv20230713 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCDEEPv20240506 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCDR2 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCDR3 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCDR4 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCDR5 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20110909 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20120126 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20121128 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20130304 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20130805 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20140428 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20140903 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20150309 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20151218 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20160311 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20160822 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20170109 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20170411 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20171101 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20180702 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20181120 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20191212 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20210708 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20230816 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VMCv20240226 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VVVDR2 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VVVXDR1 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP |
VVVv20110718 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, sharksAstrometricInfo, sharksDetection, sharksSourceXDetectionBestMatch |
SHARKSv20210222 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, ultravistaAstrometricInfo, ultravistaDetection, ultravistaMapRemeasAver, ultravistaMapRemeasurement, ultravistaSourceXDetectionBestMatch |
ULTRAVISTADR4 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, vhsAstrometricInfo |
VHSDR6 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, vhsDetection, vhsListRemeasurement |
VHSDR1 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, videoAstrometricInfo, videoDetection, videoSourceXDetectionBestMatch |
VIDEODR2 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, videoListRemeasurement |
VIDEOv20100513 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, vikingAstrometricInfo, vikingDetection, vikingSourceXDetectionBestMatch |
VIKINGDR2 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, vikingListRemeasurement |
VIKINGv20110714 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, vmcAstrometricInfo, vmcDetection |
VMCDR1 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, vmcListRemeasurement |
VMCv20110816 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, vvvAstrometricInfo, vvvDetection, vvvSourceXDetectionBestMatch |
VVVDR1 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
PreviousMFDZP, vvvListRemeasurement |
VVVv20100531 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
sharksCurrentAstrometry, sharksMultiframeDetector, ultravistaCurrentAstrometry, ultravistaMultiframeDetector, vhsCurrentAstrometry, vhsMultiframeDetector, videoCurrentAstrometry, videoMultiframeDetector, vikingCurrentAstrometry, vikingMultiframeDetector, vmcCurrentAstrometry, vmcMultiframeDetector, vvvCurrentAstrometry, vvvMultiframeDetector |
VSAQC |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
vikingMapRemeasAver, vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
extNum |
vmcdeepAstrometricInfo |
VMCDEEPv20240506 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.id |
extNum |
vmcdeepAstrometricInfo, vmcdeepDetection |
VMCDEEPv20230713 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.id |
extNum |
vvvxAstrometricInfo, vvvxSourceXDetectionBestMatch |
VVVXDR1 |
the extension number of this frame |
tinyint |
1 |
|
|
meta.id |
extPixelID |
vvvSourceExtinction |
VVVDR5 |
Pixel ID from 3D extinction map that matches source position |
int |
4 |
|
-99999999 |
|
extPixelID |
vvvxSourceExtinction |
VVVXDR1 |
Pixel ID from 3D extinction map that matches source position |
int |
4 |
|
-99999999 |
|
extProgID |
RequiredNeighbours |
SHARKSv20210222 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
SHARKSv20210421 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
ULTRAVISTADR4 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSDR1 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSDR2 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSDR3 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSDR4 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSDR5 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSDR6 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSv20120926 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSv20130417 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSv20150108 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSv20160114 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSv20160507 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSv20170630 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSv20180419 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSv20201209 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSv20231101 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VHSv20240731 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIDEODR2 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIDEODR3 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIDEODR4 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIDEODR5 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIDEOv20100513 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIDEOv20111208 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGDR2 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGDR3 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGDR4 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGv20110714 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGv20111019 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGv20130417 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGv20150421 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGv20151230 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGv20160406 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGv20161202 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VIKINGv20170715 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCDEEPv20230713 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCDEEPv20240506 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCDR1 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCDR3 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCDR4 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCDR5 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20110816 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20110909 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20120126 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20121128 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20130304 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20130805 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20140428 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20140903 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20150309 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20151218 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20160311 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20160822 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20170109 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20170411 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20171101 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20180702 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20181120 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20191212 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20210708 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20230816 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VMCv20240226 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VSAQC |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VVVDR1 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VVVDR2 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VVVDR5 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VVVXDR1 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VVVv20100531 |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
extProgID |
RequiredNeighbours |
VVVv20110718 |
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 |
extractor |
RequiredListDrivenProduct |
VHSv20120926 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
'NONE' |
|
extractor |
RequiredListDrivenProduct |
VHSv20130417 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
NONE |
|
extractor |
RequiredListDrivenProduct |
VIDEODR3 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
'NONE' |
|
extractor |
RequiredListDrivenProduct |
VIKINGDR3 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
'NONE' |
|
extractor |
RequiredListDrivenProduct |
VIKINGv20130417 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
NONE |
|
extractor |
RequiredListDrivenProduct |
VMCv20121128 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
'NONE' |
|
extractor |
RequiredListDrivenProduct |
VMCv20130304 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
'NONE' |
|
extractor |
RequiredListDrivenProduct |
VMCv20130805 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
NONE |
|
extractor |
RequiredListDrivenProduct |
VVVDR1 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
'NONE' |
|
extractor |
RequiredMatchedApertureProduct |
SHARKSv20210222 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
SHARKSv20210421 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
ULTRAVISTADR4 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VHSv20201209 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VHSv20231101 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VHSv20240731 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VMCDEEPv20230713 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VMCDEEPv20240506 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VMCDR5 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VMCv20191212 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VMCv20210708 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VMCv20230816 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VMCv20240226 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VVVDR5 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMatchedApertureProduct |
VVVXDR1 |
CASU list driven or SExtractor dual image mode |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
SHARKSv20210222 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
SHARKSv20210421 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
ULTRAVISTADR4 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VHSv20201209 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VHSv20231101 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VHSv20240731 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VMCDEEPv20230713 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VMCDEEPv20240506 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VMCDR5 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VMCv20191212 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VMCv20210708 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VMCv20230816 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VMCv20240226 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VVVDR5 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractor |
RequiredMosaicTopLevel |
VVVXDR1 |
Extraction software (e.g. SExtractor) |
varchar |
16 |
|
|
|
extractParamTemp |
RequiredMosaicTopLevel |
SHARKSv20210222 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
SHARKSv20210421 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
ULTRAVISTADR4 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VHSv20201209 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VHSv20231101 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VHSv20240731 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VMCDEEPv20230713 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VMCDEEPv20240506 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VMCDR5 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VMCv20191212 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VMCv20210708 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VMCv20230816 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VMCv20240226 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VVVDR5 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractParamTemp |
RequiredMosaicTopLevel |
VVVXDR1 |
Template file for SWARP parameters |
varchar |
32 |
|
NONE |
|
extractTool |
Programme |
SHARKSv20210222 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
SHARKSv20210421 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
ULTRAVISTADR4 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSDR1 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSDR2 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSDR3 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSDR4 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSDR5 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSDR6 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSv20120926 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSv20130417 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSv20150108 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSv20160114 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSv20160507 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSv20170630 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSv20180419 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSv20201209 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSv20231101 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VHSv20240731 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIDEODR2 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIDEODR3 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIDEODR4 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIDEODR5 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIDEOv20100513 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIDEOv20111208 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGDR2 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGDR3 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGDR4 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGv20110714 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGv20111019 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGv20130417 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGv20150421 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGv20151230 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGv20160406 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGv20161202 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VIKINGv20170715 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCDEEPv20230713 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCDEEPv20240506 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCDR1 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCDR3 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCDR4 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCDR5 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20110816 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20110909 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20120126 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20121128 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20130304 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20130805 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20140428 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20140903 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20150309 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20151218 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20160311 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20160822 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20170109 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20170411 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20171101 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20180702 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20181120 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20191212 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20210708 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20230816 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VMCv20240226 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VSAQC |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VVVDR1 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VVVDR2 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VVVDR5 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VVVXDR1 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VVVv20100531 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extractTool |
Programme |
VVVv20110718 |
Name of extraction tool to be used |
varchar |
8 |
|
NONE |
?? |
extTableID |
ExternalSurveyTable |
SHARKSv20210421 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
ULTRAVISTADR4 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSDR1 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSDR2 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSDR3 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSDR4 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSDR5 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSDR6 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSv20120926 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSv20130417 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSv20150108 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSv20160114 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSv20160507 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSv20170630 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSv20180419 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSv20201209 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSv20231101 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VHSv20240731 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIDEODR2 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIDEODR3 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIDEODR4 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIDEODR5 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIDEOv20100513 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIDEOv20111208 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGDR2 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGDR3 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGDR4 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGv20110714 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGv20111019 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGv20130417 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGv20150421 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGv20151230 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGv20160406 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGv20161202 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VIKINGv20170715 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCDEEPv20230713 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCDEEPv20240506 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCDR1 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCDR3 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCDR4 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCDR5 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20110816 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20110909 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20120126 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20121128 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20130304 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20130805 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20140428 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20140903 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20150309 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20151218 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20160311 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20160822 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20170109 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20170411 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20171101 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20180702 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20181120 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20191212 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20210708 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20230816 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VMCv20240226 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VSAQC |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VVVDR1 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VVVDR2 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VVVDR5 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VVVXDR1 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VVVv20100531 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable |
VVVv20110718 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableID |
ExternalSurveyTable, RequiredNeighbours |
SHARKSv20210222 |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
extTableName |
ExternalSurveyTable |
SHARKSv20210222 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
SHARKSv20210421 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
ULTRAVISTADR4 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSDR1 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSDR2 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSDR3 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSDR4 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSDR5 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSDR6 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSv20120926 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSv20130417 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSv20150108 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSv20160114 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSv20160507 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSv20170630 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSv20180419 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSv20201209 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSv20231101 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VHSv20240731 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIDEODR2 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIDEODR3 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIDEODR4 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIDEODR5 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIDEOv20100513 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIDEOv20111208 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGDR2 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGDR3 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGDR4 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGv20110714 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGv20111019 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGv20130417 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGv20150421 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGv20151230 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGv20160406 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGv20161202 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VIKINGv20170715 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCDEEPv20230713 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCDEEPv20240506 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCDR1 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCDR3 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCDR4 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCDR5 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20110816 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20110909 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20120126 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20121128 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20130304 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20130805 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20140428 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20140903 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20150309 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20151218 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20160311 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20160822 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20170109 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20170411 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20171101 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20180702 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20181120 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20191212 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20210708 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20230816 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VMCv20240226 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VSAQC |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VVVDR1 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VVVDR2 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VVVDR5 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VVVXDR1 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VVVv20100531 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
extTableName |
ExternalSurveyTable |
VVVv20110718 |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |
eYmag |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Error on VVV DR4 Y photometry. {catalogue TType keyword: eYmag} |
real |
4 |
mag |
-999999500.0 |
|
eZmag |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Error on VVV DR4 Z photometry. {catalogue TType keyword: eZmag} |
real |
4 |
mag |
-999999500.0 |
|