V |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
var |
iras_psc |
IRAS |
percent Likelihood of Variability |
smallint |
2 |
|
|
CODE_VARIAB |
VAR_EXP_ID |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
XMM |
If the source is detected as variable (that is, if VAR_FLAG is set to True), the exposure ID ('S' or 'U' followed by a three-digit number) of the exposure with the smallest Chi² probability is given here. |
varchar |
4 |
|
|
|
VAR_FLAG |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
XMM |
The flag is set to True if this source was detected as variable (Chi² probability < 1E-5, see PN_CHI2PROB, M1_CHI2PROB, M2_CHI2PROB) in at least one exposure. |
varchar |
5 |
|
|
|
var_flag |
combo17CDFSSource |
COMBO17 |
variability flag (0=not variable); flag only set for objects which are detected with high S/N and which show clear variability between different observing runs (magnitude difference greater 0.15 mag, at least one magnitude has to be measured with 10 sigma, difference has to be at least 6 sigma |
tinyint |
1 |
|
|
|
VAR_INST_ID |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
XMM |
If the source is detected as variable (that is, if VAR_FLAG is set to True), the instrument ID (PN, M1, M2) of the exposure given in VAR_EXP_ID is listed here. |
varchar |
2 |
|
|
|
variabilityTable |
Programme |
VSAQC |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
variabilityTable |
Programme |
VSASVNGC253 |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
variabilityTable |
Programme |
VSASVORION |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
variabilityTable |
Programme |
VSAUltraVISTA |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
variabilityTable |
Programme |
VSAVHS |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
variabilityTable |
Programme |
VSAVIDEO |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
variabilityTable |
Programme |
VSAVIKING |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
variabilityTable |
Programme |
VSAVMC |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
variabilityTable |
Programme |
VSAVVV |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
variableClass |
ultravistaVariability |
VSAUltraVISTA |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
|
This gives an overall classification. Currently the weighted intrinsicRMS/expectedRMS (wsrms) is calculated across all bands, where the weighting is directly proportional to the number of good observations in each band, where any bands with <5 observations have w=0 and the band with the most observations has a weighting of 1. If wsrms>3, then variableClass=1 (i.e. the source is variable), else variableClass=0. In the future, the classification will take into account other statistics, such as correlations between bands and will also include motion and skew, and will not be limited to 0 or 1. |
variableClass |
ultravistaVariability, videoVariability, vikingVariability, vmcVariability, vvvVariability |
VSAQC |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
|
This gives an overall classification. Currently the weighted intrinsicRMS/expectedRMS (wsrms) is calculated across all bands, where the weighting is directly proportional to the number of good observations in each band, where any bands with <5 observations have w=0 and the band with the most observations has a weighting of 1. If wsrms>3, then variableClass=1 (i.e. the source is variable), else variableClass=0. In the future, the classification will take into account other statistics, such as correlations between bands and will also include motion and skew, and will not be limited to 0 or 1. |
VbMag |
combo17CDFSSource |
COMBO17 |
Absolute restframe magnitude in Bessell V (calculated from redshifted best_fit template, depending on redshift and filter extrapolation outside the COMBO-17 filter set can be necessary, only calculated for objects classified as galaxies) |
real |
4 |
mag |
|
|
vc |
twomass_sixx2_xsc |
2MASS |
visual verification score for source |
smallint |
2 |
|
|
|
vc |
twomass_xsc |
2MASS |
visual verification score for source. |
smallint |
2 |
|
|
CODE_MISC |
vegaToAB |
Filter |
VSAQC |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VSASVNGC253 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VSASVORION |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VSAUltraVISTA |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VSAVHS |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VSAVIDEO |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VSAVIKING |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VSAVMC |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VSAVVV |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
versionDate |
sage_lmcIracSource, sage_lmcMips160Source, sage_lmcMips24Source, sage_lmcMips70Source |
SPITZER |
Date catalogue was produced in the following format, "mon dd yyyy", "Dec 5 2007" |
varchar |
12 |
|
|
|
versionNo |
sage_lmcIracSource, sage_lmcMips160Source, sage_lmcMips24Source, sage_lmcMips70Source |
SPITZER |
Version number assigned by MIPS/IRAC pipeline team |
real |
4 |
|
|
|
versionNum |
Multiframe |
VSASVNGC253 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
VERSNUM |
For deep stacks and mosaics produced in Edinburgh, (frameType=deep%stack, fileName=eYYYYMMDD_%) this refers to the database release number. For all other files, the versNum refers to the CASU pipeline version number. |
versionNum |
Multiframe |
VSASVORION |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
VERSNUM |
For deep stacks and mosaics produced in Edinburgh, (frameType=deep%stack, fileName=eYYYYMMDD_%) this refers to the database release number. For all other files, the versNum refers to the CASU pipeline version number. |
versionNum |
Multiframe |
VSAUltraVISTA |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
VERSNUM |
For deep stacks and mosaics produced in Edinburgh, (frameType=deep%stack, fileName=eYYYYMMDD_%) this refers to the database release number. For all other files, the versNum refers to the CASU pipeline version number. |
versionNum |
Multiframe |
VSAVHS |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
VERSNUM |
For deep stacks and mosaics produced in Edinburgh, (frameType=deep%stack, fileName=eYYYYMMDD_%) this refers to the database release number. For all other files, the versNum refers to the CASU pipeline version number. |
versionNum |
Multiframe |
VSAVIDEO |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
VERSNUM |
For deep stacks and mosaics produced in Edinburgh, (frameType=deep%stack, fileName=eYYYYMMDD_%) this refers to the database release number. For all other files, the versNum refers to the CASU pipeline version number. |
versionNum |
Multiframe |
VSAVIKING |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
VERSNUM |
For deep stacks and mosaics produced in Edinburgh, (frameType=deep%stack, fileName=eYYYYMMDD_%) this refers to the database release number. For all other files, the versNum refers to the CASU pipeline version number. |
versionNum |
Multiframe |
VSAVMC |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
VERSNUM |
For deep stacks and mosaics produced in Edinburgh, (frameType=deep%stack, fileName=eYYYYMMDD_%) this refers to the database release number. For all other files, the versNum refers to the CASU pipeline version number. |
versionNum |
Multiframe |
VSAVVV |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
VERSNUM |
For deep stacks and mosaics produced in Edinburgh, (frameType=deep%stack, fileName=eYYYYMMDD_%) this refers to the database release number. For all other files, the versNum refers to the CASU pipeline version number. |
versionNum |
ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
VERSNUM |
versNum |
AstrCalVers |
VSASVNGC253 |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
versNum |
AstrCalVers |
VSASVORION |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
versNum |
AstrCalVers |
VSAUltraVISTA |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
versNum |
AstrCalVers |
VSAVHS |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
versNum |
AstrCalVers |
VSAVIDEO |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
versNum |
AstrCalVers |
VSAVIKING |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
versNum |
AstrCalVers |
VSAVMC |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
versNum |
AstrCalVers |
VSAVVV |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
versNum |
PhotCalVers |
VSASVORION |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
versNum |
PhotCalVers |
VSAUltraVISTA |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
versNum |
PhotCalVers |
VSAVHS |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
versNum |
PhotCalVers |
VSAVIDEO |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
versNum |
PhotCalVers |
VSAVIKING |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
versNum |
PhotCalVers |
VSAVMC |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
versNum |
PhotCalVers |
VSAVVV |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
versNum |
PhotCalVers, PreviousMFDZP |
VSASVNGC253 |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
VF_D |
combo17CDFSSource |
COMBO17 |
flux in filter V in run D (07.10.-22.10.1999) |
float |
8 |
|
|
|
vFlag |
rosat_bsc, rosat_fsc |
ROSAT |
variability flag |
varchar |
1 |
|
|
CODE_MISC |
vigF |
rosat_fsc |
ROSAT |
vignetting factor |
float |
8 |
|
|
INST_CORR-FACTOR |
vigf |
rosat_bsc |
ROSAT |
vignetting factor |
float |
8 |
|
|
INST_CORR-FACTOR |
vistaRunNo |
Multiframe |
VSASVNGC253 |
Original VISTA run number (from filename) |
int |
4 |
|
|
REFER_CODE |
vistaRunNo |
Multiframe |
VSASVORION |
Original VISTA run number (from filename) |
int |
4 |
|
|
REFER_CODE |
vistaRunNo |
Multiframe |
VSAUltraVISTA |
Original VISTA run number (from filename) |
int |
4 |
|
|
REFER_CODE |
vistaRunNo |
Multiframe |
VSAVHS |
Original VISTA run number (from filename) |
int |
4 |
|
|
REFER_CODE |
vistaRunNo |
Multiframe |
VSAVIDEO |
Original VISTA run number (from filename) |
int |
4 |
|
|
REFER_CODE |
vistaRunNo |
Multiframe |
VSAVIKING |
Original VISTA run number (from filename) |
int |
4 |
|
|
REFER_CODE |
vistaRunNo |
Multiframe |
VSAVMC |
Original VISTA run number (from filename) |
int |
4 |
|
|
REFER_CODE |
vistaRunNo |
Multiframe |
VSAVVV |
Original VISTA run number (from filename) |
int |
4 |
|
|
REFER_CODE |
vistaRunNo |
ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Original VISTA run number (from filename) |
int |
4 |
|
|
REFER_CODE |
VjMag |
combo17CDFSSource |
COMBO17 |
Absolute restframe magnitude in Johnson V (calculated from redshifted best_fit template, depending on redshift and filter extrapolation outside the COMBO-17 filter set can be necessary, only calculated for objects classified as galaxies) |
real |
4 |
mag |
|
|
Vmag |
mcps_lmcSource, mcps_smcSource |
MCPS |
The V band magnitude |
real |
4 |
mag |
|
|
vMag |
ukirtFSstars |
VSASVNGC253 |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
PHOT_INT-MAG |
vMag |
ukirtFSstars |
VSASVORION |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
PHOT_INT-MAG |
vMag |
ukirtFSstars |
VSAUltraVISTA |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
PHOT_INT-MAG |
vMag |
ukirtFSstars |
VSAVHS |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
PHOT_INT-MAG |
vMag |
ukirtFSstars |
VSAVIDEO |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
PHOT_INT-MAG |
vMag |
ukirtFSstars |
VSAVIKING |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
PHOT_INT-MAG |
vMag |
ukirtFSstars |
VSAVMC |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
PHOT_INT-MAG |
vMag |
ukirtFSstars |
VSAVVV |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
PHOT_INT-MAG |
VmagOGLEII |
spitzer_smcSource |
SPITZER |
The OGLEII V band magnitude. |
real |
4 |
mag |
|
|
vr_m_opt |
twomass_psc |
2MASS |
Visual or red magnitude of the associated optical source. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |