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 |
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 |
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_INST_ID |
twoxmm |
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 |
WSA |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
| variabilityTable |
Programme |
WSACalib |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
| variabilityTable |
Programme |
WSATransit |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
| variableClass |
dxsVariability, udsVariability |
WSA |
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. |
| vc |
twomass_xsc |
2MASS |
visual verification score for source. |
smallint |
2 |
|
|
CODE_MISC |
| vegaToAB |
Filter |
WSA |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
| vegaToAB |
Filter |
WSACalib |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
| vegaToAB |
Filter |
WSATransit |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
| versionNum |
Multiframe |
WSA |
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 |
WSACalib |
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 |
WSATransit |
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. |
| versNum |
AstrCalVers |
WSACalib |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
| versNum |
AstrCalVers |
WSATransit |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
| versNum |
AstrCalVers, PreviousAstrometry |
WSA |
Version number of current astrometric solution |
int |
4 |
|
|
ID_VERSION |
| versNum |
PhotCalVers |
WSACalib |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
| versNum |
PhotCalVers |
WSATransit |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
| versNum |
PhotCalVers, PreviousMFDZP |
WSA |
the version number of the calibration |
int |
4 |
|
|
ID_VERSION |
| 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 |
| vMag |
ukirtFSstars |
WSA |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
PHOT_INT-MAG |
| vMag |
ukirtFSstars |
WSACalib |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
PHOT_INT-MAG |
| vr_m_opt |
twomass_psc |
2MASS |
Visual or red magnitude of the associated optical source. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |