V |
| Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
| var_flg |
allwise_sc |
WISE |
Variability flag. The variability flag is a four-character string, one character per band, in which the value for each band is related to the probability that the source flux measured on the individual WISE exposures was not constant with time. The probability calculation uses the standard deviation of the single exposure flux measurements, w?sigp1, as well as the band-to-band flux correlation significance, q12,q23,q34. CAUTION: Estimation of flux variability is unreliable for sources that are extended (ext_flg>0), and sources whose measurements are contaminated by image artifacts in a band (cc_flags[b] != '0'). |
varchar |
4 |
|
|
|
| The probability is computed for a band only when there are at least six single-exposure measurements available that satisfy minimum quality criteria. A value of "n" in a band indicates insufficient or inadequate data to make a determination of possible variability. Values of "0" through "9" indicate increasing probabilities of variation. Values of "0" through "5" are most likely not variables. Sources with values of "6" and "7" are likely flux variables, but are the most susceptible to false-positive variability. Var_flg values greater than "7" have the highest probability of being true flux variables in a band. |
| var_flg |
wise_allskysc |
WISE |
Variability flag. The variability flag is a four-character string, one character per band, in which the value for each band is related to the probability that the source flux measured on the individual WISE exposures was not constant with time. |
char |
4 |
|
NONE |
|
| var_flg |
wise_prelimsc |
WISE |
Variability flag The variability flag is a four-character string, one character per band, in which the value for each band is related to the probability that the source flux measured on the individual WISE exposures was not constant with time |
char |
4 |
|
NONE |
|
| vbroad |
gaia_source |
GAIADR3 |
Spectral line broadening parameter |
real |
4 |
km/s |
|
spect.dopplerVeloc.opt;em.opt.I |
| vbroad_error |
gaia_source |
GAIADR3 |
Uncertainty on the spectral line broadening |
real |
4 |
km/s |
|
stat.error;spect.dopplerVeloc.opt;em.opt.I |
| vbroad_nb_transits |
gaia_source |
GAIADR3 |
Number of transits used to compute vbroad |
smallint |
2 |
|
|
meta.number |
| vc |
twomass_sixx2_xsc |
TWOMASS |
visual verification score for source |
smallint |
2 |
|
|
|
| vc |
twomass_xsc |
TWOMASS |
visual verification score for source. |
smallint |
2 |
|
|
meta.code |
| vegaToAB |
Filter |
VULCANiDR |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
| visibility_periods_used |
gaia_source |
GAIADR3 |
Number of visibility periods uased in the astrometric solution |
smallint |
2 |
|
|
meta.number |
| vr_m_opt |
twomass_psc |
TWOMASS |
Visual or red magnitude of the associated optical source. |
real |
4 |
mag |
|
phot.flux |