V |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
v_flags |
masterDR2 |
SKYMAPPER |
Bitwise OR of Source Extractor flags from v-band measurements in photometry table |
smallint |
2 |
|
|
meta.code |
v_i |
hipparcos_new_reduction |
GAIADR1 |
V-I colour index |
float |
8 |
mag |
|
phot.color;em.opt.V;em.opt.I |
v_nch |
masterDR2 |
SKYMAPPER |
Number of v-band child sources combined into this object_id |
smallint |
2 |
|
|
meta.number |
v_nclip |
masterDR2 |
SKYMAPPER |
Number of v-band observations with magnitudes clipped from the final PSF magnitude estimate |
smallint |
2 |
|
|
meta.number |
v_ngood |
masterDR2 |
SKYMAPPER |
Number of v-band observations used |
smallint |
2 |
|
|
meta.number |
v_nimaflags |
masterDR2 |
SKYMAPPER |
Number of flagged pixels from bad, saturated, and crosstalk pixel masks from v-band measurements in photometry table |
int |
4 |
|
|
meta.code |
v_petro |
masterDR2 |
SKYMAPPER |
Mean v-band Petrosian magnitude |
real |
4 |
mag |
|
phot.mag;stat.mean |
v_psf |
masterDR2 |
SKYMAPPER |
Mean v-band PSF magnitude |
real |
4 |
mag |
|
phot.mag;stat.mean |
v_rchi2var |
masterDR2 |
SKYMAPPER |
Reduced chi-squared for a constant-magnitude model of the v-band PSF magnitude, including clipped sources |
real |
4 |
|
|
stat.fit.chi2 |
va |
hipparcos_new_reduction |
GAIADR1 |
Reference to variability annex |
int |
4 |
|
|
meta.note |
value |
SExtractorInputParams |
SHARKSv20210222 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
SHARKSv20210421 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
ULTRAVISTADR4 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VHSv20201209 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VHSv20231101 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VHSv20240731 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VMCDEEPv20230713 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VMCDEEPv20240506 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VMCDR5 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VMCv20191212 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VMCv20210708 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VMCv20230816 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VMCv20240226 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VVVDR5 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
value |
SExtractorInputParams |
VVVXDR1 |
Value of the input parameter |
varchar |
1024 |
|
NONE |
|
Var |
eros2LMCSource, eros2SMCSource, erosLMCSource, erosSMCSource |
EROS |
Variability flag: 1 if potentially variable star |
int |
4 |
|
|
|
var |
hipparcos_new_reduction |
GAIADR1 |
Cosmic dispersion added (stochastc solution) |
float |
8 |
|
|
stat.fit.residual |
var |
iras_psc |
IRAS |
percent Likelihood of Variability |
smallint |
2 |
|
|
meta.code;src.var |
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_EXP_ID |
xmm3dr4 |
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 |
50 |
|
|
|
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 |
xmm3dr4 |
XMM |
The flag is set to 1 if this source was detected as variable (Chi² probability < 1E-5, see PN_CHI2PROB, M1_CHI2PROB, M2_CHI2PROB) in at least one exposure. |
bit |
1 |
|
|
|
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_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 |
|
var_flg_ALLWISE |
ravedr5Source |
RAVE |
probability that flux varied in any band greater than amount expected from unc.s |
varchar |
5 |
|
|
meta.code |
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 |
|
|
|
VAR_INST_ID |
xmm3dr4 |
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 |
50 |
|
|
|
variabilityTable |
Programme |
SHARKSv20210222 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
SHARKSv20210421 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
ULTRAVISTADR4 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSDR1 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSDR2 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSDR3 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSDR4 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSDR5 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSDR6 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSv20120926 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSv20130417 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSv20150108 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSv20160114 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSv20160507 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSv20170630 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSv20180419 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSv20201209 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSv20231101 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VHSv20240731 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIDEODR2 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIDEODR3 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIDEODR4 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIDEODR5 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIDEOv20100513 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIDEOv20111208 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGDR2 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGDR3 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGDR4 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGv20110714 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGv20111019 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGv20130417 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGv20150421 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGv20151230 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGv20160406 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGv20161202 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VIKINGv20170715 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCDEEPv20230713 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCDEEPv20240506 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCDR1 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCDR3 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCDR4 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCDR5 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20110816 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20110909 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20120126 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20121128 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20130304 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20130805 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20140428 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20140903 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20150309 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20151218 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20160311 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20160822 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20170109 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20170411 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20171101 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20180702 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20181120 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20191212 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20210708 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20230816 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VMCv20240226 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VSAQC |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VVVDR1 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VVVDR2 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VVVDR5 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VVVXDR1 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VVVv20100531 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variabilityTable |
Programme |
VVVv20110718 |
Table name of merged variable sources |
varchar |
64 |
|
'NONE' |
?? |
variableClass |
sharksVariability |
SHARKSv20210222 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
sharksVariability |
SHARKSv20210421 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
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 |
ULTRAVISTADR4 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
videoVariability |
VIDEODR2 |
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 |
videoVariability |
VIDEODR3 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
videoVariability |
VIDEODR4 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
videoVariability |
VIDEODR5 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
videoVariability |
VIDEOv20100513 |
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 |
videoVariability |
VIDEOv20111208 |
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 |
vikingVariability |
VIKINGDR2 |
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 |
vikingVariability |
VIKINGDR3 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vikingVariability |
VIKINGDR4 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vikingVariability |
VIKINGv20110714 |
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 |
vikingVariability |
VIKINGv20111019 |
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 |
vikingVariability |
VIKINGv20130417 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vikingVariability |
VIKINGv20140402 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vikingVariability |
VIKINGv20150421 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vikingVariability |
VIKINGv20151230 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vikingVariability |
VIKINGv20160406 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vikingVariability |
VIKINGv20161202 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vikingVariability |
VIKINGv20170715 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCDR1 |
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 |
vmcVariability |
VMCDR2 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCDR3 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCDR4 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCDR5 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20110816 |
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 |
vmcVariability |
VMCv20110909 |
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 |
vmcVariability |
VMCv20120126 |
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 |
vmcVariability |
VMCv20121128 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20130304 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20130805 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20140428 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20140903 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20150309 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20151218 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20160311 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20160822 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20170109 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20170411 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20171101 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20180702 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20181120 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20191212 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20210708 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20230816 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcVariability |
VMCv20240226 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcdeepVariability |
VMCDEEPv20230713 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vmcdeepVariability |
VMCDEEPv20240506 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vvvVariability |
VVVDR1 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vvvVariability |
VVVDR2 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vvvVariability |
VVVDR5 |
Classification of objects across all bands. |
int |
4 |
|
-99999999 |
meta.code.class |
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 |
vvvVariability |
VVVv20100531 |
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 |
vvvVariability |
VVVv20110718 |
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. |
variableType |
vmcVariablesType |
VMCDR3 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCDR4 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20121128 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20140428 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20140903 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20150309 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20151218 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20160311 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20160822 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20170109 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20170411 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20171101 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20180702 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20181120 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20191212 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20210708 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20230816 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
variableType |
vmcVariablesType |
VMCv20240226 |
Type of variable as defined by VMC team |
varchar |
32 |
|
|
meta.code.class;src.var |
varID |
vmcCepheidVariables |
VMCv20121128 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20140428 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20140903 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20150309 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20151218 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20160311 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20160822 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20170109 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20170411 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20171101 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20180702 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20181120 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20191212 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20210708 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20230816 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables |
VMCv20240226 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables, vmcEclipsingBinaryVariables, vmcRRlyraeVariables |
VMCDR4 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcCepheidVariables, vmcVariablesType |
VMCDR3 |
UID of VMC variables |
bigint |
8 |
|
|
meta.id;meta.main |
varID |
vmcRRLyraeVariables |
VMCv20240226 |
UID of VMC Variables |
bigint |
8 |
|
|
meta.id;meta.main |
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 |
TWOMASS |
visual verification score for source |
smallint |
2 |
|
|
|
vc |
twomass_xsc |
TWOMASS |
visual verification score for source. |
smallint |
2 |
|
|
meta.code |
vegaToAB |
Filter |
SHARKSv20210421 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
ULTRAVISTADR4 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSDR1 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSDR2 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSDR3 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSDR4 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSDR5 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSDR6 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSv20120926 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSv20130417 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSv20150108 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSv20160114 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSv20160507 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSv20170630 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSv20180419 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSv20201209 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSv20231101 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VHSv20240731 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIDEODR2 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIDEODR3 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIDEODR4 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIDEODR5 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIDEOv20100513 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIDEOv20111208 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGDR2 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGDR3 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGDR4 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGv20110714 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGv20111019 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGv20130417 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGv20150421 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGv20151230 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGv20160406 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGv20161202 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VIKINGv20170715 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCDEEPv20230713 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCDEEPv20240506 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCDR1 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCDR3 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCDR4 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCDR5 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20110816 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20110909 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20120126 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20121128 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20130304 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20130805 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20140428 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20140903 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20150309 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20151218 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20160311 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20160822 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20170109 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20170411 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20171101 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20180702 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20181120 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20191212 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20210708 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20230816 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VMCv20240226 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VSAQC |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VVVDR1 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VVVDR2 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VVVDR5 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VVVXDR1 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VVVv20100531 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter |
VVVv20110718 |
The constant to convert Vega magnitudes to AB magnitudes. |
real |
4 |
mag |
-0.9999995e9 |
|
vegaToAB |
Filter, FilterSections |
SHARKSv20210222 |
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 |
|
|
|
versionDate |
sage_smcIRACv1_5Source |
SPITZER |
Date catalog was produced in the following format, "mon dd yyyy", "Dec 5 2007" |
varchar |
12 |
|
|
|
versionNo |
sage_lmcIracSource, sage_lmcMips160Source, sage_lmcMips24Source, sage_lmcMips70Source, sage_smcIRACv1_5Source |
SPITZER |
Version number assigned by MIPS/IRAC pipeline team |
real |
4 |
|
|
|
versionNum |
MapFrameStatus |
SHARKSv20210222 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
SHARKSv20210421 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
ULTRAVISTADR4 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VHSv20201209 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VHSv20231101 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VHSv20240731 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VMCDEEPv20230713 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VMCDEEPv20240506 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VMCDR5 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VMCv20191212 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VMCv20210708 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VMCv20230816 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VMCv20240226 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VVVDR5 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
MapFrameStatus |
VVVXDR1 |
Version number of the catalogue |
smallint |
2 |
|
-9999 |
|
versionNum |
Multiframe |
SHARKSv20210222 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
SHARKSv20210421 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
ULTRAVISTADR4 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSDR1 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VHSDR2 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VHSDR3 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VHSDR4 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSDR5 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSDR6 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSv20120926 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VHSv20130417 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VHSv20140409 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VHSv20150108 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSv20160114 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSv20160507 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSv20170630 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSv20180419 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSv20201209 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSv20231101 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VHSv20240731 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VIDEODR2 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIDEODR3 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIDEODR4 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VIDEODR5 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VIDEOv20100513 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIDEOv20111208 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIKINGDR2 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIKINGDR3 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIKINGDR4 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIKINGv20110714 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIKINGv20111019 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIKINGv20130417 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIKINGv20140402 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VIKINGv20150421 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VIKINGv20151230 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VIKINGv20160406 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VIKINGv20161202 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VIKINGv20170715 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCDEEPv20230713 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCDEEPv20240506 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCDR1 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCDR2 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCDR3 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCDR4 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCDR5 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20110816 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCv20110909 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCv20120126 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCv20121128 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCv20130304 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCv20130805 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCv20140428 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCv20140903 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VMCv20150309 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20151218 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20160311 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20160822 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20170109 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20170411 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20171101 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20180702 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20181120 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20191212 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20210708 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20230816 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VMCv20240226 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VVVDR1 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VVVDR2 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VVVDR5 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VVVXDR1 |
a version number for this frame (if available) |
varchar |
8 |
|
NONE |
meta.id |
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 |
VVVv20100531 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
VVVv20110718 |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
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 |
PreviousCalibParams |
SHARKSv20210222 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
SHARKSv20210421 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
VHSv20201209 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
VHSv20231101 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
VHSv20240731 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
VMCDEEPv20230713 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
VMCDEEPv20240506 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
VMCv20210708 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
VMCv20230816 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
VMCv20240226 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
VVVDR5 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
PreviousCalibParams |
VVVXDR1 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versionNum |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
a version number for this frame (if available) |
real |
4 |
|
-0.9999995e9 |
meta.id |
versionNum |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Version number of the catalogue |
smallint |
2 |
|
|
|
versionNum |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
Version number of the catalogue {catalogue extension keyword: VERSNUM} |
smallint |
2 |
|
-9999 |
|
versionNum |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Version number of the catalogue |
smallint |
2 |
|
|
|
versionNum |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Version number of the catalogue |
smallint |
2 |
|
|
|
versionNum |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Version number of the catalogue {catalogue extension keyword: VERSNUM} |
smallint |
2 |
|
-9999 |
|
versionNum |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Version number of the catalogue {catalogue extension keyword: VERSNUM} |
smallint |
2 |
|
-9999 |
|
versNum |
AstrCalVers |
SHARKSv20210222 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
SHARKSv20210421 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
ULTRAVISTADR4 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSDR1 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSDR2 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSDR3 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSDR4 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSDR5 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSDR6 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSv20120926 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSv20130417 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSv20150108 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSv20160114 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSv20160507 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSv20170630 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSv20180419 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSv20201209 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSv20231101 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VHSv20240731 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIDEODR2 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIDEODR3 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIDEODR4 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIDEODR5 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIDEOv20100513 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIDEOv20111208 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGDR2 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGDR3 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGDR4 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGv20110714 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGv20111019 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGv20130417 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGv20150421 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGv20151230 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGv20160406 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGv20161202 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VIKINGv20170715 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCDEEPv20230713 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCDEEPv20240506 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCDR1 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCDR3 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCDR4 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCDR5 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20110816 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20110909 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20120126 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20121128 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20130304 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20130805 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20140428 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20140903 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20150309 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20151218 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20160311 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20160822 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20170109 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20170411 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20171101 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20180702 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20181120 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20191212 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20210708 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20230816 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VMCv20240226 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VVVDR1 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VVVDR2 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VVVDR5 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VVVXDR1 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VVVv20100531 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
AstrCalVers |
VVVv20110718 |
Version number of current astrometric solution |
int |
4 |
|
|
meta.software |
versNum |
ExternalProductCatalogue |
SHARKSv20210222 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
SHARKSv20210421 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
ULTRAVISTADR4 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSDR3 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSDR4 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSDR5 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSDR6 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSv20150108 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSv20160114 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSv20160507 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSv20170630 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSv20180419 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSv20201209 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSv20231101 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VHSv20240731 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VIDEODR4 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VIDEODR5 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VIKINGDR4 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VIKINGv20150421 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VIKINGv20151230 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VIKINGv20160406 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VIKINGv20161202 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VIKINGv20170715 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCDEEPv20230713 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCDEEPv20240506 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCDR3 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCDR4 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCDR5 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20140428 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20140903 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20150309 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20151218 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20160311 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20160822 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20170109 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20170411 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20171101 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20180702 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20181120 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20191212 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20210708 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20230816 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VMCv20240226 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VVVDR5 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
ExternalProductCatalogue |
VVVXDR1 |
Version of file sent from survey team |
int |
4 |
|
|
|
versNum |
PhotCalVers |
SHARKSv20210421 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
ULTRAVISTADR4 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSDR1 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSDR2 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSDR3 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSDR4 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSDR5 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSDR6 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSv20120926 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSv20130417 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSv20150108 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSv20160114 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSv20160507 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSv20170630 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSv20180419 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSv20201209 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSv20231101 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VHSv20240731 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIDEODR2 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIDEODR3 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIDEODR4 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIDEODR5 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIDEOv20100513 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIDEOv20111208 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGDR2 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGDR3 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGDR4 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGv20110714 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGv20111019 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGv20130417 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGv20150421 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGv20151230 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGv20160406 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGv20161202 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VIKINGv20170715 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCDEEPv20230713 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCDEEPv20240506 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCDR1 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCDR3 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCDR4 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCDR5 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20110816 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20110909 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20120126 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20121128 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20130304 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20130805 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20140428 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20140903 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20150309 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20151218 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20160311 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20160822 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20170109 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20170411 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20171101 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20180702 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20181120 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20191212 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20210708 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20230816 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VMCv20240226 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VVVDR1 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VVVDR2 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VVVDR5 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VVVXDR1 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VVVv20100531 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers |
VVVv20110718 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
versNum |
PhotCalVers, PreviousMFDZP |
SHARKSv20210222 |
the version number of the calibration |
int |
4 |
|
|
meta.software |
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 |
|
|
meta.code |
vigF |
rosat_fsc |
ROSAT |
vignetting factor |
float |
8 |
|
|
instr.param |
vigf |
rosat_bsc |
ROSAT |
vignetting factor |
float |
8 |
|
|
instr.param |
viracID |
vvvParallaxCatalogue |
VVVDR5 |
unique source identifier in VIRAC catalogue. {catalogue TType keyword: sourceid} |
bigint |
8 |
|
-99999999 |
meta.id;meta.main |
viracID |
vvvProperMotionCatalogue |
VVVDR5 |
unique source identifier from VIRAC catalogue. {catalogue TType keyword: sourceid} |
bigint |
8 |
|
-99999999 |
meta.id;meta.main |
visibility_periods_used |
gaia_source |
GAIADR2 |
Number of visibility periods uased in the astrometric solution |
smallint |
2 |
|
|
meta.number |
visibility_periods_used |
gaia_source |
GAIAEDR3 |
Number of visibility periods uased in the astrometric solution |
smallint |
2 |
|
|
meta.number |
vistaRunNo |
Multiframe |
SHARKSv20210222 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
SHARKSv20210421 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
ULTRAVISTADR4 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSDR1 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSDR2 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSDR3 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSDR4 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSDR5 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSDR6 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20120926 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20130417 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20140409 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20150108 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20160114 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20160507 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20170630 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20180419 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20201209 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20231101 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VHSv20240731 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIDEODR2 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIDEODR3 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIDEODR4 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIDEODR5 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIDEOv20100513 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIDEOv20111208 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGDR2 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGDR3 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGDR4 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGv20110714 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGv20111019 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGv20130417 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGv20140402 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGv20150421 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGv20151230 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGv20160406 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGv20161202 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VIKINGv20170715 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCDEEPv20230713 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCDEEPv20240506 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCDR1 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCDR2 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCDR3 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCDR4 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCDR5 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20110816 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20110909 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20120126 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20121128 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20130304 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20130805 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20140428 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20140903 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20150309 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20151218 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20160311 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20160822 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20170109 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20170411 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20171101 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20180702 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20181120 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20191212 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20210708 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20230816 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VMCv20240226 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VVVDR1 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VVVDR2 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VVVDR5 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VVVXDR1 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VVVv20100531 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
Multiframe |
VVVv20110718 |
Original VISTA run number (from filename) |
int |
4 |
|
-99999999 |
meta.bib |
vistaRunNo |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Original VISTA run number (from filename) |
int |
4 |
|
|
meta.bib |
vivaID |
vvvVivaCatalogue, vvvVivaXMatchCatalogue |
VVVDR5 |
Unique identifier for VIVA catalogue, and also VVVDR4 sourceID {catalogue TType keyword: sourceID} |
bigint |
8 |
|
-99999999 |
meta.id;meta.main |
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 |
VIDEOv20100513 |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
vMag |
ukirtFSstars |
VIKINGv20110714 |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
vMag |
ukirtFSstars |
VVVv20100531 |
V band total magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
Vmag_APASSDR9 |
ravedr5Source |
RAVE |
V magnitude from APASSDR9 |
real |
4 |
mag |
|
phot.mag;em.opt.V |
VmagOGLEII |
spitzer_smcSource |
SPITZER |
The OGLEII V band magnitude. |
real |
4 |
mag |
|
|
vmcID |
vmcRRLyraeLightCurves |
VMCv20240226 |
UID of VMC variables {catalogue TType keyword: vmcID} |
bigint |
8 |
|
|
meta.id;meta.main |
vmcID |
vmcRRLyraeVariables |
VMCv20240226 |
UID: VMC source ID from release VMCv20181120 {catalogue TType keyword: rel_id} |
bigint |
8 |
|
|
meta.id |
vmcMlID |
vmcMLClassificationCatalogue |
VMCv20240226 |
UID of star in the proper motion catalogue |
bigint |
8 |
|
|
meta.id;meta.main |
vMeanMag |
vmcCepheidVariables |
VMCDR3 |
Mean V band magnitude {catalogue TType keyword: V} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcCepheidVariables |
VMCDR4 |
Mean V band magnitude {catalogue TType keyword: Vmag} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcCepheidVariables |
VMCv20121128 |
Mean V band magnitude {catalogue TType keyword: V} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcCepheidVariables |
VMCv20140428 |
Mean V band magnitude {catalogue TType keyword: V} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcCepheidVariables |
VMCv20140903 |
Mean V band magnitude {catalogue TType keyword: V} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcCepheidVariables |
VMCv20150309 |
Mean V band magnitude {catalogue TType keyword: V} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcCepheidVariables |
VMCv20151218 |
Mean V band magnitude {catalogue TType keyword: V} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcCepheidVariables |
VMCv20160311 |
Mean V band magnitude {catalogue TType keyword: Vmag} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcCepheidVariables |
VMCv20160822 |
Mean V band magnitude {catalogue TType keyword: Vmag} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcRRlyraeVariables |
VMCDR4 |
Mean V band magnitude from OGLE-3 survey {catalogue TType keyword: VMAG} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcRRlyraeVariables |
VMCv20160822 |
Mean V band magnitude from OGLE-3 survey {catalogue TType keyword: VMAG} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcRRlyraeVariables |
VMCv20170109 |
Mean V band magnitude from OGLE-3 survey {catalogue TType keyword: VMAG} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcRRlyraeVariables |
VMCv20170411 |
Mean V band magnitude from OGLE-3 survey {catalogue TType keyword: VMAG} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcRRlyraeVariables |
VMCv20171101 |
Mean V band magnitude from OGLE-3 survey {catalogue TType keyword: VMAG} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcRRlyraeVariables |
VMCv20180702 |
Mean V band magnitude from OGLE-3 survey {catalogue TType keyword: VMAG} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcRRlyraeVariables |
VMCv20181120 |
Mean V band magnitude from OGLE-3 survey {catalogue TType keyword: VMAG} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcRRlyraeVariables |
VMCv20191212 |
Mean V band magnitude from OGLE-3 survey {catalogue TType keyword: VMAG} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcRRlyraeVariables |
VMCv20210708 |
Mean V band magnitude from OGLE-3 survey {catalogue TType keyword: VMAG} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vMeanMag |
vmcRRlyraeVariables |
VMCv20230816 |
Mean V band magnitude from OGLE-3 survey {catalogue TType keyword: VMAG} |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean;em.opt.V |
vr_m_opt |
twomass_psc |
TWOMASS |
Visual or red magnitude of the associated optical source. |
real |
4 |
mag |
|
phot.flux |
vt_mag |
tycho2 |
GAIADR1 |
Tycho2 VT magnitude |
real |
4 |
mag |
|
phot.mag;em.opt.V |
VTmag_TYCHO2 |
ravedr5Source |
RAVE |
magnitude from TYCHO2 |
real |
4 |
mag VT |
|
phot.mag;em.opt.V |