F |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
F1 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Flux in IRAC band 1 |
real |
4 |
mJy |
-999.9 |
|
f1 |
hipparcos_new_reduction |
GAIADR1 |
Percentage rejected data |
int |
4 |
|
|
arith.ratio;stat.value |
F1_err |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
1sigma flux error (IRAC band 1) |
real |
4 |
mJy |
-999.9 |
|
F1_rms |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
RMS dev. of detection from F1 |
real |
4 |
mJy |
-999.9 |
|
F2 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Flux in IRAC band 2 |
real |
4 |
mJy |
-999.9 |
|
f2 |
hipparcos_new_reduction |
GAIADR1 |
Goodness of fit |
float |
8 |
|
|
stat.fit.goodness |
F24umMag |
spitzer_smcSource |
SPITZER |
The SPITZER F24μm band magnitude. |
real |
4 |
mag |
|
|
F2_err |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
1sigma flux error (IRAC band 2) |
real |
4 |
mJy |
-999.9 |
|
F2_rms |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
RMS dev. of detection from F2 |
real |
4 |
mJy |
-999.9 |
|
F3 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Flux in IRAC band 3 |
real |
4 |
mJy |
-999.9 |
|
F3_6 |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
3.6um IRAC (Band 1) flux |
real |
4 |
mJy |
-999.9 |
|
F3_6_err |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
3.6um IRAC (Band 1) 1 sigma error |
real |
4 |
mJy |
-999.9 |
|
F3_6_rms |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
RMS deviation of the individual detections from the final flux for 3.6um IRAC (Band 1) |
real |
4 |
mJy |
-999.9 |
|
F3_6umMag |
spitzer_smcSource |
SPITZER |
The SPITZER F3.6μm band magnitude. |
real |
4 |
mag |
|
|
F3_err |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
1sigma flux error (IRAC band 3) |
real |
4 |
mJy |
-999.9 |
|
F3_rms |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
RMS dev. of detection from F3 |
real |
4 |
mJy |
-999.9 |
|
F4 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Flux in IRAC band 4 |
real |
4 |
mJy |
-999.9 |
|
F4_5 |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
4.5um IRAC (Band 2) flux |
real |
4 |
mJy |
-999.9 |
|
F4_5_err |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
4.5um IRAC (Band 2) 1 sigma error |
real |
4 |
mJy |
-999.9 |
|
F4_5_rms |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
RMS deviation of the individual detections from the final flux for 4.5um IRAC (Band 2) |
real |
4 |
mJy |
-999.9 |
|
F4_5umMag |
spitzer_smcSource |
SPITZER |
The SPITZER F4.5μm band magnitude. |
real |
4 |
mag |
|
|
F4_err |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
1sigma flux error (IRAC band 4) |
real |
4 |
mJy |
-999.9 |
|
F4_rms |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
RMS dev. of detection from F4 |
real |
4 |
mJy |
-999.9 |
|
F5_8 |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
5.8um IRAC (Band 3) flux |
real |
4 |
mJy |
-999.9 |
|
F5_8_err |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
5.8um IRAC (Band 3) 1 sigma error |
real |
4 |
mJy |
-999.9 |
|
F5_8_rms |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
RMS deviation of the individual detections from the final flux for 5.8um IRAC (Band 3) |
real |
4 |
mJy |
-999.9 |
|
F5_8umMag |
spitzer_smcSource |
SPITZER |
The SPITZER F5.8μm band magnitude. |
real |
4 |
mag |
|
|
F70umMag |
spitzer_smcSource |
SPITZER |
The SPITZER F70μm band magnitude. |
real |
4 |
mag |
|
|
F8_0 |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
8.0um IRAC (Band 4) flux |
real |
4 |
mJy |
-999.9 |
|
F8_0_err |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
8.0um IRAC (Band 4) 1 sigma error |
real |
4 |
mJy |
-999.9 |
|
F8_0_rms |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
RMS deviation of the individual detections from the final flux for 8.0um IRAC (Band 4) |
real |
4 |
mJy |
-999.9 |
|
F8_0umMag |
spitzer_smcSource |
SPITZER |
The SPITZER F8.0μm band magnitude. |
real |
4 |
mag |
|
|
f_resFlux |
nvssSource |
NVSS |
[PS* ] Residual Code |
varchar |
2 |
|
|
meta.code |
faPcorrelation2 |
vvvVivaCatalogue |
VVVDR5 |
False alarm probability for Kfi variability index {catalogue TType keyword: FAPcorrelation2} |
float |
8 |
|
-9.999995e8 |
|
fCor_100 |
iras_psc |
IRAS |
Flux correction factor applied (times 1000, 100 micron) |
smallint |
2 |
|
|
instr.param |
fCor_12 |
iras_psc |
IRAS |
Flux correction factor applied (times 1000, 12 micron) |
smallint |
2 |
|
|
instr.param |
fCor_25 |
iras_psc |
IRAS |
Flux correction factor applied (times 1000, 25 micron) |
smallint |
2 |
|
|
instr.param |
fCor_60 |
iras_psc |
IRAS |
Flux correction factor applied (times 1000, 60 micron) |
smallint |
2 |
|
|
instr.param |
Fe |
ravedr5Source |
RAVE |
[Fe/H] abundance of Fe |
real |
4 |
dex |
|
phys.abund.Z |
Fe_N |
ravedr5Source |
RAVE |
Number of used spectral lines in calc. of [Fe/H] |
smallint |
2 |
|
|
meta.number |
fg_flg |
twomass_xsc |
TWOMASS |
flux-growth convergence flag. |
varchar |
6 |
|
|
meta.code |
FH |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
2MASS All-Sky PSC H Band flux |
real |
4 |
mJy |
-999.9 |
|
FH_err |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
2MASS All-Sky PSC H Band 1 sigma error |
real |
4 |
mJy |
-999.9 |
|
FiberNumber |
ravedr5Source |
RAVE |
Instrument fiber number (2df) [1..150] |
tinyint |
1 |
|
|
meta.id;instr.part |
FIBRE_R |
spectra |
SIXDF |
fibre number (row on CCD) |
smallint |
2 |
|
|
|
FIBRE_V |
spectra |
SIXDF |
fibre number (row on CCD) |
smallint |
2 |
|
|
|
field |
nvssSource |
NVSS |
Name of the original survey image field from which the component was derived. |
varchar |
8 |
|
|
obs.field |
field1 |
iras_asc |
IRAS |
object field #1 (magnitude/other) |
smallint |
2 |
|
|
obs.field |
field2 |
iras_asc |
IRAS |
object field #2 (magnitude/other) |
smallint |
2 |
|
|
obs.field |
field3 |
iras_asc |
IRAS |
object field #3 (size/other) |
smallint |
2 |
|
|
obs.field |
fieldID |
ExternalProductCatalogue |
SHARKSv20210222 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
SHARKSv20210421 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
ULTRAVISTADR4 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSDR3 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSDR4 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSDR5 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSDR6 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSv20150108 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSv20160114 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSv20160507 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSv20170630 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSv20180419 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSv20201209 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSv20231101 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VHSv20240731 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VIDEODR4 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VIDEODR5 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VIKINGDR4 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VIKINGv20150421 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VIKINGv20151230 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VIKINGv20160406 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VIKINGv20161202 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VIKINGv20170715 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCDEEPv20230713 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCDEEPv20240506 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCDR4 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCDR5 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20140428 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20140903 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20150309 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20151218 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20160311 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20160822 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20170109 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20170411 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20171101 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20180702 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20181120 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20191212 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20210708 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20230816 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VMCv20240226 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VVVDR5 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue |
VVVXDR1 |
ID of field |
varchar |
16 |
|
NONE |
meta.id |
fieldID |
ExternalProductCatalogue, vmcCepheidVariables, vmcPsfCatalogue |
VMCDR3 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
ProgrammeFrame |
SHARKSv20210222 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
SHARKSv20210421 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
ULTRAVISTADR4 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VHSDR6 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VHSv20180419 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VHSv20201209 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VHSv20231101 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VHSv20240731 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VMCDEEPv20230713 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VMCDEEPv20240506 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VMCDR5 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VMCv20171101 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VMCv20180702 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VMCv20181120 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VMCv20191212 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VMCv20210708 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VMCv20230816 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VMCv20240226 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VSAQC |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VVVDR5 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
ProgrammeFrame |
VVVXDR1 |
UID of position on sky, set just after ProgrammeBuilder runs |
int |
4 |
|
-99999999 |
meta.bib |
fieldID |
RegionFieldLinks |
SHARKSv20210222 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
SHARKSv20210421 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
ULTRAVISTADR4 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VHSv20201209 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VHSv20231101 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VHSv20240731 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VMCDEEPv20230713 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VMCDEEPv20240506 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VMCDR5 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VMCv20191212 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VMCv20210708 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VMCv20230816 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VMCv20240226 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VVVDR5 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RegionFieldLinks |
VVVXDR1 |
Identifier assigned to each pointing in RequiredMosaic |
int |
4 |
|
|
?? |
fieldID |
RequiredMergeLogMultiEpoch |
SHARKSv20210222 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
SHARKSv20210421 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
ULTRAVISTADR4 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VHSDR5 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VHSDR6 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VHSv20160114 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VHSv20160507 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VHSv20170630 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VHSv20180419 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VHSv20201209 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VHSv20231101 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VHSv20240731 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VIKINGv20151230 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VIKINGv20160406 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VIKINGv20161202 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VIKINGv20170715 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCDEEPv20230713 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCDEEPv20240506 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCDR4 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCDR5 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20151218 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20160311 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20160822 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20170109 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20170411 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20171101 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20180702 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20181120 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20191212 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20210708 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20230816 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VMCv20240226 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VVVDR5 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMergeLogMultiEpoch |
VVVXDR1 |
UID of position on sky. References Required{productType}.fieldID |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
SHARKSv20210421 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
ULTRAVISTADR4 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSDR1 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSDR2 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSDR3 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSDR4 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSDR5 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSDR6 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSv20120926 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSv20130417 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSv20150108 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSv20160114 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSv20160507 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSv20170630 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSv20180419 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSv20201209 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSv20231101 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VHSv20240731 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIDEODR2 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIDEODR3 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIDEODR4 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIDEODR5 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIDEOv20111208 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGDR2 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGDR3 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGDR4 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGv20110714 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGv20111019 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGv20130417 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGv20150421 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGv20151230 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGv20160406 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGv20161202 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VIKINGv20170715 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCDEEPv20230713 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCDEEPv20240506 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCDR1 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCDR3 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCDR4 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCDR5 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20110816 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20110909 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20120126 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20121128 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20130304 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20130805 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20140428 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20140903 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20150309 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20151218 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20160311 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20160822 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20170109 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20170411 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20171101 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20180702 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20181120 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20191212 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20210708 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20230816 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VMCv20240226 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VVVDR1 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VVVDR2 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VVVDR5 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VVVXDR1 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VVVv20100531 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic |
VVVv20110718 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
RequiredMosaic, RequiredStack, RequiredTile |
SHARKSv20210222 |
UID of position on sky. |
int |
4 |
|
-99999999 |
?? |
fieldID |
StdFieldInfo |
VIDEOv20100513 |
The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations |
int |
4 |
|
|
obs.field |
fieldID |
StdFieldInfo |
VIKINGv20110714 |
The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations |
int |
4 |
|
|
obs.field |
fieldID |
StdFieldInfo |
VVVv20100531 |
The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations |
int |
4 |
|
|
obs.field |
fieldID |
rosat_bsc, rosat_fsc |
ROSAT |
identification number of SASS field |
varchar |
8 |
|
|
obs.field |
fieldID |
ultravistaMapLcVarFrameSetInfo |
ULTRAVISTADR4 |
fieldID, assigned in grouping procedure |
bigint |
8 |
|
|
meta.id;obs.field |
fieldID |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
field ID assigned by ProgrammeBuilder module when grouping. |
bigint |
8 |
|
|
meta.id;obs.field |
fieldID |
vmcRRlyraeVariables |
VMCDR4 |
ID of field {catalogue TType keyword: FIELDID} |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
vmcRRlyraeVariables |
VMCv20160822 |
ID of field {catalogue TType keyword: FIELDID} |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
vmcRRlyraeVariables |
VMCv20170109 |
ID of field {catalogue TType keyword: FIELDID} |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
vmcRRlyraeVariables |
VMCv20170411 |
ID of field {catalogue TType keyword: FIELDID} |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
vmcRRlyraeVariables |
VMCv20171101 |
ID of field {catalogue TType keyword: FIELDID} |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
vmcRRlyraeVariables |
VMCv20180702 |
ID of field {catalogue TType keyword: FIELDID} |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
vmcRRlyraeVariables |
VMCv20181120 |
ID of field {catalogue TType keyword: FIELDID} |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
vmcRRlyraeVariables |
VMCv20191212 |
ID of field {catalogue TType keyword: FIELDID} |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
vmcRRlyraeVariables |
VMCv20210708 |
ID of field {catalogue TType keyword: FIELDID} |
varchar |
8 |
|
NONE |
meta.id |
fieldID |
vmcRRlyraeVariables |
VMCv20230816 |
ID of field {catalogue TType keyword: FIELDID} |
varchar |
8 |
|
NONE |
meta.id |
fieldid |
smashdr2_source |
SMASH |
Field ID |
int |
4 |
|
|
|
FieldName |
ravedr5Source |
RAVE |
Center of Observed Field (RA/Dec) |
varchar |
8 |
|
|
meta.id;meta.file |
fieldName |
PreviousCalibParams |
SHARKSv20210222 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
SHARKSv20210421 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
VHSv20201209 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
VHSv20231101 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
VHSv20240731 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
VMCDEEPv20230713 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
VMCDEEPv20240506 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
VMCv20210708 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
VMCv20230816 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
VMCv20240226 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
VVVDR5 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
PreviousCalibParams |
VVVXDR1 |
Pointing within the table (if all updated in the same way, use ALL) |
varchar |
16 |
|
|
|
fieldName |
StdFieldInfo |
VIDEOv20100513 |
reference name of field |
varchar |
16 |
|
NONE |
???? |
fieldName |
StdFieldInfo |
VIKINGv20110714 |
reference name of field |
varchar |
16 |
|
NONE |
???? |
fieldName |
StdFieldInfo |
VVVv20100531 |
reference name of field |
varchar |
16 |
|
NONE |
???? |
fieldName |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
Name of the coadded image containing the source (encodes the position of the field center). |
varchar |
12 |
|
|
obs.image |
fieldName |
vmcPointings |
VMCDR4 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCDR5 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20160311 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20160822 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20170109 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20170411 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20171101 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20180702 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20181120 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20191212 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20210708 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20230816 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcPointings |
VMCv20240226 |
Pointing name, region_tile e.g. LMC_8_8 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vmcProperMotionCatalogue, vmcPsfSource |
VMCv20240226 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldName |
vmcPsfDetections |
VMCv20180702 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldName |
vmcPsfDetections |
VMCv20181120 |
ID of field |
varchar |
8 |
|
NONE |
meta.id |
fieldName |
vvvPointings |
VVVDR5 |
Pointing name, region_tile e.g. B318 |
varchar |
16 |
|
NONE |
meta.id,meta.main |
fieldName |
vvvProperMotionCatalogue, vvvVivaCatalogue |
VVVDR5 |
UID of the pointing that this object comes from |
varchar |
16 |
|
|
meta.id |
fieldName |
vvvPsfDaophotJKsMergeLog, vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
the name of the pointing e.g. B418 |
varchar |
16 |
|
|
meta.id,meta.main |
fileName |
ExternalProductCatalogue |
SHARKSv20210222 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
SHARKSv20210421 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
ULTRAVISTADR4 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSDR3 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSDR4 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSDR5 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSDR6 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSv20150108 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSv20160114 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSv20160507 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSv20170630 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSv20180419 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSv20201209 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSv20231101 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VHSv20240731 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VIDEODR4 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VIDEODR5 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VIKINGDR4 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VIKINGv20150421 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VIKINGv20151230 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VIKINGv20160406 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VIKINGv20161202 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VIKINGv20170715 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCDEEPv20230713 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCDEEPv20240506 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCDR3 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCDR4 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCDR5 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20140428 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20140903 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20150309 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20151218 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20160311 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20160822 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20170109 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20170411 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20171101 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20180702 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20181120 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20191212 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20210708 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20230816 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VMCv20240226 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VVVDR5 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
ExternalProductCatalogue |
VVVXDR1 |
Filename of file sent from survey team |
varchar |
128 |
|
|
|
fileName |
Multiframe |
SHARKSv20210222 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
SHARKSv20210421 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
ULTRAVISTADR4 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSDR1 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSDR2 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSDR3 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSDR4 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSDR5 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSDR6 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20120926 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20130417 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20140409 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20150108 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20160114 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20160507 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20170630 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20180419 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20201209 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20231101 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VHSv20240731 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIDEODR2 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIDEODR3 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIDEODR4 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIDEODR5 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIDEOv20100513 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIDEOv20111208 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGDR2 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGDR3 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGDR4 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGv20110714 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGv20111019 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGv20130417 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGv20140402 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGv20150421 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGv20151230 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGv20160406 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGv20161202 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VIKINGv20170715 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCDEEPv20230713 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCDEEPv20240506 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCDR1 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCDR2 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCDR3 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCDR4 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCDR5 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20110816 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20110909 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20120126 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20121128 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20130304 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20130805 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20140428 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20140903 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20150309 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20151218 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20160311 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20160822 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20170109 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20170411 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20171101 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20180702 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20181120 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20191212 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20210708 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20230816 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VMCv20240226 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VVVDR1 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VVVDR2 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VVVDR5 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VVVXDR1 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VVVv20100531 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
Multiframe |
VVVv20110718 |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
'NONE' |
meta.id;meta.file |
fileName |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
|
meta.id;meta.file |
fileNameRoot |
ExternalProduct |
SHARKSv20210222 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
SHARKSv20210421 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
ULTRAVISTADR4 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSDR3 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSDR4 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSDR5 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSDR6 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSv20150108 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSv20160114 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSv20160507 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSv20170630 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSv20180419 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSv20201209 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSv20231101 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VHSv20240731 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VIDEODR4 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VIDEODR5 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VIDEOv20111208 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VIKINGDR4 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VIKINGv20150421 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VIKINGv20151230 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VIKINGv20160406 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VIKINGv20161202 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VIKINGv20170715 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCDEEPv20230713 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCDEEPv20240506 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCDR3 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCDR4 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCDR5 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20140428 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20140903 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20150309 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20151218 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20160311 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20160822 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20170109 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20170411 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20171101 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20180702 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20181120 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20191212 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20210708 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20230816 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VMCv20240226 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VVVDR5 |
File name root of the products |
varchar |
32 |
|
|
|
fileNameRoot |
ExternalProduct |
VVVXDR1 |
File name root of the products |
varchar |
32 |
|
|
|
fileTimeStamp |
Multiframe |
SHARKSv20210222 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
SHARKSv20210421 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
ULTRAVISTADR4 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSDR1 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSDR2 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSDR3 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSDR4 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSDR5 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSDR6 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20120926 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20130417 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20140409 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20150108 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20160114 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20160507 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20170630 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20180419 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20201209 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20231101 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VHSv20240731 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIDEODR2 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIDEODR3 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIDEODR4 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIDEODR5 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIDEOv20100513 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIDEOv20111208 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGDR2 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGDR3 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGDR4 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGv20110714 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGv20111019 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGv20130417 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGv20140402 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGv20150421 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGv20151230 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGv20160406 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGv20161202 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VIKINGv20170715 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCDEEPv20230713 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCDEEPv20240506 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCDR1 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCDR2 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCDR3 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCDR4 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCDR5 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20110816 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20110909 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20120126 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20121128 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20130304 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20130805 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20140428 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20140903 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20150309 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20151218 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20160311 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20160822 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20170109 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20170411 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20171101 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20180702 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20181120 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20191212 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20210708 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20230816 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VMCv20240226 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VVVDR1 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VVVDR2 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VVVDR5 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VVVXDR1 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VVVv20100531 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
Multiframe |
VVVv20110718 |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
-99999999 |
?? |
fileTimeStamp |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
|
?? |
filter |
smashdr2_source |
SMASH |
Filter, u, g, r, i, or z |
varchar |
1 |
|
|
|
filter1 |
RequiredDiffImage |
SHARKSv20210222 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
SHARKSv20210421 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
ULTRAVISTADR4 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSDR1 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSDR2 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSDR3 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSDR4 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSDR5 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSDR6 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSv20120926 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSv20130417 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSv20150108 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSv20160114 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSv20160507 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSv20170630 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSv20180419 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSv20201209 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSv20231101 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VHSv20240731 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIDEODR2 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIDEODR3 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIDEODR4 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIDEODR5 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIDEOv20100513 |
UID of WFCAM narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIDEOv20111208 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGDR2 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGDR3 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGDR4 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGv20110714 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGv20111019 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGv20130417 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGv20150421 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGv20151230 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGv20160406 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGv20161202 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VIKINGv20170715 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCDEEPv20230713 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCDEEPv20240506 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCDR1 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCDR3 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCDR4 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCDR5 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20110816 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20110909 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20120126 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20121128 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20130304 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20130805 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20140428 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20140903 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20150309 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20151218 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20160311 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20160822 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20170109 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20170411 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20171101 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20180702 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20181120 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20191212 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20210708 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20230816 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VMCv20240226 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VVVDR1 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VVVDR2 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VVVDR5 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VVVXDR1 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VVVv20100531 |
UID of WFCAM narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1 |
RequiredDiffImage |
VVVv20110718 |
UID of narrow band (primary) filter |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter1_bfilmax |
machoLMCSource, machoSMCSource |
MACHO |
Filter 1, blue: max value of optimum filter for LC |
real |
4 |
|
|
|
filter1_bfiltime |
machoLMCSource, machoSMCSource |
MACHO |
Filter 1, blue: LC time at which maximum occurred |
real |
4 |
|
|
|
filter1_bNhi |
machoLMCSource, machoSMCSource |
MACHO |
Filter 1, blue: number points sigmathreshold high within duration of filter at peak (bfiltime) |
smallint |
2 |
|
|
|
filter1_rfilmax |
machoLMCSource, machoSMCSource |
MACHO |
Filter 1, red: max value of optimum filter for LC |
real |
4 |
|
|
|
filter1_rfiltime |
machoLMCSource, machoSMCSource |
MACHO |
Filter 1, red: LC time at which maximum occurred |
real |
4 |
|
|
|
filter1_rNhi |
machoLMCSource, machoSMCSource |
MACHO |
Filter 1, red: number points sigmathreshold high within duration of filter at peak (rfiltime) |
smallint |
2 |
|
|
|
filter2 |
RequiredDiffImage |
SHARKSv20210222 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
SHARKSv20210421 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
ULTRAVISTADR4 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSDR1 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSDR2 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSDR3 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSDR4 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSDR5 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSDR6 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSv20120926 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSv20130417 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSv20150108 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSv20160114 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSv20160507 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSv20170630 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSv20180419 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSv20201209 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSv20231101 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VHSv20240731 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIDEODR2 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIDEODR3 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIDEODR4 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIDEODR5 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIDEOv20100513 |
UID of WFCAM broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIDEOv20111208 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGDR2 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGDR3 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGDR4 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGv20110714 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGv20111019 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGv20130417 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGv20150421 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGv20151230 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGv20160406 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGv20161202 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VIKINGv20170715 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCDEEPv20230713 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCDEEPv20240506 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCDR1 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCDR3 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCDR4 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCDR5 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20110816 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20110909 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20120126 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20121128 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20130304 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20130805 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20140428 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20140903 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20150309 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20151218 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20160311 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20160822 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20170109 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20170411 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20171101 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20180702 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20181120 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20191212 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20210708 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20230816 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VMCv20240226 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VVVDR1 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VVVDR2 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VVVDR5 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VVVXDR1 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VVVv20100531 |
UID of WFCAM broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2 |
RequiredDiffImage |
VVVv20110718 |
UID of broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
meta.code;instr.filter |
filter2_bfilmax |
machoLMCSource, machoSMCSource |
MACHO |
Filter 2, blue: max value of optimum filter for LC |
real |
4 |
|
|
|
filter2_bfiltime |
machoLMCSource, machoSMCSource |
MACHO |
Filter 2, blue: LC time at which maximum occurred |
real |
4 |
|
|
|
filter2_bNhi |
machoLMCSource, machoSMCSource |
MACHO |
Filter 2, blue: number points sigmathreshold high within duration of filter at peak (bfiltime) |
smallint |
2 |
|
|
|
filter2_rfilmax |
machoLMCSource, machoSMCSource |
MACHO |
Filter 2, red: max value of optimum filter for LC |
real |
4 |
|
|
|
filter2_rfiltime |
machoLMCSource, machoSMCSource |
MACHO |
Filter 2, red: LC time at which maximum occurred |
real |
4 |
|
|
|
filter2_rNhi |
machoLMCSource, machoSMCSource |
MACHO |
Filter 2, red: number points sigmathreshold high within duration of filter at peak (rfiltime) |
smallint |
2 |
|
|
|
filter3_bfilmax |
machoLMCSource, machoSMCSource |
MACHO |
Filter 3, blue: max value of optimum filter for LC |
real |
4 |
|
|
|
filter3_bfiltime |
machoLMCSource, machoSMCSource |
MACHO |
Filter 3, blue: LC time at which maximum occurred |
real |
4 |
|
|
|
filter3_bNhi |
machoLMCSource, machoSMCSource |
MACHO |
Filter 3, blue: number points sigmathreshold high within duration of filter at peak (bfiltime) |
smallint |
2 |
|
|
|
filter3_rfilmax |
machoLMCSource, machoSMCSource |
MACHO |
Filter 3, red: max value of optimum filter for LC |
real |
4 |
|
|
|
filter3_rfiltime |
machoLMCSource, machoSMCSource |
MACHO |
Filter 3, red: LC time at which maximum occurred |
real |
4 |
|
|
|
filter3_rNhi |
machoLMCSource, machoSMCSource |
MACHO |
Filter 3, red: number points sigmathreshold high within duration of filter at peak (rfiltime) |
smallint |
2 |
|
|
|
filteredImageName |
MapFrameStatus |
SHARKSv20210222 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
SHARKSv20210421 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
ULTRAVISTADR4 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VHSv20201209 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VHSv20231101 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VHSv20240731 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VMCDEEPv20230713 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VMCDEEPv20240506 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VMCDR5 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VMCv20191212 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VMCv20210708 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VMCv20230816 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VMCv20240226 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VVVDR5 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filteredImageName |
MapFrameStatus |
VVVXDR1 |
the filename of the associated filtered image name, eg. server:/path/filename_st_tl_two.fit |
varchar |
256 |
|
NONE |
|
filterID |
CombinedFilters |
SHARKSv20210222 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
SHARKSv20210421 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
ULTRAVISTADR4 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VHSv20201209 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VHSv20231101 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VHSv20240731 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VMCDEEPv20230713 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VMCDEEPv20240506 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VMCDR5 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VMCv20191212 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VMCv20210708 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VMCv20230816 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VMCv20240226 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VVVDR5 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
CombinedFilters |
VVVXDR1 |
UID of combined filter |
tinyint |
1 |
|
|
meta.code |
filterID |
Detection |
PS1DR2 |
Filter identifier. Details in the Filter table. |
tinyint |
1 |
|
|
|
filterID |
Filter |
SHARKSv20210421 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
ULTRAVISTADR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSDR6 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSv20120926 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSv20130417 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSv20150108 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSv20160114 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSv20160507 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSv20170630 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSv20180419 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSv20201209 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSv20231101 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VHSv20240731 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIDEODR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIDEODR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIDEODR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIDEODR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIDEOv20100513 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIDEOv20111208 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGv20110714 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGv20111019 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGv20130417 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGv20150421 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGv20151230 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGv20160406 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGv20161202 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VIKINGv20170715 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCDEEPv20230713 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCDEEPv20240506 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20110816 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20110909 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20120126 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20121128 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20130304 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20130805 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20140428 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20140903 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20150309 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20151218 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20160311 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20160822 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20170109 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20170411 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20171101 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20180702 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20181120 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20191212 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20210708 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20230816 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VMCv20240226 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VSAQC |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VVVDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VVVDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VVVDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VVVXDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VVVv20100531 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter |
VVVv20110718 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Filter, MapFilterLupt, RequiredFilters, RequiredMosaic, RequiredStack, RequiredTile |
SHARKSv20210222 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterExtinctionCoefficients |
EXTINCT |
UID of filter |
smallint |
2 |
|
|
meta.id;meta.main |
filterID |
FilterSections |
SHARKSv20210421 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
ULTRAVISTADR4 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSDR3 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSDR4 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSDR5 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSDR6 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSv20150108 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSv20160114 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSv20160507 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSv20170630 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSv20180419 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSv20201209 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSv20231101 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VHSv20240731 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VIDEODR4 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VIDEODR5 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VIKINGDR4 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VIKINGv20150421 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VIKINGv20151230 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VIKINGv20160406 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VIKINGv20161202 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VIKINGv20170715 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCDEEPv20230713 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCDEEPv20240506 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCDR3 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCDR4 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCDR5 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20140428 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20140903 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20150309 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20151218 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20160311 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20160822 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20170109 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20170411 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20171101 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20180702 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20181120 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20191212 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20210708 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20230816 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VMCv20240226 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VSAQC |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VVVDR5 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections |
VVVXDR1 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
FilterSections, RequiredMergeLogMultiEpoch |
SHARKSv20210222 |
UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
Multiframe |
SHARKSv20210222 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
SHARKSv20210421 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
ULTRAVISTADR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSDR6 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20120926 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20130417 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20140409 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20150108 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20160114 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20160507 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20170630 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20180419 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20201209 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20231101 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VHSv20240731 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIDEODR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIDEODR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIDEODR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIDEODR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIDEOv20100513 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIDEOv20111208 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGv20110714 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGv20111019 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGv20130417 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGv20140402 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGv20150421 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGv20151230 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGv20160406 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGv20161202 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VIKINGv20170715 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCDEEPv20230713 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCDEEPv20240506 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20110816 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20110909 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20120126 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20121128 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20130304 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20130805 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20140428 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20140903 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20150309 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20151218 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20160311 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20160822 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20170109 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20170411 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20171101 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20180702 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20181120 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20191212 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20210708 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20230816 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VMCv20240226 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VVVDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VVVDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VVVDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VVVXDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VVVv20100531 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
Multiframe |
VVVv20110718 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
SHARKSv20210222 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
SHARKSv20210421 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
ULTRAVISTADR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSDR6 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20120926 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20130417 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20140409 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20150108 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20160114 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20160507 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20170630 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20180419 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20201209 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20231101 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VHSv20240731 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIDEODR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIDEODR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIDEODR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIDEODR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIDEOv20100513 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIDEOv20111208 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGv20110714 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGv20111019 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGv20130417 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGv20140402 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGv20150421 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGv20151230 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGv20160406 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGv20161202 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VIKINGv20170715 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCDEEPv20230713 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCDEEPv20240506 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20110816 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20110909 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20120126 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20121128 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20130304 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20130805 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20140428 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20140903 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20150309 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20151218 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20160311 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20160822 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20170109 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20170411 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20171101 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20180702 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20181120 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20191212 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20210708 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20230816 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VMCv20240226 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VVVDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VVVDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VVVDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VVVXDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VVVv20100531 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
MultiframeDetector |
VVVv20110718 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
tinyint |
1 |
|
0 |
meta.code;instr.filter |
filterID |
RequiredListDrivenProduct |
VHSv20120926 |
filterID of the data that the list is driven from. If 0, then take the source list. |
tinyint |
1 |
|
0 |
|
filterID |
RequiredListDrivenProduct |
VIDEODR3 |
filterID of the data that the list is driven from. If 0, then take the source list. |
tinyint |
1 |
|
0 |
|
filterID |
RequiredListDrivenProduct |
VIKINGDR3 |
filterID of the data that the list is driven from. If 0, then take the source list. |
tinyint |
1 |
|
0 |
|
filterID |
RequiredListDrivenProduct |
VMCv20121128 |
filterID of the data that the list is driven from. If 0, then take the source list. |
tinyint |
1 |
|
0 |
|
filterID |
RequiredListDrivenProduct |
VMCv20130304 |
filterID of the data that the list is driven from. If 0, then take the source list. |
tinyint |
1 |
|
0 |
|
filterID |
RequiredListDrivenProduct |
VVVDR1 |
filterID of the data that the list is driven from. If 0, then take the source list. |
tinyint |
1 |
|
0 |
|
filterID |
sharksDetection |
SHARKSv20210222 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
sharksDetection |
SHARKSv20210421 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
sharksMultiframe, sharksMultiframeDetector, ultravistaMultiframe, ultravistaMultiframeDetector, vhsMultiframe, vhsMultiframeDetector, videoMultiframe, videoMultiframeDetector, vikingMultiframe, vikingMultiframeDetector, vmcMultiframe, vmcMultiframeDetector, vvvMultiframe, vvvMultiframeDetector |
VSAQC |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
ultravistaDetection |
ULTRAVISTADR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
UID of combined filter (assigned in VSA) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSDR6 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20120926 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20130417 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20140409 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20150108 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20160114 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20160507 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20170630 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20180419 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20201209 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20231101 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsDetection |
VHSv20240731 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vhsListRemeasurement |
VHSDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
videoDetection |
VIDEODR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
videoDetection |
VIDEODR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
videoDetection |
VIDEODR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
videoDetection |
VIDEODR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
videoDetection |
VIDEOv20100513 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
videoDetection |
VIDEOv20111208 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
videoListRemeasurement |
VIDEOv20100513 |
UID of combined filter (assigned in WSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGv20110714 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGv20111019 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGv20130417 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGv20140402 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGv20150421 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGv20151230 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGv20160406 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGv20161202 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingDetection |
VIKINGv20170715 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingListRemeasurement |
VIKINGv20110714 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingListRemeasurement |
VIKINGv20111019 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vikingMapRemeasAver, vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCDR3 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCDR4 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20110816 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20110909 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20120126 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20121128 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20130304 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20130805 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20140428 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20140903 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20150309 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20151218 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20160311 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20160822 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20170109 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20170411 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20171101 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20180702 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20181120 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20191212 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20210708 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20230816 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcDetection |
VMCv20240226 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcListRemeasurement |
VMCv20110816 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcListRemeasurement |
VMCv20110909 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcRRLyraeLightCurves |
VMCv20240226 |
Filter ID |
smallint |
2 |
|
|
|
filterID |
vmcdeepDetection |
VMCDEEPv20230713 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vmcdeepDetection |
VMCDEEPv20240506 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vvvDetection |
VVVDR1 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vvvDetection |
VVVDR2 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vvvDetection |
VVVv20100531 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vvvListRemeasurement |
VVVv20100531 |
UID of combined filter (assigned in WSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterID |
vvvListRemeasurement |
VVVv20110718 |
UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
|
meta.code;instr.filter |
filterIDList |
CombinedFilters |
SHARKSv20210222 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
SHARKSv20210421 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
ULTRAVISTADR4 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VHSv20201209 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VHSv20231101 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VHSv20240731 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VMCDEEPv20230713 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VMCDEEPv20240506 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VMCDR5 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VMCv20191212 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VMCv20210708 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VMCv20230816 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VMCv20240226 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VVVDR5 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterIDList |
CombinedFilters |
VVVXDR1 |
List of filters as comma separated string. Optional put archive in front if filters from multiple archives: eg. WSA-1,2,3;SDSS-2,3,4 |
varchar |
64 |
|
|
|
filterList |
RequiredListDrivenProduct |
VHSv20130417 |
the list of filters used in initial selection? (standard programmeFilters) if NONE |
varchar |
64 |
|
NONE |
|
filterList |
RequiredListDrivenProduct |
VIKINGv20130417 |
the list of filters used in initial selection? (standard programmeFilters) if NONE |
varchar |
64 |
|
NONE |
|
filterList |
RequiredListDrivenProduct |
VMCv20130805 |
the list of filters used in initial selection? (standard programmeFilters) if NONE |
varchar |
64 |
|
NONE |
|
filterN |
machoLMCSource, machoSMCSource |
MACHO |
number of filters applied; always 3 |
smallint |
2 |
|
|
|
filterName |
Multiframe |
SHARKSv20210222 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
SHARKSv20210421 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
ULTRAVISTADR4 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSDR1 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSDR2 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSDR3 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSDR4 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSDR5 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSDR6 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20120926 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20130417 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20140409 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20150108 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20160114 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20160507 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20170630 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20180419 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20201209 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20231101 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VHSv20240731 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIDEODR2 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIDEODR3 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIDEODR4 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIDEODR5 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIDEOv20100513 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIDEOv20111208 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGDR2 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGDR3 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGDR4 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGv20110714 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGv20111019 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGv20130417 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGv20140402 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGv20150421 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGv20151230 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGv20160406 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGv20161202 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VIKINGv20170715 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCDEEPv20230713 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCDEEPv20240506 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCDR1 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCDR2 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCDR3 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCDR4 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCDR5 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20110816 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20110909 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20120126 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20121128 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20130304 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20130805 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20140428 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20140903 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20150309 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20151218 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20160311 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20160822 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20170109 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20170411 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20171101 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20180702 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20181120 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20191212 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20210708 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20230816 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VMCv20240226 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VVVDR1 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VVVDR2 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VVVDR5 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VVVXDR1 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VVVv20100531 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
Multiframe |
VVVv20110718 |
VISTA combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME} |
varchar |
16 |
|
'NONE' |
?? |
filterName |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
VISTA combined filter name |
varchar |
16 |
|
|
?? |
filterType |
Filter |
SHARKSv20210222 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
SHARKSv20210421 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
ULTRAVISTADR4 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSDR4 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSDR5 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSDR6 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSv20150108 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSv20160114 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSv20160507 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSv20170630 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSv20180419 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSv20201209 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSv20231101 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VHSv20240731 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VIDEODR4 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VIDEODR5 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VIKINGv20150421 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VIKINGv20151230 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VIKINGv20160406 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VIKINGv20161202 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VIKINGv20170715 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCDEEPv20230713 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCDEEPv20240506 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCDR4 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCDR5 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20140903 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20150309 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20151218 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20160311 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20160822 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20170109 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20170411 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20171101 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20180702 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20181120 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20191212 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20210708 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20230816 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VMCv20240226 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VSAQC |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VVVDR5 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
filterType |
Filter |
VVVXDR1 |
The type of filter BROAD, NARROW, BROADLIST |
varchar |
16 |
|
NONE |
|
finalProductTable |
RequiredMatchedApertureProduct |
SHARKSv20210222 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
SHARKSv20210421 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
ULTRAVISTADR4 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VHSv20201209 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VHSv20231101 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VHSv20240731 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VMCDEEPv20230713 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VMCDEEPv20240506 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VMCDR5 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VMCv20191212 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VMCv20210708 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VMCv20230816 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VMCv20240226 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VVVDR5 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
finalProductTable |
RequiredMatchedApertureProduct |
VVVXDR1 |
the name of the final product table for this product |
varchar |
64 |
|
|
meta.id;meta.dataset |
fInt |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
integrated flux densities |
real |
4 |
mJy |
|
phot.flux.density;em.radio.750-1500MHz |
Fit_Flag_Binney |
ravedr5Source |
RAVE |
See final paragraph 3 (Binney et al. 2014) |
int |
4 |
|
|
meta.code.qual |
Fitmag_I |
denisDR3Source |
DENIS |
Magnitude in I band from PSF fit |
float |
8 |
mag |
|
|
Fitmag_J |
denisDR3Source |
DENIS |
Magnitude in J band from PSF fit |
float |
8 |
mag |
|
|
Fitmag_K |
denisDR3Source |
DENIS |
Magnitude in K band from PSF fit |
float |
8 |
mag |
|
|
FitQuality_Binney |
ravedr5Source |
RAVE |
Given by symbol F in eq 15 of Binney et al. (2014) |
real |
4 |
|
|
meta.code.qual |
FJ |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
2MASS All-Sky PSC J Band flux |
real |
4 |
mJy |
-999.9 |
|
FJ_err |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
2MASS All-Sky PSC J Band 1 sigma error |
real |
4 |
mJy |
-999.9 |
|
FKs |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
2MASS All-Sky PSC Ks Band flux |
real |
4 |
mJy |
-999.9 |
|
FKs_err |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
2MASS All-Sky PSC Ks Band 1 sigma error |
real |
4 |
mJy |
-999.9 |
|
flag |
sharksSourceXDetectionBestMatch |
SHARKSv20210222 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
sharksSourceXDetectionBestMatch |
SHARKSv20210421 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
smashdr2_deep, smashdr2_object |
SMASH |
OR-combined Source Extractor FLAG value from coadd image |
smallint |
2 |
|
|
|
flag |
smashdr2_source |
SMASH |
Source Extractor FLAG value from coadd image |
smallint |
2 |
|
|
|
flag |
ultravistaSourceXDetectionBestMatch |
ULTRAVISTADR4 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
videoSourceXDetectionBestMatch |
VIDEODR2 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
videoSourceXDetectionBestMatch |
VIDEODR3 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
videoSourceXDetectionBestMatch |
VIDEODR4 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
videoSourceXDetectionBestMatch |
VIDEODR5 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
videoSourceXDetectionBestMatch |
VIDEOv20100513 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
videoSourceXDetectionBestMatch |
VIDEOv20111208 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGDR2 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGDR3 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGDR4 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGv20110714 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGv20111019 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGv20130417 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGv20140402 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGv20150421 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGv20151230 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGv20160406 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGv20161202 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vikingSourceXDetectionBestMatch |
VIKINGv20170715 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCDR1 |
Flag for potential matching problems |
int |
4 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCDR2 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCDR3 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCDR4 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCDR5 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20110816 |
Flag for potential matching problems |
int |
4 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20110909 |
Flag for potential matching problems |
int |
4 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20120126 |
Flag for potential matching problems |
int |
4 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20121128 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20130304 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20130805 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20140428 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20140903 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20150309 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20151218 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20160311 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20160822 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20170109 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20170411 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20171101 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20180702 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20181120 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20191212 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20210708 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20230816 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcSourceXSynopticSourceBestMatch |
VMCv20240226 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcdeepSourceXSynopticSourceBestMatch |
VMCDEEPv20230713 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vmcdeepSourceXSynopticSourceBestMatch |
VMCDEEPv20240506 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vvvSourceXDetectionBestMatch |
VVVDR1 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vvvSourceXDetectionBestMatch |
VVVDR2 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vvvSourceXDetectionBestMatch |
VVVDR5 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vvvSourceXDetectionBestMatch |
VVVv20100531 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vvvSourceXDetectionBestMatch |
VVVv20110718 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
|
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vvvSourceXSynopticSourceBestMatch |
VVVDR1 |
Flag for potential matching problems |
int |
4 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag |
vvvxSourceXDetectionBestMatch |
VVVXDR1 |
Flag for potential matching problems |
tinyint |
1 |
|
0 |
meta.code.qual |
flag=1 if the same intermediate stack detection is linked to two different unique sources. This can happen in images where the seeing was poorer than average or if a source has moved over time and overlaps with another source. flag=2 no intermediate stack detection, but the expected location is in 1 dither offset of the edge of the stack. |
flag160 |
sage_lmcMips160Source |
SPITZER |
How many times a source was observed by different AORs in a single epoch |
int |
4 |
|
|
|
flag24 |
sage_lmcMips24Source |
SPITZER |
How many times a source was observed by different AORs in a single epoch |
int |
4 |
|
|
|
flag70 |
sage_lmcMips70Source |
SPITZER |
How many times a source was observed by different AORs in a single epoch |
int |
4 |
|
|
|
Flag_I |
denisDR3Source |
DENIS |
Image and source flag in I band This flag is the concatenation of image and source flags, in hexadecimal format. For the image flag, the first two digits contain: Bit 0 - clouds during observation; Bit 1 - electronic Read-Out problem; Bit 2 - internal temperature problem; Bit 3 - very bright star; Bit 4 - bright star; Bit 5 - stray light; Bit 6 - unknown problem. For the source flag, the last two digits contain: Bit 0 - source might be a dust on mirror; Bit 1 - source is a ghost detection of a bright star; Bit 2 - source is saturated; Bit 3 - source is multiple detect. |
varchar |
5 |
|
|
|
Flag_J |
denisDR3Source |
DENIS |
Image and source flag in J band This flag is the concatenation of image and source flags, in hexadecimal format. For the image flag, the first two digits contain: Bit 0 - clouds during observation; Bit 1 - electronic Read-Out problem; Bit 2 - internal temperature problem; Bit 3 - very bright star; Bit 4 - bright star; Bit 5 - stray light; Bit 6 - unknown problem. For the source flag, the last two digits contain: Bit 0 - source might be a dust on mirror; Bit 1 - source is a ghost detection of a bright star; Bit 2 - source is saturated; Bit 3 - source is multiple detect. |
varchar |
5 |
|
|
|
Flag_K |
denisDR3Source |
DENIS |
Image and source flag in K band This flag is the concatenation of image and source flags, in hexadecimal format. For the image flag, the first two digits contain: Bit 0 - clouds during observation; Bit 1 - electronic Read-Out problem; Bit 2 - internal temperature problem; Bit 3 - very bright star; Bit 4 - bright star; Bit 5 - stray light; Bit 6 - unknown problem. For the source flag, the last two digits contain: Bit 0 - source might be a dust on mirror; Bit 1 - source is a ghost detection of a bright star; Bit 2 - source is saturated; Bit 3 - source is multiple detect. |
varchar |
5 |
|
|
|
Flag_mult |
denisDR3Source |
DENIS |
Multiplicity flag; if set to 1, this flag indicates that the source was detected in two consecutive images, and that the 2 measurements have been combined. |
tinyint |
1 |
|
|
|
flagDataType |
vvvVivaCatalogue |
VVVDR5 |
Flag about data type, i.e correlated data (CCD) or non-correlated data (NCD) {catalogue TType keyword: FlagDataType} |
varchar |
4 |
|
NONE |
|
FLAGEQ |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Eqband flag that indicates the band at which the coordinates are determined (0:N3, 1:S7, 2:S11, 3:L15, 4:L24) |
char |
1 |
|
|
|
flagFbias6 |
vvvVivaCatalogue |
VVVDR5 |
Counts of periods within $10^{-6}$ periods, calculated per tile (for more details see Sect. \ref{sec_mainperiod}) related with FreqLSG {catalogue TType keyword: FlagFbias6} |
int |
4 |
|
-9999 |
|
flagFbias7 |
vvvVivaCatalogue |
VVVDR5 |
Counts of periods within $10^{-7}$ periods, calculated per tile (for more details see Sect. \ref{sec_mainperiod}) related with FreqLSG {catalogue TType keyword: FlagFbias7} |
int |
4 |
|
-9999 |
|
flagNfreq |
vvvVivaCatalogue |
VVVDR5 |
Number of frequencies in agreement with FreqLSG or its harmonic or subharmonic. It assumes values from 1 to 5 {catalogue TType keyword: FlagNfreq} |
smallint |
2 |
|
-9999 |
|
FLAGS |
mgcDetection |
MGC |
Extraction flags |
int |
4 |
|
|
|
flags |
masterDR2 |
SKYMAPPER |
Bitwise OR of Source Extractor flags across all observations |
smallint |
2 |
|
|
meta.code |
flags_psf |
masterDR2 |
SKYMAPPER |
Bitmask indicating whether photometry is likely biased by neighbours at >1%; bits 0-5 correspond to filters z-u |
int |
4 |
|
|
meta.code |
FLAGSL15 |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Star designation The flag consist of seven characters: exposure, photometry, saturation, mux bleed, column pulldown, artifact, and multiple flags. |
char |
7 |
|
9999999 |
|
FLAGSL24 |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Star designation The flag consist of seven characters: exposure, photometry, saturation, mux bleed, column pulldown, artifact, and multiple flags. |
char |
7 |
|
9999999 |
|
FLAGSN3 |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Star designation The flag consist of seven characters: exposure, photometry, saturation, mux bleed, column pulldown, artifact, and multiple flags. |
char |
7 |
|
9999999 |
|
FLAGSS11 |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Star designation The flag consist of seven characters: exposure, photometry, saturation, mux bleed, column pulldown, artifact, and multiple flags. |
char |
7 |
|
9999999 |
|
FLAGSS7 |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Star designation The flag consist of seven characters: exposure, photometry, saturation, mux bleed, column pulldown, artifact, and multiple flags. |
char |
7 |
|
9999999 |
|
flame_flags |
gaia_source |
GAIADR2 |
Flags from Apsis-FLAME analysis |
bigint |
8 |
|
|
meta.code |
flatID |
Multiframe |
SHARKSv20210222 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
SHARKSv20210421 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
ULTRAVISTADR4 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSDR1 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSDR2 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSDR3 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSDR4 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSDR5 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSDR6 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20120926 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20130417 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20140409 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20150108 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20160114 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20160507 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20170630 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20180419 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20201209 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20231101 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VHSv20240731 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIDEODR2 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIDEODR3 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIDEODR4 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIDEODR5 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIDEOv20100513 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIDEOv20111208 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGDR2 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGDR3 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGDR4 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGv20110714 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGv20111019 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGv20130417 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGv20140402 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGv20150421 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGv20151230 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGv20160406 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGv20161202 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VIKINGv20170715 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCDEEPv20230713 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCDEEPv20240506 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCDR1 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCDR2 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCDR3 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCDR4 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCDR5 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20110816 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20110909 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20120126 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20121128 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20130304 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20130805 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20140428 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20140903 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20150309 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20151218 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20160311 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20160822 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20170109 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20170411 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20171101 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20180702 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20181120 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20191212 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20210708 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20230816 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VMCv20240226 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VVVDR1 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VVVDR2 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VVVDR5 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VVVXDR1 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VVVv20100531 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
Multiframe |
VVVv20110718 |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
flatID |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
UID of library calibration flatfield frame |
bigint |
8 |
|
-99999999 |
obs.field |
flux160 |
sage_lmcMips160Source |
SPITZER |
160um flux |
float |
8 |
mJy |
|
|
flux24 |
sage_lmcMips24Source |
SPITZER |
24um flux |
float |
8 |
mJy |
|
|
flux3_6 |
sage_lmcIracSource |
SPITZER |
3.6um flux |
real |
4 |
mJy |
|
|
flux3_6 |
sage_smcIRACv1_5Source |
SPITZER |
3.6um IRAC (Band 1) flux |
real |
4 |
mJy |
|
|
flux4_5 |
sage_lmcIracSource |
SPITZER |
4.5um flux |
real |
4 |
mJy |
|
|
flux4_5 |
sage_smcIRACv1_5Source |
SPITZER |
4.5um IRAC (Band 1) flux |
real |
4 |
mJy |
|
|
flux5_8 |
sage_lmcIracSource |
SPITZER |
5.8um flux |
real |
4 |
mJy |
|
|
flux5_8 |
sage_smcIRACv1_5Source |
SPITZER |
5.8um IRAC (Band 1) flux |
real |
4 |
mJy |
|
|
flux70 |
sage_lmcMips70Source |
SPITZER |
70um flux |
float |
8 |
mJy |
|
|
flux8_0 |
sage_lmcIracSource |
SPITZER |
8.0um flux |
real |
4 |
mJy |
|
|
flux8_0 |
sage_smcIRACv1_5Source |
SPITZER |
8.0um IRAC (Band 1) flux |
real |
4 |
mJy |
|
|
flux_100 |
iras_psc |
IRAS |
Averaged non-color corrected 100 micron flux density |
real |
4 |
Jansky (1.0E-26 W/m**2/Hz) |
|
phot.flux.density;em.IR.60-100um |
flux_12 |
iras_psc |
IRAS |
Averaged non-color corrected 12 micron flux density |
real |
4 |
Jansky (1.0E-26 W/m**2/Hz) |
|
phot.flux.density;em.IR.8-15um |
flux_25 |
iras_psc |
IRAS |
Averaged non-color corrected 25 micron flux density |
real |
4 |
Jansky (1.0E-26 W/m**2/Hz) |
|
phot.flux.density;em.IR.15-30um |
flux_60 |
iras_psc |
IRAS |
Averaged non-color corrected 60 micron flux density |
real |
4 |
Jansky (1.0E-26 W/m**2/Hz) |
|
phot.flux.density;em.IR.30-60um |
fluxH |
sage_lmcIracSource |
SPITZER |
H band flux |
real |
4 |
mJy |
|
|
fluxH |
sage_smcIRACv1_5Source |
SPITZER |
2MASS All-Sky PSC H band flux |
real |
4 |
mJy |
|
|
fluxJ |
sage_lmcIracSource |
SPITZER |
J band flux |
real |
4 |
mJy |
|
|
fluxJ |
sage_smcIRACv1_5Source |
SPITZER |
2MASS All-Sky PSC J band flux |
real |
4 |
mJy |
|
|
fluxK |
sage_lmcIracSource |
SPITZER |
K band flux |
real |
4 |
mJy |
|
|
fluxK |
sage_smcIRACv1_5Source |
SPITZER |
2MASS All-Sky PSC K band flux |
real |
4 |
mJy |
|
|
FMAG |
grs_ngpSource, grs_ranSource, grs_sgpSource |
TWODFGRS |
Unmatched raw APM 2" profile integrated mag |
real |
4 |
|
|
|
fMaj |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
major axes derived from the elliptical Gaussian model for the source before deconvolution. |
real |
4 |
arcsec |
|
phys.angSize.smajAxis |
fMin |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
minor axes derived from the elliptical Gaussian model for the source before deconvolution. |
real |
4 |
arcsec |
|
phys.angSize.sminAxis |
focus |
twomass_scn |
TWOMASS |
Focus setting of telescope at beginning of scan. |
smallint |
2 |
|
|
instr.tel.focalLength |
focus |
twomass_sixx2_scn |
TWOMASS |
telescope focus setting |
smallint |
2 |
|
|
|
FOCUS_R |
spectra |
SIXDF |
R frame spectrograph focus value |
real |
4 |
|
|
|
FOCUS_V |
spectra |
SIXDF |
V frame spectrograph focus value |
real |
4 |
|
|
|
FootPrint_Flag |
ravedr5Source |
RAVE |
1 => in RAVE selection function footprint, 0 => outside footprint |
tinyint |
1 |
|
|
meta.code.qual |
forced |
smashdr2_source |
SMASH |
Boolean flag indicating if this is forced (ALLFRAME) photometry |
smallint |
2 |
|
|
|
fPA |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
position angle (east of north) derived from the elliptical Gaussian model for the source before deconvolution. |
real |
4 |
degrees |
|
pos.posAng |
fPeak |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
peak flux densities |
real |
4 |
mJy |
|
phot.flux.density;em.radio.750-1500MHz |
fQual_100 |
iras_psc |
IRAS |
100 micron flux density quality. |
smallint |
2 |
|
|
meta.code.qual |
fQual_12 |
iras_psc |
IRAS |
12 micron flux density quality. |
smallint |
2 |
|
|
meta.code.qual |
fQual_25 |
iras_psc |
IRAS |
25 micron flux density quality. |
smallint |
2 |
|
|
meta.code.qual |
fQual_60 |
iras_psc |
IRAS |
60 micron flux density quality. |
smallint |
2 |
|
|
meta.code.qual |
frac_c |
ravedr5Source |
RAVE |
Fraction of spectrum used [Chemical pipeline] (Note 2) |
real |
4 |
|
|
stat.value |
frame_rotator_object_type |
gaia_source |
GAIADR2 |
The type of the source mainly used for frame rotation |
int |
4 |
|
|
meta.code |
frameCode |
videoDetection |
VIDEOv20100513 |
Code for frameType of science frame from which these data were extracted |
tinyint |
1 |
|
0 |
|
Post-processing bit flag assigned to represent the frameType of the image that the detections were extracted from. Catalogues come from frames that are interleaved (leav) and stacked or simply stacked (stack). These may be filtered (filt) to remove variations in the background at certain scales. 6 VISTA pawprint stacks are typically tiled (tile) to make a 1.5 square degree tile. Pawprints or tiles may be stacked to produce deep stacks or tiles (deep) and multiple tiles may be mosaicked together to produce a mosaic (mosaic). Thus a science image may be one of several types and the catalogue data from these images may or may not be used in different curation use cases or by different users. The error bit flag allows users to select or reject different data. Bit | FrameType | | | | Decimal | Hexadecimal | | -- | NONE | 0 | 0x00000000 | 0 | leav | 1 | 0x00000001 | 1 | stack | 2 | 0x00000010 | 2 | filt | 4 | 0x00000100 | 3 | tile | 8 | 0x00001000 | 4 | deep | 16 | 0x00010000 | 5 | mosaic | 32 | 0x00100000 | Different frame types can be built up from these bit flags. E.g., a mosaicdeepstack would be 0x00110010 or 50 in decimal. A tile would always have bit 3 set to 1. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all detections in the VHS from tile frames, but not deep tile frames, include a predicate ... AND frameCode & 0x00001000 = 1 AND frameCode & 0x00010000 = 0. See the SQL Cookbook and other online pages for further information. All other frameTypes, such as normal, sky, dark, conf have frameCode=0. |
frameCode |
vvvDetection |
VVVv20100531 |
Code for frameType of science frame from which these data were extracted |
tinyint |
1 |
|
0 |
|
Post-processing bit flag assigned to represent the frameType of the image that the detections were extracted from. Catalogues come from frames that are interleaved (leav) and stacked or simply stacked (stack). These may be filtered (filt) to remove variations in the background at certain scales. 6 VISTA pawprint stacks are typically tiled (tile) to make a 1.5 square degree tile. Pawprints or tiles may be stacked to produce deep stacks or tiles (deep) and multiple tiles may be mosaicked together to produce a mosaic (mosaic). Thus a science image may be one of several types and the catalogue data from these images may or may not be used in different curation use cases or by different users. The error bit flag allows users to select or reject different data. Bit | FrameType | | | | Decimal | Hexadecimal | | -- | NONE | 0 | 0x00000000 | 0 | leav | 1 | 0x00000001 | 1 | stack | 2 | 0x00000010 | 2 | filt | 4 | 0x00000100 | 3 | tile | 8 | 0x00001000 | 4 | deep | 16 | 0x00010000 | 5 | mosaic | 32 | 0x00100000 | Different frame types can be built up from these bit flags. E.g., a mosaicdeepstack would be 0x00110010 or 50 in decimal. A tile would always have bit 3 set to 1. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all detections in the VHS from tile frames, but not deep tile frames, include a predicate ... AND frameCode & 0x00001000 = 1 AND frameCode & 0x00010000 = 0. See the SQL Cookbook and other online pages for further information. All other frameTypes, such as normal, sky, dark, conf have frameCode=0. |
frameSetID |
sharksMergeLog |
SHARKSv20210421 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
sharksMergeLog, sharksVarFrameSetInfo, sharksVariability |
SHARKSv20210222 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
sharksSource |
SHARKSv20210222 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
sharksSource |
SHARKSv20210421 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
ultravistaMergeLog, ultravistaRemeasMergeLog, ultravistaVarFrameSetInfo, ultravistaVariability |
ULTRAVISTADR4 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
ultravistaSource |
ULTRAVISTADR4 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
vhsMergeLog |
VHSDR1 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSDR2 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSDR3 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSDR4 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSDR5 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSDR6 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20120926 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20130417 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20140409 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20150108 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20160114 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20160507 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20170630 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20180419 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20201209 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20231101 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsMergeLog |
VHSv20240731 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSDR1 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSDR2 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSDR3 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSDR4 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSDR5 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSDR6 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20120926 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20130417 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20140409 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20150108 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20160114 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20160507 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20170630 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20180419 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20201209 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20231101 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSource |
VHSv20240731 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vhsSourceRemeasurement |
VHSDR1 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
videoMergeLog |
VIDEODR3 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoMergeLog |
VIDEODR4 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoMergeLog |
VIDEODR5 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoMergeLog |
VIDEOv20100513 |
frame set ID, unique over the whole WSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoMergeLog |
VIDEOv20111208 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoMergeLog, videoVarFrameSetInfo, videoVariability |
VIDEODR2 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoSource |
VIDEODR2 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoSource |
VIDEODR3 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoSource |
VIDEODR4 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoSource |
VIDEODR5 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoSource |
VIDEOv20100513 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoSource |
VIDEOv20111208 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
videoSourceRemeasurement |
VIDEOv20100513 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
vikingMergeLog |
VIKINGDR3 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog |
VIKINGDR4 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog |
VIKINGv20110714 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog |
VIKINGv20111019 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog |
VIKINGv20130417 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog |
VIKINGv20140402 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog |
VIKINGv20150421 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog |
VIKINGv20151230 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog |
VIKINGv20160406 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog |
VIKINGv20161202 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog |
VIKINGv20170715 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingMergeLog, vikingVarFrameSetInfo, vikingVariability |
VIKINGDR2 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGDR2 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGDR3 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGDR4 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGv20110714 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGv20111019 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGv20130417 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGv20140402 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGv20150421 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGv20151230 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGv20160406 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGv20161202 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSource |
VIKINGv20170715 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingSourceRemeasurement |
VIKINGv20110714 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
vikingSourceRemeasurement |
VIKINGv20111019 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20160909 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20170124 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
vmcMergeLog |
VMCDR2 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCDR3 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCDR4 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCDR5 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20110816 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20110909 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20120126 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20121128 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20130304 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20130805 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20140428 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20140903 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20150309 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20151218 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20160311 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20160822 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20170109 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20170411 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20171101 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20180702 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20181120 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20191212 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20210708 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20230816 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog |
VMCv20240226 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcMergeLog, vmcVarFrameSetInfo, vmcVariability |
VMCDR1 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcProperMotionCatalogue, vmcPsfSource |
VMCv20240226 |
frame set ID, linked to vmcMergeLog, assigned by merging procedure |
bigint |
8 |
|
|
meta.id |
frameSetID |
vmcPsfDetections |
VMCv20180702 |
frame set ID, linked to vmcMergeLog, assigned by merging procedure |
bigint |
8 |
|
|
meta.id |
frameSetID |
vmcPsfDetections |
VMCv20181120 |
frame set ID, linked to vmcMergeLog, assigned by merging procedure |
bigint |
8 |
|
|
meta.id |
frameSetID |
vmcSource |
VMCDR1 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCDR2 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCDR3 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCDR4 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCDR5 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20110816 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20110909 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20120126 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20121128 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20130304 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20130805 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20140428 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20140903 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20150309 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20151218 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20160311 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20160822 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20170109 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20170411 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20171101 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20180702 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20181120 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20191212 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20210708 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20230816 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSource |
VMCv20240226 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcSourceRemeasurement |
VMCv20110816 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
vmcSourceRemeasurement |
VMCv20110909 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
vmcdeepMergeLog |
VMCDEEPv20240506 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcdeepMergeLog, vmcdeepVarFrameSetInfo, vmcdeepVariability |
VMCDEEPv20230713 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcdeepSource |
VMCDEEPv20230713 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vmcdeepSource |
VMCDEEPv20240506 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvMergeLog |
VVVDR2 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvMergeLog |
VVVv20100531 |
frame set ID, unique over the whole WSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvMergeLog |
VVVv20110718 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvMergeLog, vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvMergeLog, vvvVarFrameSetInfo, vvvVariability |
VVVDR1 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvPsfDaophotJKsMergeLog |
VVVDR5 |
frame set ID, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvPsfDaophotJKsSource, vvvPsfDophotZYJHKsSource |
VVVDR5 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvSource |
VVVDR1 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvSource |
VVVDR2 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvSource |
VVVDR5 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvSource |
VVVv20100531 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvSource |
VVVv20110718 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.bib |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvSourceRemeasurement |
VVVv20100531 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
vvvSourceRemeasurement |
VVVv20110718 |
UID of the set of frames that this remeasured source comes from |
bigint |
8 |
|
|
meta.bib |
frameSetID |
vvvxMergeLog, vvvxVarFrameSetInfo, vvvxVariability |
VVVXDR1 |
frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
meta.id;obs.field |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetID |
vvvxSource |
VVVXDR1 |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
meta.id |
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
frameSetTolerance |
Programme |
SHARKSv20210222 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
SHARKSv20210421 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
ULTRAVISTADR4 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSDR1 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSDR2 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSDR3 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSDR4 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSDR5 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSDR6 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSv20120926 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSv20130417 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSv20150108 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSv20160114 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSv20160507 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSv20170630 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSv20180419 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSv20201209 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSv20231101 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VHSv20240731 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIDEODR2 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIDEODR3 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIDEODR4 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIDEODR5 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIDEOv20100513 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIDEOv20111208 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGDR2 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGDR3 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGDR4 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGv20110714 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGv20111019 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGv20130417 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGv20150421 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGv20151230 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGv20160406 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGv20161202 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VIKINGv20170715 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCDEEPv20230713 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCDEEPv20240506 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCDR1 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCDR3 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCDR4 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCDR5 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20110816 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20110909 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20120126 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20121128 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20130304 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20130805 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20140428 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20140903 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20150309 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20151218 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20160311 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20160822 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20170109 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20170411 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20171101 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20180702 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20181120 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20191212 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20210708 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20230816 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VMCv20240226 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VSAQC |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VVVDR1 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VVVDR2 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VVVDR5 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VVVXDR1 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VVVv20100531 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameSetTolerance |
Programme |
VVVv20110718 |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
frameType |
Multiframe |
SHARKSv20210222 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
SHARKSv20210421 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
ULTRAVISTADR4 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSDR1 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSDR2 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSDR3 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSDR4 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSDR5 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSDR6 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20120926 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20130417 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20140409 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20150108 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20160114 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20160507 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20170630 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20180419 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20201209 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20231101 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VHSv20240731 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIDEODR2 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIDEODR3 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIDEODR4 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIDEODR5 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIDEOv20100513 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIDEOv20111208 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGDR2 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGDR3 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGDR4 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGv20110714 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGv20111019 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGv20130417 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGv20140402 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGv20150421 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGv20151230 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGv20160406 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGv20161202 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VIKINGv20170715 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCDEEPv20230713 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCDEEPv20240506 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCDR1 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCDR2 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCDR3 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCDR4 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCDR5 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20110816 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20110909 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20120126 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20121128 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20130304 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20130805 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20140428 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20140903 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20150309 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20151218 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20160311 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20160822 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20170109 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20170411 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20171101 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20180702 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20181120 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20191212 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20210708 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20230816 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VMCv20240226 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VVVDR1 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VVVDR2 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VVVDR5 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VVVXDR1 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VVVv20100531 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
Multiframe |
VVVv20110718 |
The type of multiframe (e.g. stack|tile|mosaic etc.) A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are: confidence = "conf" | dark = "dark" | deep = "deep" | difference = "diff" | filtered = "filt" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | sky = "sky" | stack = "stack" | default value = "normal" | |
frameType |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
The type of multiframe (e.g. stack|tile|mosaic etc.) |
varchar |
64 |
|
normal |
meta.code.class |
freqLSG |
vvvVivaCatalogue |
VVVDR5 |
main variability frequency using Lomb-Scargle generalized method {catalogue TType keyword: FreqLSG} |
float |
8 |
days^{-1} |
-9.999995e8 |
|
freqPDM |
vvvVivaCatalogue |
VVVDR5 |
Main variability frequency using Phase Dispersion Minimization method {catalogue TType keyword: FreqPDM} |
float |
8 |
days^{-1} |
-9.999995e8 |
|
freqPKfi2 |
vvvVivaCatalogue |
VVVDR5 |
Main variability frequency using flux independent period method {catalogue TType keyword: FreqPKfi2} |
float |
8 |
days^{-1} |
-9.999995e8 |
|
freqPLfi2 |
vvvVivaCatalogue |
VVVDR5 |
Main variability frequency using panchromatic period method {catalogue TType keyword: FreqPLfi2} |
float |
8 |
days^{-1} |
-9.999995e8 |
|
freqSTR |
vvvVivaCatalogue |
VVVDR5 |
Main variability frequency using String Length Method method {catalogue TType keyword: FreqSTR} |
float |
8 |
days^{-1} |
-9.999995e8 |
|
frinID |
Multiframe |
SHARKSv20210222 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
SHARKSv20210421 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
ULTRAVISTADR4 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSDR1 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSDR2 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSDR3 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSDR4 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSDR5 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSDR6 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20120926 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20130417 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20140409 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20150108 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20160114 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20160507 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20170630 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20180419 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20201209 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20231101 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VHSv20240731 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIDEODR2 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIDEODR3 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIDEODR4 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIDEODR5 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIDEOv20100513 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIDEOv20111208 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGDR2 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGDR3 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGDR4 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGv20110714 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGv20111019 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGv20130417 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGv20140402 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGv20150421 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGv20151230 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGv20160406 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGv20161202 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VIKINGv20170715 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCDEEPv20230713 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCDEEPv20240506 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCDR1 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCDR2 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCDR3 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCDR4 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCDR5 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20110816 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20110909 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20120126 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20121128 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20130304 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20130805 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20140428 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20140903 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20150309 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20151218 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20160311 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20160822 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20170109 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20170411 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20171101 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20180702 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20181120 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20191212 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20210708 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20230816 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VMCv20240226 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VVVDR1 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VVVDR2 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VVVDR5 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VVVXDR1 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VVVv20100531 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
Multiframe |
VVVv20110718 |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
frinID |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
obs.field |
fromAllSky |
twompzPhotoz |
TWOMPZ |
Is the WISE designation from the wise_allskysc catalogue 0 NO/1 YES |
tinyint |
1 |
|
0 |
|
fromAllSky |
wiseScosPhotoz, wiseScosPhotozRejects, wiseScosSvm |
WISExSCOSPZ |
Is the WISE designation from the wise_allskysc catalogue 0 NO/1 YES {image primary HDU keyword: fromAllSky} |
tinyint |
1 |
|
0 |
|
FWHM_IMAGE |
mgcDetection |
MGC |
FWHM assuming a gaussian core |
real |
4 |
pixel |
|
|