D |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
D_MODULUS |
mgcGalaxyStruct |
MGC |
B proper distance to the object (h=1) |
real |
4 |
Mpc |
|
|
darkID |
Multiframe |
SHARKSv20210222 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
SHARKSv20210421 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
ULTRAVISTADR4 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSDR1 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSDR2 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSDR3 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSDR4 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSDR5 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSDR6 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20120926 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20130417 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20140409 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20150108 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20160114 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20160507 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20170630 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20180419 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20201209 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20231101 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VHSv20240731 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIDEODR2 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIDEODR3 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIDEODR4 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIDEODR5 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIDEOv20100513 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIDEOv20111208 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGDR2 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGDR3 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGDR4 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGv20110714 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGv20111019 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGv20130417 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGv20140402 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGv20150421 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGv20151230 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGv20160406 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGv20161202 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VIKINGv20170715 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCDEEPv20230713 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCDEEPv20240506 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCDR1 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCDR2 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCDR3 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCDR4 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCDR5 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20110816 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20110909 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20120126 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20121128 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20130304 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20130805 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20140428 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20140903 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20150309 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20151218 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20160311 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20160822 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20170109 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20170411 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20171101 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20180702 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20181120 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20191212 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20210708 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20230816 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VMCv20240226 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VVVDR1 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VVVDR2 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VVVDR5 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VVVXDR1 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VVVv20100531 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
Multiframe |
VVVv20110718 |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
darkID |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
UID of library calibration dark frame |
bigint |
8 |
|
-99999999 |
obs.field |
databaseName |
ExternalSurvey |
SHARKSv20210222 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
SHARKSv20210421 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
ULTRAVISTADR4 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSDR1 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSDR2 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSDR3 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSDR4 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSDR5 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSDR6 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSv20120926 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSv20130417 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSv20150108 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSv20160114 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSv20160507 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSv20170630 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSv20180419 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSv20201209 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSv20231101 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VHSv20240731 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIDEODR2 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIDEODR3 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIDEODR4 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIDEODR5 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIDEOv20100513 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIDEOv20111208 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGDR2 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGDR3 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGDR4 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGv20110714 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGv20111019 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGv20130417 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGv20150421 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGv20151230 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGv20160406 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGv20161202 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VIKINGv20170715 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCDEEPv20230713 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCDEEPv20240506 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCDR1 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCDR3 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCDR4 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCDR5 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20110816 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20110909 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20120126 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20121128 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20130304 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20130805 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20140428 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20140903 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20150309 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20151218 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20160311 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20160822 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20170109 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20170411 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20171101 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20180702 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20181120 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20191212 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20210708 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20230816 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VMCv20240226 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VSAQC |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VVVDR1 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VVVDR2 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VVVDR5 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VVVXDR1 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VVVv20100531 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
databaseName |
ExternalSurvey |
VVVv20110718 |
The name of the database within the VSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
dataScale |
MultiframeDetector |
SHARKSv20210222 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
SHARKSv20210421 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
ULTRAVISTADR4 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSDR1 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSDR2 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSDR3 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSDR4 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSDR5 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSDR6 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20120926 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20130417 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20140409 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20150108 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20160114 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20160507 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20170630 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20180419 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20201209 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20231101 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VHSv20240731 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIDEODR2 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIDEODR3 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIDEODR4 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIDEODR5 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIDEOv20100513 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIDEOv20111208 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGDR2 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGDR3 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGDR4 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGv20110714 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGv20111019 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGv20130417 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGv20140402 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGv20150421 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGv20151230 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGv20160406 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGv20161202 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VIKINGv20170715 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCDEEPv20230713 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCDEEPv20240506 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCDR1 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCDR2 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCDR3 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCDR4 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCDR5 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20110816 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20110909 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20120126 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20121128 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20130304 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20130805 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20140428 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20140903 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20150309 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20151218 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20160311 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20160822 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20170109 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20170411 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20171101 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20180702 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20181120 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20191212 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20210708 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20230816 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VMCv20240226 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VVVDR1 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VVVDR2 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VVVDR5 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VVVXDR1 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VVVv20100531 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
MultiframeDetector |
VVVv20110718 |
Scale factor {image extension keyword: BSCALE} |
real |
4 |
|
-0.9999995e9 |
|
dataScale |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Scale factor |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
SHARKSv20210222 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
SHARKSv20210421 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
ULTRAVISTADR4 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSDR1 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSDR2 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSDR3 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSDR4 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSDR5 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSDR6 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20120926 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20130417 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20140409 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20150108 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20160114 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20160507 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20170630 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20180419 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20201209 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20231101 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VHSv20240731 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIDEODR2 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIDEODR3 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIDEODR4 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIDEODR5 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIDEOv20100513 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIDEOv20111208 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGDR2 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGDR3 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGDR4 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGv20110714 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGv20111019 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGv20130417 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGv20140402 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGv20150421 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGv20151230 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGv20160406 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGv20161202 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VIKINGv20170715 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCDEEPv20230713 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCDEEPv20240506 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCDR1 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCDR2 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCDR3 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCDR4 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCDR5 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20110816 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20110909 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20120126 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20121128 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20130304 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20130805 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20140428 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20140903 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20150309 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20151218 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20160311 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20160822 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20170109 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20170411 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20171101 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20180702 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20181120 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20191212 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20210708 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20230816 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VMCv20240226 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VVVDR1 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VVVDR2 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VVVDR5 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VVVXDR1 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VVVv20100531 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
MultiframeDetector |
VVVv20110718 |
Offset factor {image extension keyword: BZERO} |
real |
4 |
|
-0.9999995e9 |
|
dataZero |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Offset factor |
real |
4 |
|
-0.9999995e9 |
|
date |
twomass_psc, twomass_xsc |
TWOMASS |
The observation reference date for this source expressed in ISO standard format. (YYYY-MM-DD) |
datetime |
8 |
yyyy-mm-dd |
|
time.epoch |
date |
twomass_scn |
TWOMASS |
The observation reference date for this scan expressed in ISO standard format. (YYYY-MM-DD) |
datetime |
8 |
yyyy-mm-dd |
|
time.epoch |
date |
twomass_sixx2_scn |
TWOMASS |
observation date |
datetime |
8 |
yyyy-mm-dd |
|
|
dateObs |
Multiframe |
SHARKSv20210222 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
SHARKSv20210421 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
ULTRAVISTADR4 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSDR1 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSDR2 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSDR3 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSDR4 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSDR5 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSDR6 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20120926 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20130417 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20140409 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20150108 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20160114 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20160507 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20170630 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20180419 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20201209 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20231101 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VHSv20240731 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIDEODR2 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIDEODR3 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIDEODR4 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIDEODR5 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIDEOv20100513 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIDEOv20111208 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGDR2 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGDR3 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGDR4 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGv20110714 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGv20111019 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGv20130417 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGv20140402 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGv20150421 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGv20151230 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGv20160406 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGv20161202 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VIKINGv20170715 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCDEEPv20230713 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCDEEPv20240506 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCDR1 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCDR2 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCDR3 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCDR4 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCDR5 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20110816 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20110909 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20120126 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20121128 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20130304 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20130805 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20140428 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20140903 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20150309 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20151218 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20160311 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20160822 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20170109 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20170411 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20171101 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20180702 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20181120 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20191212 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20210708 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20230816 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VMCv20240226 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VVVDR1 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VVVDR2 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VVVDR5 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VVVXDR1 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VVVv20100531 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
VVVv20110718 |
Observing date {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Observing date |
datetime |
8 |
|
12-31-9999 |
time.epoch |
dbName |
Release |
SHARKSv20210222 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
SHARKSv20210421 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
ULTRAVISTADR4 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSDR1 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSDR2 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSDR3 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSDR4 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSDR5 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSDR6 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSv20120926 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSv20130417 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSv20150108 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSv20160114 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSv20160507 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSv20170630 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSv20180419 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSv20201209 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSv20231101 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VHSv20240731 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIDEODR2 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIDEODR3 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIDEODR4 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIDEODR5 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIDEOv20100513 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIDEOv20111208 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGDR2 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGDR3 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGDR4 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGZYSELJv20160909 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGZYSELJv20170124 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGv20110714 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGv20111019 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGv20130417 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGv20150421 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGv20151230 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGv20160406 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGv20161202 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VIKINGv20170715 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCDEEPv20230713 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCDEEPv20240506 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCDR1 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCDR3 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCDR4 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCDR5 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20110816 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20110909 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20120126 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20121128 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20130304 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20130805 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20140428 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20140903 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20150309 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20151218 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20160311 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20160822 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20170109 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20170411 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20171101 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20180702 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20181120 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20191212 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20210708 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20230816 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VMCv20240226 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VVVDR1 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VVVDR2 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VVVDR5 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VVVXDR1 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VVVv20100531 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
VVVv20110718 |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbNamePrefix |
Survey |
SHARKSv20210222 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
SHARKSv20210421 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
ULTRAVISTADR4 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSDR1 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSDR2 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSDR3 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSDR4 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSDR5 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSDR6 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSv20120926 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSv20130417 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSv20150108 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSv20160114 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSv20160507 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSv20170630 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSv20180419 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSv20201209 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSv20231101 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VHSv20240731 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIDEODR2 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIDEODR3 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIDEODR4 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIDEODR5 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIDEOv20100513 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIDEOv20111208 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGDR2 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGDR3 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGDR4 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGv20110714 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGv20111019 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGv20130417 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGv20150421 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGv20151230 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGv20160406 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGv20161202 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VIKINGv20170715 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCDEEPv20230713 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCDEEPv20240506 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCDR1 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCDR3 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCDR4 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCDR5 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20110816 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20110909 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20120126 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20121128 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20130304 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20130805 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20140428 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20140903 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20150309 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20151218 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20160311 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20160822 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20170109 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20170411 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20171101 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20180702 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20181120 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20191212 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20210708 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20230816 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VMCv20240226 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VSAQC |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VVVDR1 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VVVDR2 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VVVDR5 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VVVXDR1 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VVVv20100531 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
VVVv20110718 |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
ddec |
sage_lmcIracSource, sage_lmcMips160Source, sage_lmcMips24Source, sage_lmcMips70Source, sage_smcIRACv1_5Source |
SPITZER |
Error in declination |
float |
8 |
arcseconds |
|
|
de_deg |
tycho2 |
GAIADR1 |
Observed Tycho2 Declination in ICRS |
float |
8 |
degrees |
|
pos.eq.dec |
de_m_deg |
tycho2 |
GAIADR1 |
Mean Declination, ICRS, epoch = J2000 |
float |
8 |
degrees |
|
pos.eq.dec |
de_rad |
hipparcos_new_reduction |
GAIADR1 |
Declination in the ICRS at epoch 1991.25 |
float |
8 |
radians |
|
pos.eq.dec |
DE_TGAS |
ravedr5Source |
RAVE |
TGAS Declination (epocflag= 2015) |
float |
8 |
deg |
|
pos.eq.dec |
DEC |
agntwomass, denisi, denisj, durukst, fsc, hes, hipass, nvss, rass, shapley, sumss, supercos, twomass |
SIXDF |
Dec J2000 |
float |
8 |
degrees |
|
|
DEC |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Declination J2000 |
float |
8 |
degrees |
|
|
DEC |
target |
SIXDF |
master Dec J2000 (decimal degrees) |
float |
8 |
degrees |
|
|
DEC |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Corrected Declination of the detection in degrees (J2000) after statistical correlation of the emldetect coordinates, RA_UNC and DEC_UNC, with the USNO B1.0 optical source catalogue using the SAS task eposcorr. In case where the cross-correlation is determined to be unreliable no correction is applied and this value is therefore the same as DEC_UNC. |
float |
8 |
degrees |
|
|
dec |
Detection |
PS1DR2 |
Declination. |
float |
8 |
degrees |
-999 |
|
dec |
MapApertureIDsultraVistaMapLc, MapApertureIDsultravistaDual, ultravistaMergeLog, ultravistaRemeasMergeLog, ultravistaTileSet |
ULTRAVISTADR4 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
MapApertureIDsvikingZY_selJ |
VIKINGZYSELJv20170124 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
MapApertureIDsvikingZY_selJ, vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20160909 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
SHARKSv20210421 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
ULTRAVISTADR4 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSDR1 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSDR2 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSDR3 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSDR4 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSDR5 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSDR6 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSv20120926 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSv20130417 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSv20150108 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSv20160114 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSv20160507 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSv20170630 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSv20180419 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSv20201209 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSv20231101 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VHSv20240731 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIDEODR2 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIDEODR3 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIDEODR4 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIDEODR5 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIDEOv20100513 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIDEOv20111208 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGDR2 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGDR3 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGDR4 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGv20110714 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGv20111019 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGv20130417 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGv20150421 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGv20151230 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGv20160406 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGv20161202 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VIKINGv20170715 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCDEEPv20230713 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCDEEPv20240506 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCDR1 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCDR3 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCDR4 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCDR5 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20110816 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20110909 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20120126 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20121128 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20130304 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20130805 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20140428 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20140903 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20150309 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20151218 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20160311 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20160822 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20170109 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20170411 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20171101 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20180702 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20181120 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20191212 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20210708 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20230816 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VMCv20240226 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VVVDR1 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VVVDR2 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VVVDR5 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VVVXDR1 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VVVv20100531 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic |
VVVv20110718 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredMosaic, RequiredRegion |
SHARKSv20210222 |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
SHARKSv20210421 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
ULTRAVISTADR4 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSDR1 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSDR2 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSDR3 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSDR4 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSDR5 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSDR6 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSv20120926 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSv20130417 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSv20150108 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSv20160114 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSv20160507 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSv20170630 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSv20180419 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSv20201209 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSv20231101 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VHSv20240731 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIDEODR2 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIDEODR3 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIDEODR4 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIDEODR5 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIDEOv20100513 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIDEOv20111208 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGDR2 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGDR3 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGDR4 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGv20110714 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGv20111019 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGv20130417 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGv20150421 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGv20151230 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGv20160406 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGv20161202 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VIKINGv20170715 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCDEEPv20230713 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCDEEPv20240506 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCDR1 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCDR3 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCDR4 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCDR5 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20110816 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20110909 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20120126 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20121128 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20130304 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20130805 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20140428 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20140903 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20150309 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20151218 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20160311 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20160822 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20170109 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20170411 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20171101 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20180702 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20181120 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20191212 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20210708 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20230816 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VMCv20240226 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VSAQC |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VVVDR1 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VVVDR2 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VVVDR5 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VVVXDR1 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VVVv20100531 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack |
VVVv20110718 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
RequiredStack, RequiredTile |
SHARKSv20210222 |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
allwise_sc |
WISE |
J2000 declination with respect to the 2MASS PSC reference frame from the non-moving source extraction. |
float |
8 |
deg |
|
|
dec |
aux_qso_icrf2_match, gaia_source, tgas_source |
GAIADR1 |
Celestial Declination |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
catwise_2020 |
WISE |
declination (ICRS) |
float |
8 |
deg |
|
|
dec |
catwise_prelim |
WISE |
declination (J2000) |
float |
8 |
deg |
|
|
dec |
combo17CDFSSource |
COMBO17 |
J2000 declination with respect to the ICRS |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
decapsSource |
DECAPS |
Declination (degrees) {catalogue TType keyword: dec} |
float |
8 |
Degrees |
-999999500.0 |
pos.eq.dec;meta.main |
dec |
eros2LMCSource, eros2SMCSource, erosLMCSource, erosSMCSource |
EROS |
J2000 declination |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
J2000 Celestial Declination |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca, glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Declination (J2000) |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
grs_ngpSource, grs_ranSource, grs_sgpSource |
TWODFGRS |
Dec. (B1950) in DD MM SS.S |
float |
8 |
|
|
|
dec |
hipparcos_new_reduction |
GAIADR1 |
Declination in the ICRS at epoch 1991.25 |
float |
8 |
degrees |
|
meta.main;pos.eq.dec |
dec |
igsl_source |
GAIADR1 |
Celestial Declination at catalogue epoch |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
iras_psc |
IRAS |
J2000 Celestial Declination |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
machoLMCSource, machoSMCSource |
MACHO |
J2000 declination |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
mcps_lmcSource, mcps_smcSource |
MCPS |
J2000 declination |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
mgcDetection |
MGC |
Object declination (J2000) |
float |
8 |
deg |
|
|
dec |
nvssSource |
NVSS |
J2000 Celestial Declination |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
ogle3LpvLmcSource, ogle3LpvSmcSource, ogle4CepLmcSource, ogle4CepSmcSource, ogle4RRLyrLmcSource, ogle4RRLyrSmcSource |
OGLE |
J2000 Celestial Declination |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
rosat_bsc, rosat_fsc |
ROSAT |
Declination (decimal degrees; J2000) |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
sage_lmcIracSource, sage_lmcMips160Source, sage_lmcMips24Source, sage_lmcMips70Source, sage_smcIRACv1_5Source |
SPITZER |
Declination (J2000) |
float |
8 |
deg |
|
|
dec |
sharksDetection |
SHARKSv20210421 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
sharksDetection, sharksSource, sharksTilePawPrints |
SHARKSv20210222 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
sharksMergeLog |
SHARKSv20210421 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
sharksMergeLog, sharksTileSet |
SHARKSv20210222 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
sharksTilePawTDOnly |
SHARKSv20210222 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
sharksTilePawTDOnly |
SHARKSv20210421 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
sharksVariability |
SHARKSv20210222 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
sharksVariability |
SHARKSv20210421 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
smashdr2_deep, smashdr2_object |
SMASH |
Declination (J2000.0) of source, in degrees |
float |
8 |
|
|
|
dec |
smashdr2_source |
SMASH |
Declination (J2000.0) of source |
float |
8 |
degrees |
|
|
dec |
spitzer_smcSource |
SPITZER |
J2000 declination |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
twomass_psc |
TWOMASS |
J2000 declination with respect to the ICRS |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
twomass_scn |
TWOMASS |
Declination of scan center for equinox J2000. |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
twomass_sixx2_psc |
TWOMASS |
declination (J2000 decimal deg) |
float |
8 |
deg |
|
|
dec |
twomass_sixx2_scn |
TWOMASS |
declination (J2000 decimal deg) of scan center |
float |
8 |
deg |
|
|
dec |
twomass_sixx2_xsc |
TWOMASS |
declination (J2000 decimal deg) based on peak pixel |
float |
8 |
deg |
|
|
dec |
twomass_xsc |
TWOMASS |
Declination (J2000 decimal deg) based on peak pixel. |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
twompzPhotoz |
TWOMPZ |
Dec. (J2000) based on the peak pixel {image primary HDU keyword: DEJ2000} |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
tycho2 |
GAIADR1 |
Observed Tycho2 Declination in ICRS |
float |
8 |
degrees |
|
meta.main;pos.eq.dec |
dec |
ukirtFSstars |
VIDEOv20100513 |
Declination of star at Equinox J2000.0 |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
ukirtFSstars |
VIKINGv20110714 |
Declination of star at Equinox J2000.0 |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
ukirtFSstars |
VVVv20100531 |
Declination of star at Equinox J2000.0 |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
ultravistaDetection, ultravistaMapRemeasurement, ultravistaSource, ultravistaTilePawPrints |
ULTRAVISTADR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Celestial Declination of aperture |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
ultravistaTilePawTDOnly |
ULTRAVISTADR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
ultravistaVariability |
ULTRAVISTADR4 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vhsDetection |
VHSDR3 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSDR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSDR5 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSDR6 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20120926 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20130417 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20140409 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20150108 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20160114 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20160507 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20170630 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20180419 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20201209 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20231101 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection |
VHSv20240731 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection, vhsListRemeasurement, vhsSource, vhsSourceRemeasurement, vhsTilePawPrints |
VHSDR1 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsDetection, vhsTilePawPrints |
VHSDR2 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vhsMergeLog |
VHSDR2 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSDR3 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSDR4 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSDR5 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSDR6 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20120926 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20130417 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20140409 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20150108 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20160114 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20160507 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20170630 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20180419 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20201209 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20231101 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog |
VHSv20240731 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsMergeLog, vhsTileSet |
VHSDR1 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSDR1 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSDR2 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSDR3 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSDR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSDR5 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSDR6 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20120926 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20130417 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20140409 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20150108 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20160114 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20160507 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20170630 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20180419 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20201209 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20231101 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vhsTilePawTDOnly |
VHSv20240731 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
videoDetection |
VIDEODR3 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
videoDetection |
VIDEODR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
videoDetection |
VIDEODR5 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
videoDetection |
VIDEOv20111208 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
videoDetection, videoListRemeasurement, videoSourceRemeasurement |
VIDEOv20100513 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
videoDetection, videoSource, videoTilePawPrints |
VIDEODR2 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
videoMergeLog |
VIDEODR3 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
videoMergeLog |
VIDEODR4 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
videoMergeLog |
VIDEODR5 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
videoMergeLog |
VIDEOv20100513 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
videoMergeLog |
VIDEOv20111208 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
videoMergeLog, videoTileSet |
VIDEODR2 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
videoTilePawTDOnly |
VIDEODR2 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
videoTilePawTDOnly |
VIDEODR3 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
videoTilePawTDOnly |
VIDEODR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
videoTilePawTDOnly |
VIDEODR5 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
videoTilePawTDOnly |
VIDEOv20111208 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
videoVariability |
VIDEODR2 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
videoVariability |
VIDEODR3 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
videoVariability |
VIDEODR4 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
videoVariability |
VIDEODR5 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
videoVariability |
VIDEOv20100513 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
videoVariability |
VIDEOv20111208 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingDetection |
VIKINGDR3 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection |
VIKINGDR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection |
VIKINGv20111019 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection |
VIKINGv20130417 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection |
VIKINGv20140402 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection |
VIKINGv20150421 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection |
VIKINGv20151230 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection |
VIKINGv20160406 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection |
VIKINGv20161202 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection |
VIKINGv20170715 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection, vikingListRemeasurement, vikingSourceRemeasurement |
VIKINGv20110714 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingDetection, vikingSource, vikingTilePawPrints |
VIKINGDR2 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingMergeLog |
VIKINGDR3 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog |
VIKINGDR4 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog |
VIKINGv20110714 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog |
VIKINGv20111019 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog |
VIKINGv20130417 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog |
VIKINGv20140402 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog |
VIKINGv20150421 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog |
VIKINGv20151230 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog |
VIKINGv20160406 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog |
VIKINGv20161202 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog |
VIKINGv20170715 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingMergeLog, vikingTileSet |
VIKINGDR2 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGDR2 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGDR3 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGDR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGv20111019 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGv20130417 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGv20140402 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGv20150421 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGv20151230 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGv20160406 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGv20161202 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingTilePawTDOnly |
VIKINGv20170715 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vikingVariability |
VIKINGDR2 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGDR3 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGDR4 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGv20110714 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGv20111019 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGv20130417 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGv20140402 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGv20150421 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGv20151230 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGv20160406 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGv20161202 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingVariability |
VIKINGv20170715 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
Celestial Declination of aperture |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
Celestial Declination of aperture |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcCepheidVariables |
VMCDR3 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcCepheidVariables |
VMCv20121128 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcCepheidVariables |
VMCv20140428 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcCepheidVariables |
VMCv20140903 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcCepheidVariables |
VMCv20150309 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcCepheidVariables |
VMCv20151218 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcCepheidVariables |
VMCv20160311 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcCepheidVariables |
VMCv20160822 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcCepheidVariables |
VMCv20170109 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcCepheidVariables |
VMCv20170411 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcCepheidVariables |
VMCv20171101 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcCepheidVariables |
VMCv20180702 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcCepheidVariables |
VMCv20181120 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcCepheidVariables |
VMCv20191212 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcCepheidVariables |
VMCv20210708 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcCepheidVariables |
VMCv20230816 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcCepheidVariables |
VMCv20240226 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcCepheidVariables, vmcEclipsingBinaryVariables, vmcRRlyraeVariables |
VMCDR4 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcDetection |
VMCDR2 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCDR3 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCDR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCDR5 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20110909 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20120126 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20121128 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20130304 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20130805 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20140428 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20140903 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20150309 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20151218 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20160311 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20160822 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20170109 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20170411 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20171101 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20180702 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20181120 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20191212 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20210708 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20230816 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection |
VMCv20240226 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection, vmcListRemeasurement, vmcSourceRemeasurement |
VMCv20110816 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcDetection, vmcSource, vmcSynopticSource, vmcTilePawPrints |
VMCDR1 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcMLClassificationCatalogue |
VMCv20240226 |
DEC in degrees (J2000) from the VMC catalogue {catalogue TType keyword: VMC_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCDR2 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCDR3 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCDR4 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCDR5 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20110816 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20110909 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20120126 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20121128 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20130304 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20130805 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20140428 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20140903 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20150309 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20151218 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20160311 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20160822 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20170109 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20170411 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20171101 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20180702 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20181120 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20191212 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20210708 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20230816 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog |
VMCv20240226 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcMergeLog, vmcSynopticMergeLog, vmcTileSet |
VMCDR1 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcPointings |
VMCDR4 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCDR5 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20160311 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20160822 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20170109 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20170411 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20171101 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20180702 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20181120 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20191212 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20210708 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20230816 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcPointings |
VMCv20240226 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vmcProperMotionCatalogue |
VMCv20240226 |
Average celestial Declination of source from VMC PSF catalogue {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcPsfCatalogue |
VMCDR3 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcPsfCatalogue |
VMCDR4 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcPsfCatalogue |
VMCv20121128 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcPsfCatalogue |
VMCv20140428 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcPsfCatalogue |
VMCv20140903 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec |
dec |
vmcPsfCatalogue |
VMCv20150309 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcPsfCatalogue |
VMCv20151218 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcPsfCatalogue |
VMCv20160311 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcPsfCatalogue |
VMCv20160822 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcPsfCatalogue |
VMCv20170109 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcPsfCatalogue |
VMCv20170411 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcPsfCatalogue |
VMCv20171101 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcPsfDetections |
VMCv20181120 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcPsfDetections, vmcPsfSource |
VMCv20180702 |
PSF Y,J,Ks average Dec centre (main) {catalogue TType keyword: AVERAGE_DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcRRLyraeVariables |
VMCv20240226 |
Celestial Declination from VMC {catalogue TType keyword: DEC} |
float |
8 |
deg |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCDR1 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCDR2 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCDR3 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCDR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCDR5 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20110816 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20110909 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20120126 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20121128 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20130304 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20130805 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20140428 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20140903 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20150309 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20151218 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20160311 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20160822 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20170109 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20170411 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20171101 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20180702 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20181120 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20191212 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20210708 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20230816 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcTilePawTDOnly |
VMCv20240226 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcVariability |
VMCDR1 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCDR2 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCDR3 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCDR4 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCDR5 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20110816 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20110909 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20120126 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20121128 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20130304 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20130805 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20140428 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20140903 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20150309 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20151218 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20160311 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20160822 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20170109 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20170411 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20171101 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20180702 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20181120 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20191212 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20210708 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20230816 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariability |
VMCv20240226 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcVariablesType |
VMCDR3 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec |
dec |
vmcVariablesType |
VMCDR4 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec |
dec |
vmcVariablesType |
VMCv20121128 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec |
dec |
vmcVariablesType |
VMCv20140428 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec |
dec |
vmcVariablesType |
VMCv20140903 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec |
dec |
vmcVariablesType |
VMCv20150309 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec |
dec |
vmcVariablesType |
VMCv20151218 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec |
dec |
vmcVariablesType |
VMCv20160311 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec |
dec |
vmcVariablesType |
VMCv20160822 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec |
dec |
vmcVariablesType |
VMCv20170109 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec |
dec |
vmcVariablesType |
VMCv20170411 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcVariablesType |
VMCv20171101 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcVariablesType |
VMCv20180702 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcVariablesType |
VMCv20181120 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcVariablesType |
VMCv20191212 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcVariablesType |
VMCv20210708 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcVariablesType |
VMCv20230816 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcVariablesType |
VMCv20240226 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcdeepDetection |
VMCDEEPv20240506 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcdeepDetection, vmcdeepSource, vmcdeepSynopticSource, vmcdeepTilePawPrints |
VMCDEEPv20230713 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vmcdeepMergeLog |
VMCDEEPv20240506 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcdeepMergeLog, vmcdeepSynopticMergeLog, vmcdeepTileSet |
VMCDEEPv20230713 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vmcdeepTilePawTDOnly |
VMCDEEPv20230713 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcdeepTilePawTDOnly |
VMCDEEPv20240506 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vmcdeepVariability |
VMCDEEPv20230713 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vmcdeepVariability |
VMCDEEPv20240506 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vvvBulgeExtMapCoords |
EXTINCT |
Celestial Declination of pixel |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vvvDetection |
VVVDR2 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vvvDetection, vvvListRemeasurement, vvvSourceRemeasurement |
VVVv20100531 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vvvDetection, vvvSource, vvvSynopticSource, vvvTilePawPrints |
VVVDR1 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vvvMergeLog |
VVVDR2 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vvvMergeLog |
VVVv20100531 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vvvMergeLog |
VVVv20110718 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vvvMergeLog, vvvPsfDaophotJKsMergeLog, vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vvvMergeLog, vvvSynopticMergeLog, vvvTileSet |
VVVDR1 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Right Ascension and Declination are products of the astrometric fit, {catalogue TType keyword: de} |
float |
8 |
|
-999999500.0 |
pos.eq.dec;meta.main |
dec |
vvvPointings |
VVVDR5 |
Pointing centre |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
dec |
vvvPsfDaophotJKsSource |
VVVDR5 |
Celestial Declination {catalogue TType keyword: DEC} |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vvvPsfDophotZYJHKsSource |
VVVDR5 |
Celestial Declination, epoch 1 {catalogue TType keyword: dec} |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
vvvTilePawTDOnly |
VVVDR1 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vvvTilePawTDOnly |
VVVDR2 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vvvTilePawTDOnly |
VVVDR5 |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
vvvVariability |
VVVDR1 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vvvVariability |
VVVDR2 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vvvVariability |
VVVDR5 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vvvVariability |
VVVv20100531 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vvvVariability |
VVVv20110718 |
Mean Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
vvvVivaCatalogue |
VVVDR5 |
Right Ascension and Declination are products of the astrometric fit, {catalogue TType keyword: decJ2000} |
float |
8 |
|
-999999500.0 |
pos.eq.dec;meta.main |
dec |
wiseScosPhotoz, wiseScosPhotozRejects, wiseScosSvm |
WISExSCOSPZ |
Dec. (J2000) from WISE {image primary HDU keyword: dec_WISE} |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
dec |
wise_allskysc |
WISE |
J2000 declination with respect to the 2MASS PSC reference frame. |
float |
8 |
degrees |
|
|
dec |
wise_prelimsc |
WISE |
J2000 declination with respect to the 2MASS PSC reference frame CAUTION: Approximately 20% of sources fainter than W1~14.5 mag in the Preliminary Release Source Catalog suffer from a source extraction software error that resulted in their declinations being offset between 0.2 and 1.0 arcsec from the true position |
float |
8 |
degrees |
|
|
dec_1 |
twomass_scn |
TWOMASS |
J2000 declination of the eastern corner at start of scan. |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec_1 |
twomass_sixx2_scn |
TWOMASS |
declination (J2000 decimal deg) of scan corner 1 |
float |
8 |
deg |
|
|
dec_2 |
twomass_scn |
TWOMASS |
J2000 declination of the western corner at start of scan. |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec_2 |
twomass_sixx2_scn |
TWOMASS |
declination (J2000 decimal deg) of scan corner 2 |
float |
8 |
deg |
|
|
dec_3 |
twomass_scn |
TWOMASS |
J2000 declination of the eastern corner at end of scan. |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec_3 |
twomass_sixx2_scn |
TWOMASS |
declination (J2000 decimal deg) of scan corner 3 |
float |
8 |
deg |
|
|
dec_4 |
twomass_scn |
TWOMASS |
J2000 declination of the western corner at end of scan. |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec_4 |
twomass_sixx2_scn |
TWOMASS |
declination (J2000 decimal deg) of scan corner 4 |
float |
8 |
deg |
|
|
dec_epoch |
igsl_source |
GAIADR1 |
Mean Epoch of Declination |
real |
4 |
years |
|
time.epoch |
dec_err |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca, glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Error in Declination |
float |
8 |
arcsec |
|
stat.error |
dec_error |
aux_qso_icrf2_match |
GAIADR1 |
Uncertainty on celestial Declination |
float |
8 |
milliarcseconds |
|
stat.error;pos.eq.dec |
dec_error |
gaia_source |
GAIADR2 |
Standard error of Declination |
float |
8 |
milliarcsec |
|
stat.error;pos.eq.dec |
dec_error |
gaia_source |
GAIAEDR3 |
Standard error of Declination |
float |
8 |
milliarcsec |
|
stat.error;pos.eq.dec |
dec_error |
gaia_source, tgas_source |
GAIADR1 |
Standard error of Declination |
float |
8 |
milliarcsec |
|
stat.error;pos.eq.dec |
dec_error |
igsl_source |
GAIADR1 |
Standard error of Declination |
real |
4 |
milliarcsec |
|
stat.error;pos.eq.dec |
dec_ok |
decapsSource |
DECAPS |
Declination, good detections only {catalogue TType keyword: dec_ok} |
float |
8 |
Degrees |
-999999500.0 |
pos.eq.dec |
dec_parallax_corr |
gaia_source |
GAIADR2 |
Correlation between Declination and parallax |
real |
4 |
|
|
stat.correlation;pos.eq.dec;pos.parallax |
dec_parallax_corr |
gaia_source |
GAIAEDR3 |
Correlation between Declination and parallax |
real |
4 |
|
|
stat.correlation;pos.eq.dec;pos.parallax |
dec_parallax_corr |
gaia_source, tgas_source |
GAIADR1 |
Correlation between Declination and parallax |
real |
4 |
|
|
stat.correlation |
dec_pm |
allwise_sc |
WISE |
Declination at epoch MJD=55400.0 (2010.5589) from the profile-fitting measurement model that includes motion. This column is null if the fit failed to converge or was not attempted. NOTE: This will be similar but not identical to the value of dec which is the measured declination of the source from the non-moving profile-fit. |
float |
8 |
deg |
|
|
dec_pm |
catwise_2020, catwise_prelim |
WISE |
declination (J2000) |
float |
8 |
deg |
|
|
dec_pmdec_corr |
gaia_source |
GAIADR2 |
Correlation between Declination and proper motion in Declination |
real |
4 |
|
|
stat.correlation;pos.eq.dec;pos.pm;pos.eq.dec |
dec_pmdec_corr |
gaia_source |
GAIAEDR3 |
Correlation between Declination and proper motion in Declination |
real |
4 |
|
|
stat.correlation;pos.eq.dec;pos.pm;pos.eq.dec |
dec_pmdec_corr |
gaia_source, tgas_source |
GAIADR1 |
Correlation between Declination and proper motion in Declination |
real |
4 |
|
|
stat.correlation |
dec_pmra_corr |
gaia_source |
GAIADR2 |
Correlation between Declination and proper motion in Right Ascension |
real |
4 |
|
|
stat.correlation;pos.eq.dec;pos.pm;pos.eq.ra |
dec_pmra_corr |
gaia_source |
GAIAEDR3 |
Correlation between Declination and proper motion in Right Ascension |
real |
4 |
|
|
stat.correlation;pos.eq.dec;pos.pm;pos.eq.ra |
dec_pmra_corr |
gaia_source, tgas_source |
GAIADR1 |
Correlation between Declination and proper motion in Right Ascension |
real |
4 |
|
|
stat.correlation |
dec_pseudocolour_corr |
gaia_source |
GAIAEDR3 |
Correlation between declination and pseudocolour |
real |
4 |
|
|
stat.correlation;em.wavenumber;pos.eq.dec |
DEC_R |
spectra |
SIXDF |
observed dec (J2000 degrees) |
float |
8 |
degrees |
|
|
DEC_UNC |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Declination of the source in degrees (J2000) as determined by the SAS task emldetect by fitting a detection simultaneously in all cameras and energy bands. |
float |
8 |
degrees |
|
|
DEC_V |
spectra |
SIXDF |
observed dec (J2000 degrees) |
float |
8 |
degrees |
|
|
decB1950 |
mgcDetection |
MGC |
Object declination (B1950) |
float |
8 |
deg |
|
|
decBase |
Multiframe |
SHARKSv20210222 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
SHARKSv20210421 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
ULTRAVISTADR4 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSDR1 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSDR2 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSDR3 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSDR4 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSDR5 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSDR6 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20120926 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20130417 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20140409 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20150108 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20160114 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20160507 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20170630 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20180419 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20201209 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20231101 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VHSv20240731 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIDEODR2 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIDEODR3 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIDEODR4 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIDEODR5 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIDEOv20100513 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIDEOv20111208 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGDR2 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGDR3 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGDR4 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGv20110714 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGv20111019 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGv20130417 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGv20140402 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGv20150421 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGv20151230 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGv20160406 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGv20161202 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VIKINGv20170715 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCDEEPv20230713 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCDEEPv20240506 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCDR1 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCDR2 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCDR3 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCDR4 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCDR5 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20110816 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20110909 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20120126 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20121128 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20130304 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20130805 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20140428 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20140903 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20150309 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20151218 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20160311 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20160822 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20170109 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20170411 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20171101 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20180702 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20181120 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20191212 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20210708 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20230816 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VMCv20240226 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VVVDR1 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VVVDR2 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VVVDR5 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VVVXDR1 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VVVv20100531 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
Multiframe |
VVVv20110718 |
Declination of base position (J2000) {image primary HDU keyword: DEC} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decBase |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Declination of base position (J2000) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decCen |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Celestial Declination of centroid |
float |
8 |
Degrees |
|
pos.eq.dec |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
decCen |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
Celestial Declination of centroid |
float |
8 |
Degrees |
|
pos.eq.dec |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
decCen |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
Celestial Declination of centroid |
float |
8 |
Degrees |
|
pos.eq.dec |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
decCentre |
StdFieldInfo |
VIDEOv20100513 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.ra;meta.main |
decCentre |
StdFieldInfo |
VIKINGv20110714 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.ra;meta.main |
decCentre |
StdFieldInfo |
VVVv20100531 |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.ra;meta.main |
decDMS |
ogle3LpvLmcSource, ogle3LpvSmcSource, ogle4CepLmcSource, ogle4CepSmcSource, ogle4RRLyrLmcSource, ogle4RRLyrSmcSource |
OGLE |
Declination, equinox 2000.0 |
varchar |
12 |
d:m:s |
|
pos.eq.dec;meta.main |
decErr |
Detection |
PS1DR2 |
Declination error. |
real |
4 |
arcsec |
-999 |
|
decErr |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Error in averaged Celestial Declination |
float |
8 |
pixels |
|
|
decErr |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Error in averaged Celestial Declination |
float |
8 |
pixels |
|
|
decErr |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Error in averaged Celestial Declination |
float |
8 |
pixels |
|
|
decerr |
smashdr2_deep, smashdr2_object |
SMASH |
Uncertainty in mean DEC of object (arcseconds) from indiv values |
real |
4 |
|
|
|
decerr |
smashdr2_source |
SMASH |
Uncertainty in DEC (arcseconds) based on S/N of source and PSF FWHM |
real |
4 |
|
|
|
decExtent |
RequiredMosaic |
SHARKSv20210421 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
ULTRAVISTADR4 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSDR1 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSDR2 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSDR3 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSDR4 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSDR5 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSDR6 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSv20120926 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSv20130417 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSv20150108 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSv20160114 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSv20160507 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSv20170630 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSv20180419 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSv20201209 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSv20231101 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VHSv20240731 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIDEODR2 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIDEODR3 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIDEODR4 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIDEODR5 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIDEOv20100513 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIDEOv20111208 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGDR2 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGDR3 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGDR4 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGv20110714 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGv20111019 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGv20130417 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGv20150421 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGv20151230 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGv20160406 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGv20161202 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VIKINGv20170715 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCDEEPv20230713 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCDEEPv20240506 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCDR1 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCDR3 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCDR4 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCDR5 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20110816 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20110909 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20120126 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20121128 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20130304 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20130805 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20140428 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20140903 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20150309 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20151218 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20160311 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20160822 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20170109 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20170411 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20171101 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20180702 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20181120 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20191212 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20210708 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20230816 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VMCv20240226 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VVVDR1 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VVVDR2 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VVVDR5 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VVVXDR1 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VVVv20100531 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
VVVv20110718 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic, RequiredRegion |
SHARKSv20210222 |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decindiv |
smashdr2_source |
SMASH |
Declination of source, from the original chip X/Y and WCS |
float |
8 |
|
|
|
decJ |
vmcPsfCatalogue |
VMCDR3 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfCatalogue |
VMCDR4 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfCatalogue |
VMCv20121128 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
decJ |
vmcPsfCatalogue |
VMCv20140428 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfCatalogue |
VMCv20140903 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfCatalogue |
VMCv20150309 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfCatalogue |
VMCv20151218 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfCatalogue |
VMCv20160311 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfCatalogue |
VMCv20160822 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfCatalogue |
VMCv20170109 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfCatalogue |
VMCv20170411 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfCatalogue |
VMCv20171101 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfDetections |
VMCv20181120 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decJ |
vmcPsfDetections, vmcPsfSource |
VMCv20180702 |
PSF fit Dec centre J filter {catalogue TType keyword: DEC_J} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.J |
decKs |
vmcPsfCatalogue |
VMCDR3 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfCatalogue |
VMCDR4 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfCatalogue |
VMCv20121128 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
decKs |
vmcPsfCatalogue |
VMCv20140428 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfCatalogue |
VMCv20140903 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfCatalogue |
VMCv20150309 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfCatalogue |
VMCv20151218 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfCatalogue |
VMCv20160311 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfCatalogue |
VMCv20160822 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfCatalogue |
VMCv20170109 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfCatalogue |
VMCv20170411 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfCatalogue |
VMCv20171101 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfDetections |
VMCv20181120 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decKs |
vmcPsfDetections, vmcPsfSource |
VMCv20180702 |
PSF fit Dec centre Ks filter {catalogue TType keyword: DEC_Ks} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.K |
decMean |
ObjectThin |
PS1DR2 |
Declination from single epoch detections (weighted mean) in equinox J2000 at the mean epoch given by epochMean. |
float |
8 |
degrees |
-999 |
pos.eq.dec |
decMeanErr |
ObjectThin |
PS1DR2 |
Declination standard deviation from single epoch detections. |
real |
4 |
arcsec |
-999 |
stat.error |
decMoon |
Multiframe |
SHARKSv20210222 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
SHARKSv20210421 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
ULTRAVISTADR4 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSDR1 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSDR2 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSDR3 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSDR4 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSDR5 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSDR6 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20120926 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20130417 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20140409 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20150108 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20160114 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20160507 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20170630 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20180419 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20201209 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20231101 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VHSv20240731 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIDEODR2 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIDEODR3 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIDEODR4 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIDEODR5 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIDEOv20100513 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIDEOv20111208 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGDR2 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGDR3 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGDR4 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGv20110714 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGv20111019 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGv20130417 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGv20140402 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGv20150421 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGv20151230 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGv20160406 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGv20161202 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VIKINGv20170715 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCDEEPv20230713 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCDEEPv20240506 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCDR1 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCDR2 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCDR3 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCDR4 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCDR5 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20110816 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20110909 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20120126 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20121128 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20130304 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20130805 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20140428 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20140903 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20150309 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20151218 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20160311 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20160822 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20170109 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20170411 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20171101 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20180702 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20181120 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20191212 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20210708 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20230816 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VMCv20240226 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VVVDR1 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VVVDR2 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VVVDR5 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VVVXDR1 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VVVv20100531 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
Multiframe |
VVVv20110718 |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoon |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
SHARKSv20210222 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
SHARKSv20210421 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
ULTRAVISTADR4 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSDR1 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSDR2 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSDR3 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSDR4 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSDR5 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSDR6 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20120926 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20130417 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20140409 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20150108 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20160114 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20160507 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20170630 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20180419 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20201209 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20231101 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VHSv20240731 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIDEODR2 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIDEODR3 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIDEODR4 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIDEODR5 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIDEOv20100513 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIDEOv20111208 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGDR2 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGDR3 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGDR4 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGv20110714 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGv20111019 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGv20130417 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGv20140402 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGv20150421 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGv20151230 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGv20160406 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGv20161202 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VIKINGv20170715 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCDEEPv20230713 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCDEEPv20240506 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCDR1 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCDR2 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCDR3 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCDR4 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCDR5 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20110816 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20110909 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20120126 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20121128 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20130304 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20130805 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20140428 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20140903 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20150309 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20151218 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20160311 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20160822 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20170109 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20170411 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20171101 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20180702 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20181120 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20191212 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20210708 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20230816 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VMCv20240226 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VVVDR1 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VVVDR2 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VVVDR5 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VVVXDR1 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VVVv20100531 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
Multiframe |
VVVv20110718 |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decref |
smashdr2_source |
SMASH |
Declination (J2000.0) of source, from the referene chip chip file using XREF/YREF coords and the reference chip WCS |
float |
8 |
degrees |
|
|
decscatter |
smashdr2_deep, smashdr2_object |
SMASH |
RMS scatter in DEC from multiple measurements of this object |
real |
4 |
|
|
|
decStack |
ObjectThin |
PS1DR2 |
Declination from stack detections, weighted mean value across filters, in equinox J2000. See StackObjectThin for stack epoch information. |
float |
8 |
degrees |
-999 |
pos.eq.dec |
decStackErr |
ObjectThin |
PS1DR2 |
Declination standard deviation from stack detections. |
real |
4 |
arcsec |
-999 |
stat.error |
decurtainRange |
MultiframeDetector |
SHARKSv20210222 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
SHARKSv20210421 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
ULTRAVISTADR4 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSDR1 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSDR2 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSDR3 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSDR4 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSDR5 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSDR6 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20120926 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20130417 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20140409 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20150108 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20160114 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20160507 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20170630 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20180419 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20201209 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20231101 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VHSv20240731 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIDEODR2 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIDEODR3 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIDEODR4 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIDEODR5 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIDEOv20100513 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIDEOv20111208 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGDR2 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGDR3 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGDR4 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGv20110714 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGv20111019 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGv20130417 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGv20140402 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGv20150421 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGv20151230 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGv20160406 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGv20161202 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VIKINGv20170715 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCDEEPv20230713 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCDEEPv20240506 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCDR1 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCDR2 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCDR3 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCDR4 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCDR5 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20110816 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20110909 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20120126 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20121128 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20130304 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20130805 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20140428 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20140903 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20150309 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20151218 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20160311 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20160822 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20170109 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20170411 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20171101 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20180702 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20181120 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20191212 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20210708 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20230816 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VMCv20240226 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VVVDR1 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VVVDR2 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VVVDR5 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VVVXDR1 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VVVv20100531 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
VVVv20110718 |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Range of decurtain correction |
real |
4 |
|
-0.9999995e9 |
?? |
decY |
vmcPsfCatalogue |
VMCDR3 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfCatalogue |
VMCDR4 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfCatalogue |
VMCv20121128 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec |
decY |
vmcPsfCatalogue |
VMCv20140428 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfCatalogue |
VMCv20140903 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfCatalogue |
VMCv20150309 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfCatalogue |
VMCv20151218 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfCatalogue |
VMCv20160311 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfCatalogue |
VMCv20160822 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfCatalogue |
VMCv20170109 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfCatalogue |
VMCv20170411 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfCatalogue |
VMCv20171101 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfDetections |
VMCv20181120 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
decY |
vmcPsfDetections, vmcPsfSource |
VMCv20180702 |
PSF fit Dec centre Y filter {catalogue TType keyword: DEC_Y} |
float |
8 |
deg |
-0.9999995e9 |
pos.eq.dec;em.IR.NIR |
DEdeg |
denisDR3Source |
DENIS |
Declination (J2000) |
real |
4 |
deg |
|
|
DEdeg |
ravedr5Source |
RAVE |
Declination (J2000) |
float |
8 |
deg |
|
pos.eq.dec |
dej2000 |
masterDR2 |
SKYMAPPER |
Mean ICRS Declination of the object |
float |
8 |
deg |
|
pos.eq.dec;meta.main;stat.mean |
Delat |
catwise_2020, catwise_prelim |
WISE |
desc-asce ecliptic latitude |
real |
4 |
arcsec |
|
|
DelatSig |
catwise_2020, catwise_prelim |
WISE |
one-sigma uncertainty in Delat |
real |
4 |
arcsec |
|
|
DelatSNR |
catwise_2020, catwise_prelim |
WISE |
|Delat|/DelatSig |
real |
4 |
|
|
|
Delon |
catwise_2020, catwise_prelim |
WISE |
desc-asce ecliptic longitude |
real |
4 |
arcsec |
|
|
DelonSig |
catwise_2020, catwise_prelim |
WISE |
one-sigma uncertainty in Delon |
real |
4 |
arcsec |
|
|
Delon may have a bias correction for a systematic error induced by residual PSF errors that manifest themselves in ascending-descending differences; see the "-pb" command line option of the mrgad program. Delon is defined as descending position minus ascending position in order to have the proper sign for parallax (∼ Delon/2). Delon is the straightforward difference in ecliptic longitude, ignoring the different effective observation epochs of ascending and descending scans; Delon will be null unless ka = 3. |
DelonSNR |
catwise_2020, catwise_prelim |
WISE |
|Delon|/DelonSig |
real |
4 |
|
|
|
delPropData |
SurveyProgrammes |
SHARKSv20210222 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
SHARKSv20210421 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
ULTRAVISTADR4 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSDR1 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSDR2 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSDR3 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSDR4 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSDR5 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSDR6 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSv20120926 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSv20130417 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSv20150108 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSv20160114 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSv20160507 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSv20170630 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSv20180419 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSv20201209 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSv20231101 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VHSv20240731 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIDEODR2 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIDEODR3 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIDEODR4 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIDEODR5 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIDEOv20100513 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIDEOv20111208 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGDR2 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGDR3 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGDR4 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGv20110714 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGv20111019 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGv20130417 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGv20150421 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGv20151230 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGv20160406 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGv20161202 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VIKINGv20170715 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCDEEPv20230713 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCDEEPv20240506 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCDR1 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCDR3 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCDR4 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCDR5 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20110816 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20110909 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20120126 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20121128 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20130304 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20130805 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20140428 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20140903 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20150309 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20151218 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20160311 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20160822 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20170109 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20170411 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20171101 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20180702 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20181120 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20191212 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20210708 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20230816 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VMCv20240226 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VSAQC |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VVVDR1 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VVVDR2 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VVVDR5 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VVVXDR1 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VVVv20100531 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
VVVv20110718 |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
deltaMag |
sharksDetection |
SHARKSv20210222 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
sharksDetection |
SHARKSv20210421 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
ultravistaDetection |
ULTRAVISTADR4 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
ultravistaMapRemeasurement |
ULTRAVISTADR4 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vhsDetection |
VHSDR1 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
vhsDetection |
VHSDR2 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
vhsDetection |
VHSDR3 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vhsDetection |
VHSDR4 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vhsDetection |
VHSDR5 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vhsDetection |
VHSDR6 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vhsDetection |
VHSv20120926 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vhsDetection |
VHSv20130417 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vhsDetection |
VHSv20140409 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vhsDetection |
VHSv20150108 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vhsDetection |
VHSv20160114 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vhsDetection |
VHSv20160507 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vhsDetection |
VHSv20170630 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vhsDetection |
VHSv20180419 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vhsDetection |
VHSv20201209 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vhsDetection |
VHSv20231101 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vhsDetection |
VHSv20240731 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
videoDetection |
VIDEODR2 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
videoDetection |
VIDEODR3 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
videoDetection |
VIDEODR4 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
videoDetection |
VIDEODR5 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
videoDetection |
VIDEOv20100513 |
sum of magnitude corrections for faster processing |
real |
4 |
|
-0.9999995e9 |
|
deltaMag |
videoDetection |
VIDEOv20111208 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
vikingDetection |
VIKINGDR2 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
vikingDetection |
VIKINGDR3 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vikingDetection |
VIKINGDR4 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vikingDetection |
VIKINGv20110714 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
vikingDetection |
VIKINGv20111019 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
vikingDetection |
VIKINGv20130417 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vikingDetection |
VIKINGv20140402 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vikingDetection |
VIKINGv20150421 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vikingDetection |
VIKINGv20151230 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vikingDetection |
VIKINGv20160406 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vikingDetection |
VIKINGv20161202 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vikingDetection |
VIKINGv20170715 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vmcDetection |
VMCDR1 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
vmcDetection |
VMCDR2 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vmcDetection |
VMCDR3 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCDR4 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCDR5 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20110816 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
vmcDetection |
VMCv20110909 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
vmcDetection |
VMCv20120126 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
|
deltaMag |
vmcDetection |
VMCv20121128 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vmcDetection |
VMCv20130304 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vmcDetection |
VMCv20130805 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vmcDetection |
VMCv20140428 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vmcDetection |
VMCv20140903 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20150309 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20151218 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20160311 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20160822 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20170109 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20170411 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20171101 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20180702 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20181120 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20191212 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20210708 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20230816 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcDetection |
VMCv20240226 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcdeepDetection |
VMCDEEPv20230713 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vmcdeepDetection |
VMCDEEPv20240506 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaMag |
vvvDetection |
VVVDR1 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vvvDetection |
VVVDR2 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deltaMag |
vvvDetection |
VVVv20100531 |
sum of magnitude corrections for faster processing |
real |
4 |
|
-0.9999995e9 |
|
deltaMag |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param;phot.mag |
deltaVal |
PreviousCalibParams |
SHARKSv20210222 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
SHARKSv20210421 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
VHSv20201209 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
VHSv20231101 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
VHSv20240731 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
VMCDEEPv20230713 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
VMCDEEPv20240506 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
VMCv20210708 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
VMCv20230816 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
VMCv20240226 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
VVVDR5 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
deltaVal |
PreviousCalibParams |
VVVXDR1 |
Difference from new value to old value of attribute |
real |
4 |
|
-0.9999995e9 |
|
density |
masterDR2 |
SKYMAPPER |
Number of DR2 sources within 15 arcsec (including this source) |
real |
4 |
|
|
src.density |
density |
twomass_xsc |
TWOMASS |
Coadd log(density) of stars with k<14 mag. |
real |
4 |
|
|
phys.density |
depm |
vvvParallaxCatalogue, vvvProperMotionCatalogue |
VVVDR5 |
Dec component of Proper motion {catalogue TType keyword: depm} |
float |
8 |
mas/yr |
-999999500.0 |
|
deprecated |
MapFrameStatus |
SHARKSv20210222 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
SHARKSv20210421 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
ULTRAVISTADR4 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VHSv20201209 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VHSv20231101 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VHSv20240731 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VMCDEEPv20230713 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VMCDEEPv20240506 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VMCDR5 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VMCv20191212 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VMCv20210708 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VMCv20230816 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VMCv20240226 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VVVDR5 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
MapFrameStatus |
VVVXDR1 |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
meta.code |
deprecated |
Multiframe |
SHARKSv20210222 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
SHARKSv20210421 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
ULTRAVISTADR4 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSDR1 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSDR2 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSDR3 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSDR4 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSDR5 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSDR6 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20120926 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20130417 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20140409 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20150108 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20160114 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20160507 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20170630 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20180419 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20201209 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20231101 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VHSv20240731 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIDEODR2 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIDEODR3 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIDEODR4 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIDEODR5 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIDEOv20100513 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIDEOv20111208 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGDR2 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGDR3 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGDR4 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGv20110714 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGv20111019 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGv20130417 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGv20140402 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGv20150421 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGv20151230 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGv20160406 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGv20161202 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VIKINGv20170715 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCDEEPv20230713 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCDEEPv20240506 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCDR1 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCDR2 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCDR3 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCDR4 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCDR5 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20110816 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20110909 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20120126 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20121128 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20130304 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20130805 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20140428 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20140903 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20150309 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20151218 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20160311 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20160822 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20170109 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20170411 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20171101 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20180702 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the VVV) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
VMCv20181120 |
Code for a current (=0) or deprecated (!=0) multiframe |
smallint |
2 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete OBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | < |