N |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
N1 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Possible number of detections for band 1 |
int |
4 |
|
-9 |
|
N2 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Possible number of detections for band 2 |
int |
4 |
|
-9 |
|
N3 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Possible number of detections for band 3 |
int |
4 |
|
-9 |
|
N3_6 |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
Number of possible detections for 3.6um IRAC (Band 1) |
int |
4 |
|
-9 |
|
n3_6 |
sage_lmcIracSource |
SPITZER |
Possible number of detections for band 3.6 |
int |
4 |
|
|
|
n3_6 |
sage_smcIRACv1_5Source |
SPITZER |
Number of possible detections for 3.6um IRAC (Band 1) |
int |
4 |
|
|
|
N4 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Possible number of detections for band 4 |
int |
4 |
|
-9 |
|
N4_5 |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
Number of possible detections for 4.5um IRAC (Band 2) |
int |
4 |
|
-9 |
|
n4_5 |
sage_lmcIracSource |
SPITZER |
Possible number of detections for band 4.5 |
int |
4 |
|
|
|
n4_5 |
sage_smcIRACv1_5Source |
SPITZER |
Number of possible detections for 4.5 um IRAC (Band 2) |
int |
4 |
|
|
|
N5_8 |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
Number of possible detections for 5.8um IRAC (Band 3) |
int |
4 |
|
-9 |
|
n5_8 |
sage_lmcIracSource |
SPITZER |
Possible number of detections for band 5.8 |
int |
4 |
|
|
|
n5_8 |
sage_smcIRACv1_5Source |
SPITZER |
Number of possible detections for 5.8um IRAC (Band 3) |
int |
4 |
|
|
|
N8_0 |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
Number of possible detections for 8.0um IRAC (Band 4) |
int |
4 |
|
-9 |
|
n8_0 |
sage_lmcIracSource |
SPITZER |
Possible number of detections for band 8.0 |
int |
4 |
|
|
|
n8_0 |
sage_smcIRACv1_5Source |
SPITZER |
Number of possible detections for 8.0um IRAC (Band 4) |
int |
4 |
|
|
|
n_2mass |
allwise_sc |
WISE |
The number of 2MASS PSC entries found within a 3" radius of the WISE source position. If more than one 2MASS PSC falls within 3" of the WISE position, the closest 2MASS PSC entry is listed. This column is zero if there is no associated 2MASS PSC source. |
int |
4 |
|
|
|
n_2mass |
wise_allskysc |
WISE |
The number of 2MASS PSC entries found within a 3" radius of the WISE source position. If more than one 2MASS PSC falls within 3" of the WISE position, the closest 2MASS PSC entry is listed. This column is default if there is no associated 2MASS PSC source |
smallint |
2 |
|
-9999 |
|
n_2mass |
wise_prelimsc |
WISE |
The number of 2MASS PSC entries found within a 3" radius of the WISE source position If more than one 2MASS PSC falls within 3" of the WISE position, the closest 2MASS PSC entry is listed. This column is default if there is no associated 2MASS PSC source |
smallint |
2 |
|
-9999 |
|
n_aw |
catwise_2020, catwise_prelim |
WISE |
number of AllWISE matches within 2.75 asec |
int |
4 |
|
|
|
n_blank |
twomass_xsc |
TWOMASS |
number of blanked source records. |
smallint |
2 |
|
|
meta.number |
N_DETECTIONS |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
XMM |
The number of detections of the unique source SRCID used to derive the averaged values. |
int |
4 |
|
|
|
N_DETECTIONS |
xmm3dr4 |
XMM |
The number of detections of the unique source SRCID used to derive the averaged values. |
smallint |
2 |
|
|
|
n_epmf_0 |
vvvProperMotionCatalogue |
VVVDR5 |
The number of pawprint sets with no error flags {catalogue TType keyword: n_epmf_0} |
int |
4 |
|
-99999999 |
|
n_epmf_1 |
vvvProperMotionCatalogue |
VVVDR5 |
The number of pawprint sets with median proper motion uncertainty at this magnitude >5 mas/yr {catalogue TType keyword: n_epmf_1} |
int |
4 |
|
-99999999 |
|
n_epmf_2 |
vvvProperMotionCatalogue |
VVVDR5 |
The number of pawprint sets with proper motion uncertainty for this source is significantly greater than normal for a source of its magnitude {catalogue TType keyword: n_epmf_2} |
int |
4 |
|
-99999999 |
|
n_epmf_3 |
vvvProperMotionCatalogue |
VVVDR5 |
The number of pawprint sets with both 1+2 {catalogue TType keyword: n_epmf_3} |
int |
4 |
|
-99999999 |
|
n_ext |
twomass_scn |
TWOMASS |
Number of regular extended sources detected in scan. |
int |
4 |
|
|
meta.number |
n_ext |
twomass_sixx2_scn |
TWOMASS |
number of regular extended sources detected in scan |
int |
4 |
|
|
|
N_Gauss_fit |
ravedr5Source |
RAVE |
Number of components required for multi-aussian distance modulus fit |
int |
4 |
|
|
meta.number |
N_SPEC |
mgcBrightSpec |
MGC |
Total number of spectra for this object |
smallint |
2 |
|
|
|
n_sub |
twomass_xsc |
TWOMASS |
number of subtracted source records. |
smallint |
2 |
|
|
meta.number |
na |
allwise_sc |
WISE |
Active deblending flag. Indicates if a single detection was split into multiple sources in the process of profile-fitting: 0 - the source is not actively deblended; 1 - the source is actively deblended. |
int |
4 |
|
|
|
na |
catwise_2020, catwise_prelim |
WISE |
number of actively deblended components |
int |
4 |
|
|
|
na |
wise_allskysc |
WISE |
Active deblending flag. Indicates if a single detection was split into multiple sources in the process of profile-fitting: 0 - the source is not actively deblended; 1 - the source is actively deblended. |
smallint |
2 |
|
-9999 |
|
na |
wise_prelimsc |
WISE |
Active deblending flag Indicates if a single detection was split into multiple sources in the process of profile-fitting: 0 - the source is not actively deblended; 1 - the source is actively deblended. |
smallint |
2 |
|
-9999 |
|
NAME |
grs_ngpSource, grs_ranSource, grs_sgpSource |
TWODFGRS |
2dFGRS assigned name; if either (i) BJSELOLD is fainter than 19.45, or (ii) the object could not be allocated to a fibre by the configuration algorithm, then NAME is blank |
varchar |
10 |
|
|
|
name |
Filter |
SHARKSv20210222 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
SHARKSv20210421 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
ULTRAVISTADR4 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSDR1 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSDR2 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSDR3 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSDR4 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSDR5 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSDR6 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSDR7 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSv20120926 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSv20130417 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSv20150108 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSv20160114 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSv20160507 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSv20170630 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSv20180419 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSv20201209 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VHSv20231101 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIDEODR2 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIDEODR3 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIDEODR4 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIDEODR5 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIDEOv20100513 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIDEOv20111208 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGDR2 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGDR3 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGDR4 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGv20110714 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGv20111019 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGv20130417 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGv20150421 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGv20151230 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGv20160406 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGv20161202 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VIKINGv20170715 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCDEEPv20230713 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCDEEPv20240506 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCDR1 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCDR3 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCDR4 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCDR5 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20110816 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20110909 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20120126 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20121128 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20130304 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20130805 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20140428 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20140903 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20150309 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20151218 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20160311 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20160822 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20170109 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20170411 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20171101 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20180702 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20181120 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20191212 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20210708 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20230816 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20240226 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VMCv20250130 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VSAQC |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VVVDR1 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VVVDR2 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VVVDR5 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VVVXDR1 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VVVv20100531 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
Filter |
VVVv20110718 |
The name of the filter, eg. "MKO J", "K short" etc. |
varchar |
16 |
|
|
meta.note |
name |
RequiredListDrivenProduct |
VHSv20130417 |
the name of the list |
varchar |
16 |
|
NONE |
?? |
name |
RequiredListDrivenProduct |
VIKINGv20130417 |
the name of the list |
varchar |
16 |
|
NONE |
?? |
name |
RequiredListDrivenProduct |
VMCv20130805 |
the name of the list |
varchar |
16 |
|
NONE |
?? |
name |
RequiredMatchedApertureProduct |
SHARKSv20210222 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
SHARKSv20210421 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
ULTRAVISTADR4 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VHSDR7 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VHSv20201209 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VHSv20231101 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VMCDEEPv20230713 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VMCDEEPv20240506 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VMCDR5 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VMCv20191212 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VMCv20210708 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VMCv20230816 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VMCv20240226 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VMCv20250130 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VVVDR5 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMatchedApertureProduct |
VVVXDR1 |
the name of the matched aperture product |
varchar |
16 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
SHARKSv20210421 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
ULTRAVISTADR4 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VHSDR5 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VHSDR6 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VHSDR7 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VHSv20160114 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VHSv20160507 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VHSv20170630 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VHSv20180419 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VHSv20201209 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VHSv20231101 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VIKINGv20151230 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VIKINGv20160406 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VIKINGv20161202 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VIKINGv20170715 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCDEEPv20230713 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCDEEPv20240506 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCDR4 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCDR5 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20151218 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20160311 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20160822 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20170109 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20170411 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20171101 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20180702 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20181120 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20191212 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20210708 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20230816 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20240226 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VMCv20250130 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VVVDR5 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch |
VVVXDR1 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMergeLogMultiEpoch, RequiredStack, RequiredTile |
SHARKSv20210222 |
Name of the stacked product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
SHARKSv20210222 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
SHARKSv20210421 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
ULTRAVISTADR4 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSDR1 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSDR2 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSDR3 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSDR4 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSDR5 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSDR6 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSDR7 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSv20120926 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSv20130417 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSv20150108 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSv20160114 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSv20160507 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSv20170630 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSv20180419 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSv20201209 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VHSv20231101 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIDEODR2 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIDEODR3 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIDEODR4 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIDEODR5 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIDEOv20100513 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIDEOv20111208 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGDR2 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGDR3 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGDR4 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGv20110714 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGv20111019 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGv20130417 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGv20150421 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGv20151230 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGv20160406 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGv20161202 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VIKINGv20170715 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCDEEPv20230713 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCDEEPv20240506 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCDR1 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCDR3 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCDR4 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCDR5 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20110816 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20110909 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20120126 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20121128 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20130304 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20130805 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20140428 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20140903 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20150309 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20151218 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20160311 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20160822 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20170109 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20170411 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20171101 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20180702 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20181120 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20191212 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20210708 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20230816 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20240226 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VMCv20250130 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VVVDR1 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VVVDR2 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VVVDR5 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VVVXDR1 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VVVv20100531 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaic |
VVVv20110718 |
Name of the mosaiced product |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
SHARKSv20210222 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
SHARKSv20210421 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
ULTRAVISTADR4 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VHSDR7 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VHSv20201209 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VHSv20231101 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VMCDEEPv20230713 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VMCDEEPv20240506 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VMCDR5 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VMCv20191212 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VMCv20210708 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VMCv20230816 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VMCv20240226 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VMCv20250130 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VVVDR5 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredMosaicTopLevel |
VVVXDR1 |
Name of the mosaiced product set up |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
SHARKSv20210222 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
SHARKSv20210421 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
ULTRAVISTADR4 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VHSDR7 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VHSv20201209 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VHSv20231101 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VMCDEEPv20230713 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VMCDEEPv20240506 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VMCDR5 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VMCv20191212 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VMCv20210708 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VMCv20230816 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VMCv20240226 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VMCv20250130 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VVVDR5 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
RequiredRegion |
VVVXDR1 |
Name of the region |
varchar |
64 |
|
|
?? |
name |
Survey |
SHARKSv20210222 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
SHARKSv20210421 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
ULTRAVISTADR4 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSDR1 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSDR2 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSDR3 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSDR4 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSDR5 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSDR6 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSDR7 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSv20120926 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSv20130417 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSv20150108 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSv20160114 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSv20160507 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSv20170630 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSv20180419 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSv20201209 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VHSv20231101 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIDEODR2 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIDEODR3 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIDEODR4 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIDEODR5 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIDEOv20100513 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIDEOv20111208 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGDR2 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGDR3 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGDR4 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGv20110714 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGv20111019 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGv20130417 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGv20150421 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGv20151230 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGv20160406 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGv20161202 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VIKINGv20170715 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCDEEPv20230713 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCDEEPv20240506 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCDR1 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCDR3 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCDR4 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCDR5 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20110816 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20110909 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20120126 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20121128 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20130304 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20130805 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20140428 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20140903 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20150309 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20151218 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20160311 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20160822 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20170109 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20170411 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20171101 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20180702 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20181120 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20191212 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20210708 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20230816 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20240226 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VMCv20250130 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VSAQC |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VVVDR1 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VVVDR2 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VVVDR5 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VVVXDR1 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VVVv20100531 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
Survey |
VVVv20110718 |
The short name for the survey |
varchar |
128 |
|
|
?? |
name |
iras_asc, iras_psc |
IRAS |
Source Name |
varchar |
11 |
|
|
meta.id;meta.main |
name |
ukirtFSstars |
VIDEOv20100513 |
reference name of field |
varchar |
16 |
|
NONE |
???? |
name |
ukirtFSstars |
VIKINGv20110714 |
reference name of field |
varchar |
16 |
|
NONE |
???? |
name |
ukirtFSstars |
VVVv20100531 |
reference name of field |
varchar |
16 |
|
NONE |
???? |
NAME_R |
spectra |
SIXDF |
name of object in R frame |
varchar |
32 |
|
|
|
NAME_V |
spectra |
SIXDF |
name of object in V frame |
varchar |
32 |
|
|
|
naxis |
Multiframe |
SHARKSv20210222 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
SHARKSv20210421 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
ULTRAVISTADR4 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSDR1 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSDR2 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSDR3 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSDR4 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSDR5 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSDR6 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSDR7 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSv20120926 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSv20130417 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSv20140409 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSv20150108 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSv20160114 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSv20160507 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSv20170630 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSv20180419 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSv20201209 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VHSv20231101 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIDEODR2 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIDEODR3 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIDEODR4 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIDEODR5 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIDEOv20100513 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIDEOv20111208 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGDR2 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGDR3 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGDR4 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGv20110714 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGv20111019 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGv20130417 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGv20140402 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGv20150421 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGv20151230 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGv20160406 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGv20161202 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VIKINGv20170715 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCDEEPv20230713 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCDEEPv20240506 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCDR1 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCDR2 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCDR3 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCDR4 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCDR5 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20110816 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20110909 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20120126 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20121128 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20130304 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20130805 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20140428 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20140903 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20150309 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20151218 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20160311 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20160822 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20170109 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20170411 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20171101 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20180702 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20181120 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20191212 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20210708 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20230816 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20240226 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VMCv20250130 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VVVDR1 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VVVDR2 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VVVDR5 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VVVXDR1 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VVVv20100531 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
Multiframe |
VVVv20110718 |
# of axes in data array {image primary HDU keyword: NAXIS} |
tinyint |
1 |
|
0 |
|
naxis |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
# of axes in data array |
tinyint |
1 |
|
0 |
|
nb |
allwise_sc |
WISE |
Number of PSF components used simultaneously in the profile-fitting for this source. This number includes the source itself, so the minimum value of nb is "1". Nb is greater than "1" when the source is fit concurrently with other nearby detections (passive deblending), or when a single source is split into two components during the fitting process (active deblending). |
int |
4 |
|
|
|
nb |
catwise_2020, catwise_prelim |
WISE |
number of blend components used in each fit |
int |
4 |
|
|
|
nb |
wise_allskysc |
WISE |
Number of PSF components used simultaneously in the profile-fitting for this source. This number includes the source itself, so the minimum value of nb is "1". Nb is greater than "1" when the source is fit concurrently with other nearby detections (passive deblending), or when a single source is split into two components during the fitting process (active deblending). |
smallint |
2 |
|
-9999 |
|
nb |
wise_prelimsc |
WISE |
Number of PSF components used simultaneously in the profile-fitting for this source This number includes the source itself, so the minimum value of nb is "1". Nb is greater than "1" when the source is fit concurrently with other nearby detections (passive deblending), or when a single source is split into two components during the fitting process (active deblending). |
smallint |
2 |
|
-9999 |
|
nb118AperJky3 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Default point source Nb118 aperture corrected (2.0 arcsec aperture diameter) calibrated flux If in doubt use this flux estimator |
real |
4 |
jansky |
-0.9999995e9 |
phot.flux |
nb118AperJky3Err |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in default point/extended source Nb118 (2.0 arcsec aperture diameter) calibrated flux |
real |
4 |
jansky |
-0.9999995e9 |
stat.error |
nb118AperJky4 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Point source Nb118 aperture corrected (2.8 arcsec aperture diameter) calibrated flux |
real |
4 |
jansky |
-0.9999995e9 |
phot.flux |
nb118AperJky4Err |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in point/extended source Nb118 (2.8 arcsec aperture diameter) calibrated flux |
real |
4 |
jansky |
-0.9999995e9 |
stat.error |
nb118AperJky6 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Point source Nb118 aperture corrected (5.7 arcsec aperture diameter) calibrated flux |
real |
4 |
jansky |
-0.9999995e9 |
phot.flux |
nb118AperJky6Err |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in point/extended source Nb118 (5.7 arcsec aperture diameter) calibrated flux |
real |
4 |
jansky |
-0.9999995e9 |
stat.error |
nb118AperJkyNoAperCorr3 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Default extended source Nb118 (2.0 arcsec aperture diameter, but no aperture correction applied) aperture calibrated flux If in doubt use this flux estimator |
real |
4 |
jansky |
-0.9999995e9 |
phot.flux |
nb118AperJkyNoAperCorr4 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 (2.8 arcsec aperture diameter, but no aperture correction applied) aperture calibrated flux |
real |
4 |
jansky |
-0.9999995e9 |
phot.flux |
nb118AperJkyNoAperCorr6 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 (5.7 arcsec aperture diameter, but no aperture correction applied) aperture calibrated flux |
real |
4 |
jansky |
-0.9999995e9 |
phot.flux |
nb118AperLup3 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Default point source Nb118 aperture corrected (2.0 arcsec aperture diameter) luptitude If in doubt use this flux estimator |
real |
4 |
lup |
-0.9999995e9 |
phot.lup |
nb118AperLup3Err |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in default point/extended source Nb118 (2.0 arcsec aperture diameter) luptitude |
real |
4 |
lup |
-0.9999995e9 |
stat.error |
nb118AperLup4 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Point source Nb118 aperture corrected (2.8 arcsec aperture diameter) luptitude |
real |
4 |
lup |
-0.9999995e9 |
phot.lup |
nb118AperLup4Err |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in point/extended source Nb118 (2.8 arcsec aperture diameter) luptitude |
real |
4 |
lup |
-0.9999995e9 |
stat.error |
nb118AperLup6 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Point source Nb118 aperture corrected (5.7 arcsec aperture diameter) luptitude |
real |
4 |
lup |
-0.9999995e9 |
phot.lup |
nb118AperLup6Err |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in point/extended source Nb118 (5.7 arcsec aperture diameter) luptitude |
real |
4 |
lup |
-0.9999995e9 |
stat.error |
nb118AperLupNoAperCorr3 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Default extended source Nb118 (2.0 arcsec aperture diameter, but no aperture correction applied) aperture luptitude If in doubt use this flux estimator |
real |
4 |
lup |
-0.9999995e9 |
phot.lup |
nb118AperLupNoAperCorr4 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 (2.8 arcsec aperture diameter, but no aperture correction applied) aperture luptitude |
real |
4 |
lup |
-0.9999995e9 |
phot.lup |
nb118AperLupNoAperCorr6 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 (5.7 arcsec aperture diameter, but no aperture correction applied) aperture luptitude |
real |
4 |
lup |
-0.9999995e9 |
phot.lup |
nb118AperMag3 |
ultravistaSource |
ULTRAVISTADR4 |
Default point source Nb118 aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMag3 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Default point source Nb118 aperture corrected (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMag3Err |
ultravistaSource |
ULTRAVISTADR4 |
Error in default point/extended source Nb118 mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag |
nb118AperMag3Err |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in default point/extended source Nb118 (2.0 arcsec aperture diameter) magnitude |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
nb118AperMag4 |
ultravistaSource |
ULTRAVISTADR4 |
Point source Nb118 aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMag4 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Point source Nb118 aperture corrected (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMag4Err |
ultravistaSource |
ULTRAVISTADR4 |
Error in point/extended source Nb118 mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag |
nb118AperMag4Err |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in point/extended source Nb118 (2.8 arcsec aperture diameter) magnitude |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
nb118AperMag6 |
ultravistaSource |
ULTRAVISTADR4 |
Point source Nb118 aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMag6 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Point source Nb118 aperture corrected (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMag6Err |
ultravistaSource |
ULTRAVISTADR4 |
Error in point/extended source Nb118 mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag |
nb118AperMag6Err |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in point/extended source Nb118 (5.7 arcsec aperture diameter) magnitude |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
nb118AperMagNoAperCorr3 |
ultravistaSource |
ULTRAVISTADR4 |
Default extended source Nb118 aperture mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMagNoAperCorr3 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Default extended source Nb118 (2.0 arcsec aperture diameter, but no aperture correction applied) aperture magnitude If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMagNoAperCorr4 |
ultravistaSource |
ULTRAVISTADR4 |
Extended source Nb118 aperture mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMagNoAperCorr4 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 (2.8 arcsec aperture diameter, but no aperture correction applied) aperture magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMagNoAperCorr6 |
ultravistaSource |
ULTRAVISTADR4 |
Extended source Nb118 aperture mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118AperMagNoAperCorr6 |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 (5.7 arcsec aperture diameter, but no aperture correction applied) aperture magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118aStratAst |
ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Nb118 band. |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
The best fit solution to the expected RMS position around the mean for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. |
nb118aStratPht |
ultravistaMapLcVarFrameSetInfo |
ULTRAVISTADR4 |
Strateva parameter, a, in fit to photometric rms vs magnitude in Nb118 band, see Sesar et al. 2007. |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
The best fit solution to the expected RMS brightness (in magnitudes) for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. This technique was used in Sesar et al. 2007, AJ, 134, 2236. |
nb118aStratPht |
ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Parameter, c0 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Nb118 band. |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
The best fit solution to the expected RMS brightness (in magnitudes) for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. This technique was used in Sesar et al. 2007, AJ, 134, 2236. |
nb118AverageConf |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
average confidence in 2 arcsec diameter default aperture (aper3) Nb118 |
real |
4 |
|
-0.9999995e9 |
stat.likelihood;em.IR.NIR |
nb118bestAper |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Best aperture (1-3) for photometric statistics in the Nb118 band |
int |
4 |
|
-9999 |
|
Aperture magnitude (1-6) which gives the lowest RMS for the object. All apertures have the appropriate aperture correction. This can give better values in crowded regions than aperMag3 (see Irwin et al. 2007, MNRAS, 375, 1449) |
nb118bestAper |
ultravistaVariability |
ULTRAVISTADR4 |
Best aperture (1-6) for photometric statistics in the Nb118 band |
int |
4 |
|
-9999 |
meta.code.class |
Aperture magnitude (1-6) which gives the lowest RMS for the object. All apertures have the appropriate aperture correction. This can give better values in crowded regions than aperMag3 (see Irwin et al. 2007, MNRAS, 375, 1449) |
nb118bStratAst |
ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Nb118 band. |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
The best fit solution to the expected RMS position around the mean for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. |
nb118bStratPht |
ultravistaMapLcVarFrameSetInfo |
ULTRAVISTADR4 |
Strateva parameter, b, in fit to photometric rms vs magnitude in Nb118 band, see Sesar et al. 2007. |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
The best fit solution to the expected RMS brightness (in magnitudes) for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. This technique was used in Sesar et al. 2007, AJ, 134, 2236. |
nb118bStratPht |
ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Parameter, c1 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Nb118 band. |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
The best fit solution to the expected RMS brightness (in magnitudes) for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. This technique was used in Sesar et al. 2007, AJ, 134, 2236. |
nb118chiSqAst |
ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Goodness of fit of Strateva function to astrometric data in Nb118 band |
real |
4 |
|
-0.9999995e9 |
stat.fit.goodness |
The best fit solution to the expected RMS position around the mean for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. |
nb118chiSqpd |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Chi square (per degree of freedom) fit to data (mean and expected rms) |
real |
4 |
|
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118chiSqpd |
ultravistaVariability |
ULTRAVISTADR4 |
Chi square (per degree of freedom) fit to data (mean and expected rms) |
real |
4 |
|
-0.9999995e9 |
stat.fit.chi2 |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118chiSqPht |
ultravistaMapLcVarFrameSetInfo, ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Goodness of fit of Strateva function to photometric data in Nb118 band |
real |
4 |
|
-0.9999995e9 |
stat.fit.goodness |
The best fit solution to the expected RMS brightness (in magnitudes) for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. This technique was used in Sesar et al. 2007, AJ, 134, 2236. |
nb118Class |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
discrete image classification flag in Nb118 |
smallint |
2 |
|
-9999 |
src.class |
nb118ClassStat |
ultravistaSource |
ULTRAVISTADR4 |
S-Extractor classification statistic in Nb118 |
real |
4 |
|
-0.9999995e9 |
stat |
nb118ClassStat |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
N(0,1) stellarness-of-profile statistic in Nb118 |
real |
4 |
|
-0.9999995e9 |
stat |
nb118cStratAst |
ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to astrometric rms vs magnitude in Nb118 band. |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
The best fit solution to the expected RMS position around the mean for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. |
nb118cStratPht |
ultravistaMapLcVarFrameSetInfo |
ULTRAVISTADR4 |
Strateva parameter, c, in fit to photometric rms vs magnitude in Nb118 band, see Sesar et al. 2007. |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
The best fit solution to the expected RMS brightness (in magnitudes) for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. This technique was used in Sesar et al. 2007, AJ, 134, 2236. |
nb118cStratPht |
ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Parameter, c2 from Ferreira-Lopes & Cross 2017, Eq. 18, in fit to photometric rms vs magnitude in Nb118 band. |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
The best fit solution to the expected RMS brightness (in magnitudes) for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. This technique was used in Sesar et al. 2007, AJ, 134, 2236. |
nb118Ell |
ultravistaSource |
ULTRAVISTADR4 |
1-b/a, where a/b=semi-major/minor axes in Nb118 |
real |
4 |
|
-0.9999995e9 |
src.ellipticity |
nb118Ell |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
1-b/a, where a/b=semi-major/minor axes in Nb118 |
real |
4 |
|
-0.9999995e9 |
src.ellipticty |
nb118eNum |
ultravistaMergeLog, ultravistaRemeasMergeLog |
ULTRAVISTADR4 |
the extension number of this Nb118 frame |
tinyint |
1 |
|
|
meta.number |
nb118ErrBits |
ultravistaSource |
ULTRAVISTADR4 |
processing warning/error bitwise flags in Nb118 |
int |
4 |
|
-99999999 |
meta.code |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
nb118ErrBits |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
processing warning/error bitwise flags in Nb118 |
int |
4 |
|
-99999999 |
meta.code |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
nb118Eta |
ultravistaSource |
ULTRAVISTADR4 |
Offset of Nb118 detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
nb118expML |
ultravistaMapLcVarFrameSetInfo, ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Expected magnitude limit of frameSet in this in Nb118 band. |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.max |
nb118ExpRms |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Rms calculated from polynomial fit to modal RMS as a function of magnitude in Nb118 band |
real |
4 |
mag |
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118ExpRms |
ultravistaVariability |
ULTRAVISTADR4 |
Rms calculated from polynomial fit to modal RMS as a function of magnitude in Nb118 band |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118Gausig |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
RMS of axes of ellipse fit in Nb118 |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param |
nb118HalfRad |
ultravistaSource |
ULTRAVISTADR4 |
SExtractor half-light radius in Nb118 band |
real |
4 |
pixels |
-0.9999995e9 |
phys.angSize |
nb118HlCorSMjRadAs |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Seeing corrected half-light, semi-major axis in Nb118 band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize |
nb118IntRms |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Intrinsic rms in Nb118-band |
real |
4 |
mag |
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118IntRms |
ultravistaVariability |
ULTRAVISTADR4 |
Intrinsic rms in Nb118-band |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118isDefAst |
ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Use a default model for the astrometric noise in Nb118 band. |
tinyint |
1 |
|
0 |
meta.code |
nb118isDefPht |
ultravistaMapLcVarFrameSetInfo, ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Use a default model for the photometric noise in Nb118 band. |
tinyint |
1 |
|
0 |
meta.code |
nb118IsMeas |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Is pass band Nb118 measured? 0 no, 1 yes |
tinyint |
1 |
|
0 |
meta.code |
nb118KronJky |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 calibrated flux (Kron) |
real |
4 |
jansky |
-0.9999995e9 |
phot.flux |
nb118KronJkyErr |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in extended source Nb118 calibrated flux (Kron) |
real |
4 |
janksy |
-0.9999995e9 |
stat.error |
nb118KronLup |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 luptitude (Kron) |
real |
4 |
lup |
-0.9999995e9 |
phot.lup |
nb118KronLupErr |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in extended source Nb118 luptitude (Kron) |
real |
4 |
lup |
-0.9999995e9 |
stat.error |
nb118KronMag |
ultravistaSource |
ULTRAVISTADR4 |
Extended source Nb118 mag (Kron - SExtractor MAG_AUTO) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118KronMag |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 magnitude (Kron) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118KronMagErr |
ultravistaSource |
ULTRAVISTADR4 |
Extended source Nb118 mag error (Kron - SExtractor MAG_AUTO) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag |
nb118KronMagErr |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in extended source Nb118 magnitude (Kron) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
nb118MagMAD |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Median Absolute Deviation of Nb118 magnitude |
real |
4 |
mag |
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118MagMAD |
ultravistaVariability |
ULTRAVISTADR4 |
Median Absolute Deviation of Nb118 magnitude |
real |
4 |
mag |
-0.9999995e9 |
stat.err;phot.mag |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118MagRms |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
rms of Nb118 magnitude |
real |
4 |
mag |
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118MagRms |
ultravistaVariability |
ULTRAVISTADR4 |
rms of Nb118 magnitude |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118maxCadence |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
maximum gap between observations |
real |
4 |
days |
-0.9999995e9 |
|
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118maxCadence |
ultravistaVariability |
ULTRAVISTADR4 |
maximum gap between observations |
real |
4 |
days |
-0.9999995e9 |
time.interval;obs;stat.max |
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118MaxMag |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Maximum magnitude in Nb118 band, of good detections |
real |
4 |
|
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118MaxMag |
ultravistaVariability |
ULTRAVISTADR4 |
Maximum magnitude in Nb118 band, of good detections |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.max |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118meanMag |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Mean Nb118 magnitude |
real |
4 |
mag |
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118meanMag |
ultravistaVariability |
ULTRAVISTADR4 |
Mean Nb118 magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.mean |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118medCadence |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
median gap between observations |
real |
4 |
days |
-0.9999995e9 |
|
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118medCadence |
ultravistaVariability |
ULTRAVISTADR4 |
median gap between observations |
real |
4 |
days |
-0.9999995e9 |
time.interval;obs;stat.median |
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118medianMag |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Median Nb118 magnitude |
real |
4 |
mag |
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118medianMag |
ultravistaVariability |
ULTRAVISTADR4 |
Median Nb118 magnitude |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.median |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118mfID |
ultravistaMergeLog, ultravistaRemeasMergeLog |
ULTRAVISTADR4 |
the UID of the relevant Nb118 multiframe |
bigint |
8 |
|
|
meta.id;obs.field |
nb118minCadence |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
minimum gap between observations |
real |
4 |
days |
-0.9999995e9 |
|
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118minCadence |
ultravistaVariability |
ULTRAVISTADR4 |
minimum gap between observations |
real |
4 |
days |
-0.9999995e9 |
time.interval;obs;stat.min |
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118MinMag |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Minimum magnitude in Nb118 band, of good detections |
real |
4 |
|
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118MinMag |
ultravistaVariability |
ULTRAVISTADR4 |
Minimum magnitude in Nb118 band, of good detections |
real |
4 |
mag |
-0.9999995e9 |
phot.mag;stat.min |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118Mjd |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Modified Julian Day in Nb118 band |
float |
8 |
days |
-0.9999995e9 |
time.epoch |
nb118ndof |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Number of degrees of freedom for chisquare |
smallint |
2 |
|
-9999 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118ndof |
ultravistaVariability |
ULTRAVISTADR4 |
Number of degrees of freedom for chisquare |
smallint |
2 |
|
-9999 |
stat.fit.dof |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118nDofAst |
ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Number of degrees of freedom of astrometric fit in Nb118 band. |
smallint |
2 |
|
-9999 |
stat.fit.dof;stat.param |
The best fit solution to the expected RMS position around the mean for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. |
nb118nDofPht |
ultravistaMapLcVarFrameSetInfo, ultravistaVarFrameSetInfo |
ULTRAVISTADR4 |
Number of degrees of freedom of photometric fit in Nb118 band. |
smallint |
2 |
|
-9999 |
stat.fit.dof;stat.param |
The best fit solution to the expected RMS brightness (in magnitudes) for all objects in the frameset. Objects were binned in ranges of magnitude and the median RMS (after clipping out variable objects using the median-absolute deviation) was calculated. The Strateva function $\zeta(m)>=a+b\,10^{0.4m}+c\,10^{0.8m}$ was fit, where $\zeta(m)$ is the expected RMS as a function of magnitude. The chi-squared and number of degrees of freedom are also calculated. This technique was used in Sesar et al. 2007, AJ, 134, 2236. |
nb118nFlaggedObs |
ultravistaVariability |
ULTRAVISTADR4 |
Number of detections in Nb118 band flagged as potentially spurious by ultravistaDetection.ppErrBits |
int |
4 |
|
0 |
meta.number |
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118nGoodObs |
ultravistaVariability |
ULTRAVISTADR4 |
Number of good detections in Nb118 band |
int |
4 |
|
0 |
meta.number |
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118Ngt3sig |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Number of good detections in Nb118-band that are more than 3 sigma deviations (nb118AperMagN < (nb118MeanMag-3*nb118MagRms) |
smallint |
2 |
|
-9999 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118Ngt3sig |
ultravistaVariability |
ULTRAVISTADR4 |
Number of good detections in Nb118-band that are more than 3 sigma deviations (nb118AperMagN < (nb118MeanMag-3*nb118MagRms) |
smallint |
2 |
|
-9999 |
meta.number |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118nMissingObs |
ultravistaVariability |
ULTRAVISTADR4 |
Number of Nb118 band frames that this object should have been detected on and was not |
int |
4 |
|
0 |
meta.number |
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118nNegFlagObs |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Number of flagged negative measurements in Nb118 band by ultravistaMapRemeasurement.ppErrBits |
int |
4 |
|
0 |
|
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118nNegObs |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Number of unflagged negative measurements Nb118 band |
int |
4 |
|
0 |
|
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118nPosFlagObs |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Number of flagged positive measurements in Nb118 band by ultravistaMapRemeasurement.ppErrBits |
int |
4 |
|
0 |
|
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118nPosObs |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Number of unflagged positive measurements in Nb118 band |
int |
4 |
|
0 |
|
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118PA |
ultravistaSource, ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
ellipse fit celestial orientation in Nb118 |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng |
nb118PetroJky |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 calibrated flux (Petrosian) |
real |
4 |
jansky |
-0.9999995e9 |
phot.flux |
nb118PetroJkyErr |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in extended source Nb118 calibrated flux (Petrosian) |
real |
4 |
jansky |
-0.9999995e9 |
stat.error |
nb118PetroLup |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 luptitude (Petrosian) |
real |
4 |
lup |
-0.9999995e9 |
phot.lup |
nb118PetroLupErr |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in extended source Nb118 luptitude (Petrosian) |
real |
4 |
lup |
-0.9999995e9 |
stat.error |
nb118PetroMag |
ultravistaSource |
ULTRAVISTADR4 |
Extended source Nb118 mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118PetroMag |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Extended source Nb118 magnitude (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
phot.mag |
nb118PetroMagErr |
ultravistaSource |
ULTRAVISTADR4 |
Error in extended source Nb118 mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag |
nb118PetroMagErr |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Error in extended source Nb118 magnitude (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
stat.error |
nb118ppErrBits |
ultravistaSource |
ULTRAVISTADR4 |
additional WFAU post-processing error bits in Nb118 |
int |
4 |
|
0 |
meta.code |
nb118ppErrBits |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
additional WFAU post-processing error bits in Nb118 |
int |
4 |
|
0 |
meta.code |
Post-processing error quality bit flags assigned to detections in the archive curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | 0 | 7 | Low confidence in default aperture | 128 | 0x00000080 | All VDFS catalogues | 1 | 12 | Lies within detector 16 region of a tile | 4096 | 0x00001000 | All catalogues from tiles | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | VVV only | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All catalogues | 2 | 23 | Lies within the underexposed strip (or "ear") of a tile | 8388608 | 0x00800000 | All catalogues from tiles | 3 | 24 | Lies within an underexposed region of a tile due to missing detector | 16777216 | 0x01000000 | All catalogues from tiles | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all Ks band sources in the VHS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
nb118probVar |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Probability of variable from chi-square (and other data) |
real |
4 |
|
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118probVar |
ultravistaVariability |
ULTRAVISTADR4 |
Probability of variable from chi-square (and other data) |
real |
4 |
|
-0.9999995e9 |
stat.probability |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118SeqNum |
ultravistaSource |
ULTRAVISTADR4 |
the running number of the Nb118 detection |
int |
4 |
|
-99999999 |
meta.number |
nb118skewness |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Skewness in Nb118 band (see Sesar et al. 2007) |
real |
4 |
|
-0.9999995e9 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118skewness |
ultravistaVariability |
ULTRAVISTADR4 |
Skewness in Nb118 band (see Sesar et al. 2007) |
real |
4 |
mag |
-0.9999995e9 |
stat.param |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118totalPeriod |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
total period of observations (last obs-first obs) |
real |
4 |
days |
-0.9999995e9 |
|
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118totalPeriod |
ultravistaVariability |
ULTRAVISTADR4 |
total period of observations (last obs-first obs) |
real |
4 |
days |
-0.9999995e9 |
time.duration |
The observations are classified as good, flagged or missing. Flagged observations are ones where the object has a ppErrBit flag. Missing observations are observations of the part of the sky that include the position of the object, but had no detection. All the statistics are calculated from good observations. The cadence parameters give the minimum, median and maximum time between observations, which is useful to know if the data could be used to find a particular type of variable. |
nb118VarClass |
ultravistaMapLcVariability |
ULTRAVISTADR4 |
Classification of variability in this band |
smallint |
2 |
|
-9999 |
|
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118VarClass |
ultravistaVariability |
ULTRAVISTADR4 |
Classification of variability in this band |
smallint |
2 |
|
-9999 |
meta.code.class;src.var |
The photometry is calculated for good observations in the best aperture. The mean, rms, median, median absolute deviation, minMag and maxMag are quite standard. The skewness is calculated as in Sesar et al. 2007, AJ, 134, 2236. The number of good detections that are more than 3 standard deviations can indicate a distribution with many outliers. In each frameset, the mean and rms are used to derive a fit to the expected rms as a function of magnitude. The parameters for the fit are stored in VarFrameSetInfo and the value for the source is in expRms. This is subtracted from the rms in quadrature to get the intrinsic rms: the variability of the object beyond the noise in the system. The chi-squared is calculated, assuming a non-variable object which has the noise from the expected-rms and mean calculated as above. The probVar statistic assumes a chi-squared distribution with the correct number of degrees of freedom. The varClass statistic is 1, if the probVar>0.9 and intrinsicRMS/expectedRMS>3. |
nb118Xi |
ultravistaSource |
ULTRAVISTADR4 |
Offset of Nb118 detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff |
When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 1.0 arcseconds is used. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the VHS, you might wish to insist that the offsets in the selected sample are all below 0.5 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
nbad |
MultiframeDetector |
SHARKSv20210222 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
SHARKSv20210421 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
ULTRAVISTADR4 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSDR1 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSDR2 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSDR3 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSDR4 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSDR5 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSDR6 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSDR7 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSv20120926 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSv20130417 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSv20140409 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSv20150108 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSv20160114 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSv20160507 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSv20170630 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSv20180419 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSv20201209 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VHSv20231101 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIDEODR2 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIDEODR3 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIDEODR4 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIDEODR5 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIDEOv20100513 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIDEOv20111208 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGDR2 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGDR3 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGDR4 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGv20110714 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGv20111019 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGv20130417 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGv20140402 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGv20150421 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGv20151230 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGv20160406 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGv20161202 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VIKINGv20170715 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCDEEPv20230713 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCDEEPv20240506 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCDR1 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCDR2 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCDR3 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCDR4 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCDR5 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20110816 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20110909 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20120126 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20121128 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20130304 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20130805 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20140428 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20140903 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20150309 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20151218 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20160311 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20160822 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20170109 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20170411 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20171101 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20180702 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20181120 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20191212 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20210708 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20230816 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20240226 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VMCv20250130 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VVVDR1 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VVVDR2 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VVVDR5 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VVVXDR1 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VVVv20100531 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
MultiframeDetector |
VVVv20110718 |
Number of bad pixels {image extension keyword: NBAD} |
int |
4 |
|
-99999999 |
|
nbad |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Number of bad pixels |
int |
4 |
|
-99999999 |
|
nbsize |
MultiframeDetector |
SHARKSv20210222 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
SHARKSv20210421 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
ULTRAVISTADR4 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSDR1 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSDR2 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSDR3 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSDR4 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSDR5 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSDR6 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSDR7 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSv20120926 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSv20130417 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSv20140409 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSv20150108 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSv20160114 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSv20160507 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSv20170630 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSv20180419 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSv20201209 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VHSv20231101 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIDEODR2 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIDEODR3 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIDEODR4 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIDEODR5 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIDEOv20111208 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGDR2 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGDR3 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGDR4 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGv20110714 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGv20111019 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGv20130417 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGv20140402 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGv20150421 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGv20151230 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGv20160406 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGv20161202 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VIKINGv20170715 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCDEEPv20230713 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCDEEPv20240506 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCDR1 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCDR2 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCDR3 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCDR4 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCDR5 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20110816 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20110909 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20120126 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20121128 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20130304 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20130805 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20140428 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20140903 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20150309 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20151218 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20160311 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20160822 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20170109 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20170411 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20171101 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20180702 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20181120 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20191212 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20210708 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20230816 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20240226 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VMCv20250130 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VVVDR1 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VVVDR2 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VVVDR5 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VVVXDR1 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
MultiframeDetector |
VVVv20110718 |
Smoothing box size for background {catalogue extension keyword: NBSIZE} |
smallint |
2 |
|
0 |
|
nbsize |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Smoothing box size for background |
smallint |
2 |
|
0 |
|
nc |
hipparcos_new_reduction |
GAIADR1 |
Number of components |
int |
4 |
|
|
meta.number |
nch_max |
masterDR2 |
SKYMAPPER |
Maximum number of child sources combined into this global object_id in any filter |
smallint |
2 |
|
|
meta.number |
NCOMB_R |
spectra |
SIXDF |
number of R frames combined |
smallint |
2 |
|
|
|
NCOMB_V |
spectra |
SIXDF |
number of V frames combined |
smallint |
2 |
|
|
|
nCombine |
MultiframeDetector |
SHARKSv20210222 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
SHARKSv20210421 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
ULTRAVISTADR4 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSDR1 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSDR2 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSDR3 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSDR4 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSDR5 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSDR6 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSDR7 |
Number of images in this stack {image extension keyword: NICOMB} |
int |
4 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSv20120926 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSv20130417 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSv20140409 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSv20150108 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSv20160114 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSv20160507 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSv20170630 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSv20180419 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSv20201209 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VHSv20231101 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIDEODR2 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIDEODR3 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIDEODR4 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIDEODR5 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIDEOv20111208 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGDR2 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGDR3 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGDR4 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGv20110714 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGv20111019 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGv20130417 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGv20140402 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGv20150421 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGv20151230 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGv20160406 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGv20161202 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VIKINGv20170715 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCDEEPv20230713 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCDEEPv20240506 |
Number of images in this stack {image extension keyword: NICOMB} |
int |
4 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCDR1 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCDR2 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCDR3 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCDR4 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCDR5 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20110816 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20110909 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20120126 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20121128 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20130304 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20130805 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20140428 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20140903 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20150309 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20151218 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20160311 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20160822 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20170109 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20170411 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20171101 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20180702 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20181120 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20191212 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20210708 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20230816 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20240226 |
Number of images in this stack {image extension keyword: NICOMB} |
int |
4 |
|
0 |
|
nCombine |
MultiframeDetector |
VMCv20250130 |
Number of images in this stack {image extension keyword: NICOMB} |
int |
4 |
|
0 |
|
nCombine |
MultiframeDetector |
VVVDR1 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VVVDR2 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VVVDR5 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VVVXDR1 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
MultiframeDetector |
VVVv20110718 |
Number of images in this stack {image extension keyword: NICOMB} |
smallint |
2 |
|
0 |
|
nCombine |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Number of images in this stack |
smallint |
2 |
|
0 |
|
nCorrelation2 |
vvvVivaCatalogue |
VVVDR5 |
Number of correlated measurements {catalogue TType keyword: Ncorrelation2} |
smallint |
2 |
|
-9999 |
|
ndet |
decapsSource |
DECAPS |
Total number of detections {catalogue TType keyword: ndet} |
smallint |
2 |
|
|
meta.number |
ndet |
smashdr2_deep, smashdr2_object |
SMASH |
Number of detections of this source (in ALLSRC) |
smallint |
2 |
|
|
|
ndet |
twomass_psc |
TWOMASS |
Frame detection statistics. |
varchar |
6 |
|
|
meta.number |
ndet |
twomass_sixx2_psc |
TWOMASS |
number of >3-sig. ap. mag measurements, # possible (jjhhkk) |
varchar |
6 |
|
|
|
ndet_lbs |
decapsSource |
DECAPS |
Number of detections {catalogue TType keyword: ndet_lbs} |
smallint |
2 |
|
-9999 |
meta.number |
ndet_lbs_ok |
decapsSource |
DECAPS |
Number of good detections {catalogue TType keyword: ndet_lbs_ok} |
smallint |
2 |
|
-9999 |
meta.number |
ndet_ok |
decapsSource |
DECAPS |
Number of good detections {catalogue TType keyword: ndet_ok} |
smallint |
2 |
|
|
meta.number |
nDetections |
ObjectThin |
PS1DR2 |
Number of single epoch detections in all filters. |
smallint |
2 |
|
-999 |
|
ndetg |
smashdr2_deep, smashdr2_object |
SMASH |
Number of detections in g |
smallint |
2 |
|
|
|
ndeti |
smashdr2_deep, smashdr2_object |
SMASH |
Number of detections in i |
smallint |
2 |
|
|
|
ndetr |
smashdr2_deep, smashdr2_object |
SMASH |
Number of detections in r |
smallint |
2 |
|
|
|
ndetu |
smashdr2_deep, smashdr2_object |
SMASH |
Number of detections in u |
smallint |
2 |
|
|
|
ndetz |
smashdr2_deep, smashdr2_object |
SMASH |
Number of detections in z |
smallint |
2 |
|
|
|
nditcor |
MultiframeDetector |
SHARKSv20210222 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
SHARKSv20210421 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
ULTRAVISTADR4 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSDR1 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSDR2 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSDR3 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSDR4 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSDR5 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSDR6 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSDR7 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSv20120926 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSv20130417 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSv20140409 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSv20150108 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSv20160114 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSv20160507 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSv20170630 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSv20180419 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSv20201209 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VHSv20231101 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIDEODR2 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIDEODR3 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIDEODR4 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIDEODR5 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIDEOv20100513 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIDEOv20111208 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGDR2 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGDR3 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGDR4 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGv20110714 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGv20111019 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGv20130417 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGv20140402 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGv20150421 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGv20151230 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGv20160406 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGv20161202 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VIKINGv20170715 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCDEEPv20230713 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCDEEPv20240506 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCDR1 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCDR2 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCDR3 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCDR4 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCDR5 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20110816 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20110909 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20120126 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20121128 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20130304 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20130805 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20140428 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20140903 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20150309 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20151218 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20160311 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20160822 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20170109 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20170411 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20171101 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20180702 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20181120 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20191212 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20210708 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20230816 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20240226 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VMCv20250130 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VVVDR1 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VVVDR2 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VVVDR5 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VVVXDR1 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VVVv20100531 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
MultiframeDetector |
VVVv20110718 |
Corrected to ndit=1 {image extension keyword: NDITCOR} |
tinyint |
1 |
|
0 |
|
nditcor |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Corrected to ndit=1 |
tinyint |
1 |
|
0 |
|
NED_CLASS |
mgcBrightSpec |
MGC |
MGC translation of NED_IDENT |
smallint |
2 |
|
|
|
NED_DEC |
mgcBrightSpec |
MGC |
NED object declination in deg (J2000) |
float |
8 |
|
|
|
NED_IDENT |
mgcBrightSpec |
MGC |
NED identification |
varchar |
4 |
|
|
|
NED_N |
mgcBrightSpec |
MGC |
Number of NED objects matched to this MGC object |
smallint |
2 |
|
|
|
NED_NAME |
mgcBrightSpec |
MGC |
NED object name |
varchar |
32 |
|
|
|
NED_RA |
mgcBrightSpec |
MGC |
NED object right ascension in deg (J2000) |
float |
8 |
|
|
|
NED_ZHELIO |
mgcBrightSpec |
MGC |
NED heliocentric redshift |
real |
4 |
|
|
|
NED_ZQUAL |
mgcBrightSpec |
MGC |
NED redshift quality |
tinyint |
1 |
|
|
|
neighboursSchema |
Programme |
SHARKSv20210222 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
SHARKSv20210421 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
ULTRAVISTADR4 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSDR1 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSDR2 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSDR3 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSDR4 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSDR5 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSDR6 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSDR7 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSv20120926 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSv20130417 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSv20150108 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSv20160114 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSv20160507 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSv20170630 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSv20180419 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSv20201209 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VHSv20231101 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIDEODR2 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIDEODR3 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIDEODR4 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIDEODR5 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIDEOv20100513 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIDEOv20111208 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGDR2 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGDR3 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGDR4 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGv20110714 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGv20111019 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGv20130417 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGv20150421 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGv20151230 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGv20160406 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGv20161202 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VIKINGv20170715 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCDEEPv20230713 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCDEEPv20240506 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCDR1 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCDR3 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCDR4 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCDR5 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20110816 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20110909 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20120126 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20121128 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20130304 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20130805 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20140428 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20140903 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20150309 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20151218 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20160311 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20160822 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20170109 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20170411 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20171101 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20180702 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20181120 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20191212 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20210708 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20230816 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20240226 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VMCv20250130 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VSAQC |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VVVDR1 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VVVDR2 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VVVDR5 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VVVXDR1 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VVVv20100531 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighboursSchema |
Programme |
VVVv20110718 |
Script file that describes the neighbour tables schema for this programme |
varchar |
64 |
|
|
?? |
neighbourTable |
RequiredNeighbours |
SHARKSv20210222 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
SHARKSv20210421 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
ULTRAVISTADR4 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSDR1 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSDR2 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSDR3 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSDR4 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSDR5 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSDR6 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSDR7 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSv20120926 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSv20130417 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSv20150108 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSv20160114 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSv20160507 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSv20170630 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSv20180419 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSv20201209 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VHSv20231101 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIDEODR2 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIDEODR3 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIDEODR4 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIDEODR5 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIDEOv20100513 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIDEOv20111208 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGDR2 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGDR3 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGDR4 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGv20110714 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGv20111019 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGv20130417 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGv20150421 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGv20151230 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGv20160406 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGv20161202 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VIKINGv20170715 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCDEEPv20230713 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCDEEPv20240506 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCDR1 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCDR3 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCDR4 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCDR5 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20110816 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20110909 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20120126 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20121128 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20130304 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20130805 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20140428 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20140903 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20150309 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20151218 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20160311 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20160822 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20170109 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20170411 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20171101 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20180702 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20181120 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20191212 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20210708 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20230816 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20240226 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VMCv20250130 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VSAQC |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VVVDR1 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VVVDR2 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VVVDR5 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VVVXDR1 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VVVv20100531 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
neighbourTable |
RequiredNeighbours |
VVVv20110718 |
the name of the neighbour join table |
varchar |
256 |
|
|
meta.id;meta.dataset |
nEpochs |
RequiredMapAverages |
SHARKSv20210222 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
SHARKSv20210421 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
ULTRAVISTADR4 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VHSDR7 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VHSv20201209 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VHSv20231101 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VMCDEEPv20230713 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VMCDEEPv20240506 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VMCDR5 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VMCv20191212 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VMCv20210708 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VMCv20230816 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VMCv20240226 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VMCv20250130 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VVVDR5 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
RequiredMapAverages |
VVVXDR1 |
Number of frames to average over |
int |
4 |
|
-99999999 |
|
nEpochs |
vmcEclipsingBinaryVariables |
VMCDR4 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20140903 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20150309 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20151218 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20160311 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20160822 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20170109 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20170411 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20171101 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20180702 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20181120 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20191212 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20210708 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20230816 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20240226 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nEpochs |
vmcEclipsingBinaryVariables |
VMCv20250130 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS} |
int |
4 |
|
|
meta.number |
nest4096 |
smashdr2_deep, smashdr2_object |
SMASH |
HEALPIX index (Nsides 4096, Nest scheme => ~52 arcsec size) |
bigint |
8 |
|
|
|
nest4096 |
smashdr2_source |
SMASH |
HEALPIX index (Nsides 4096, Nest scheme => ∼52 arcsec size |
bigint |
8 |
|
|
|
new_matched_transits |
gaia_source |
GAIAEDR3 |
The number of transits newly incorporated into an existing source in the current cycle |
smallint |
2 |
|
|
meta.number |
newFrameSet |
sharksMergeLog |
SHARKSv20210421 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
sharksMergeLog, sharksTileSet |
SHARKSv20210222 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
ultravistaMergeLog, ultravistaRemeasMergeLog, ultravistaTileSet |
ULTRAVISTADR4 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSDR2 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSDR3 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSDR4 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSDR5 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSDR6 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSDR7 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSv20120926 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSv20130417 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSv20140409 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSv20150108 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSv20160114 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSv20160507 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSv20170630 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSv20180419 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSv20201209 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog |
VHSv20231101 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vhsMergeLog, vhsTileSet |
VHSDR1 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
videoMergeLog |
VIDEODR3 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
videoMergeLog |
VIDEODR4 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
videoMergeLog |
VIDEODR5 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
videoMergeLog |
VIDEOv20100513 |
Flag used internally by curation applications |
tinyint |
1 |
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meta.code |
newFrameSet |
videoMergeLog |
VIDEOv20111208 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
videoMergeLog, videoTileSet |
VIDEODR2 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vikingMergeLog |
VIKINGDR3 |
Flag used internally by curation applications |
tinyint |
1 |
|
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meta.code |
newFrameSet |
vikingMergeLog |
VIKINGDR4 |
Flag used internally by curation applications |
tinyint |
1 |
|
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meta.code |
newFrameSet |
vikingMergeLog |
VIKINGv20110714 |
Flag used internally by curation applications |
tinyint |
1 |
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|
meta.code |
newFrameSet |
vikingMergeLog |
VIKINGv20111019 |
Flag used internally by curation applications |
tinyint |
1 |
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|
meta.code |
newFrameSet |
vikingMergeLog |
VIKINGv20130417 |
Flag used internally by curation applications |
tinyint |
1 |
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meta.code |
newFrameSet |
vikingMergeLog |
VIKINGv20140402 |
Flag used internally by curation applications |
tinyint |
1 |
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meta.code |
newFrameSet |
vikingMergeLog |
VIKINGv20150421 |
Flag used internally by curation applications |
tinyint |
1 |
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meta.code |
newFrameSet |
vikingMergeLog |
VIKINGv20151230 |
Flag used internally by curation applications |
tinyint |
1 |
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meta.code |
newFrameSet |
vikingMergeLog |
VIKINGv20160406 |
Flag used internally by curation applications |
tinyint |
1 |
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meta.code |
newFrameSet |
vikingMergeLog |
VIKINGv20161202 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vikingMergeLog |
VIKINGv20170715 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vikingMergeLog, vikingTileSet |
VIKINGDR2 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20160909 |
Flag used internally by curation applications |
tinyint |
1 |
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|
meta.code |
newFrameSet |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20170124 |
Flag used internally by curation applications |
tinyint |
1 |
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|
meta.code |
newFrameSet |
vmcMergeLog |
VMCDR2 |
Flag used internally by curation applications |
tinyint |
1 |
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meta.code |
newFrameSet |
vmcMergeLog |
VMCDR3 |
Flag used internally by curation applications |
tinyint |
1 |
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meta.code |
newFrameSet |
vmcMergeLog |
VMCDR4 |
Flag used internally by curation applications |
tinyint |
1 |
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|
meta.code |
newFrameSet |
vmcMergeLog |
VMCDR5 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20110816 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20110909 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20120126 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20121128 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20130304 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20130805 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20140428 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20140903 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20150309 |
Flag used internally by curation applications |
tinyint |
1 |
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|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20151218 |
Flag used internally by curation applications |
tinyint |
1 |
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|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20160311 |
Flag used internally by curation applications |
tinyint |
1 |
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meta.code |
newFrameSet |
vmcMergeLog |
VMCv20160822 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20170109 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20170411 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20171101 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20180702 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20181120 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20191212 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20210708 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20230816 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20240226 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog |
VMCv20250130 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcMergeLog, vmcSynopticMergeLog, vmcTileSet |
VMCDR1 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcdeepMergeLog |
VMCDEEPv20240506 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vmcdeepMergeLog, vmcdeepSynopticMergeLog, vmcdeepTileSet |
VMCDEEPv20230713 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vvvMergeLog |
VVVDR2 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vvvMergeLog |
VVVv20100531 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vvvMergeLog |
VVVv20110718 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vvvMergeLog, vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vvvMergeLog, vvvSynopticMergeLog, vvvTileSet |
VVVDR1 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newFrameSet |
vvvPsfDaophotJKsMergeLog |
VVVDR5 |
Flag used internally by curation applications |
tinyint |
1 |
|
1 |
meta.code |
newFrameSet |
vvvxMergeLog |
VVVXDR1 |
Flag used internally by curation applications |
tinyint |
1 |
|
|
meta.code |
newH_1frame |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newH_1frame |
vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this 1st Epoch H detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newH_2frame |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newH_2frame |
vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this 2nd Epoch H detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
ultravistaMergeLog, ultravistaRemeasMergeLog |
ULTRAVISTADR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vhsMergeLog |
VHSDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vhsMergeLog |
VHSDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSDR6 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSDR7 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSv20120926 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vhsMergeLog |
VHSv20130417 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vhsMergeLog |
VHSv20140409 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSv20150108 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSv20160114 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSv20160507 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSv20170630 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSv20180419 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSv20201209 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vhsMergeLog |
VHSv20231101 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
videoMergeLog |
VIDEODR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
videoMergeLog |
VIDEODR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
videoMergeLog |
VIDEODR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
videoMergeLog |
VIDEODR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
videoMergeLog |
VIDEOv20100513 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
videoMergeLog |
VIDEOv20111208 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vikingMergeLog |
VIKINGDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vikingMergeLog |
VIKINGDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vikingMergeLog |
VIKINGDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vikingMergeLog |
VIKINGv20110714 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vikingMergeLog |
VIKINGv20111019 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vikingMergeLog |
VIKINGv20130417 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vikingMergeLog |
VIKINGv20140402 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vikingMergeLog |
VIKINGv20150421 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vikingMergeLog |
VIKINGv20151230 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vikingMergeLog |
VIKINGv20160406 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vikingMergeLog |
VIKINGv20161202 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vikingMergeLog |
VIKINGv20170715 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20160909 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20170124 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vvvMergeLog |
VVVDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newHframe |
vvvMergeLog |
VVVv20100531 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vvvMergeLog |
VVVv20110718 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vvvMergeLog, vvvSynopticMergeLog |
VVVDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newHframe |
vvvxMergeLog |
VVVXDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.H |
newJ_1frame |
vikingMergeLog |
VIKINGv20151230 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJ_1frame |
vikingMergeLog |
VIKINGv20160406 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJ_1frame |
vikingMergeLog |
VIKINGv20161202 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJ_1frame |
vikingMergeLog |
VIKINGv20170715 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJ_1frame |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJ_1frame |
vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this 1st Epoch J detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJ_1frame |
vvvxMergeLog |
VVVXDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJ_2frame |
vikingMergeLog |
VIKINGv20151230 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJ_2frame |
vikingMergeLog |
VIKINGv20160406 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJ_2frame |
vikingMergeLog |
VIKINGv20161202 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJ_2frame |
vikingMergeLog |
VIKINGv20170715 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJ_2frame |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJ_2frame |
vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this 2nd Epoch J detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJ_2frame |
vvvxMergeLog |
VVVXDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
ultravistaMergeLog, ultravistaRemeasMergeLog |
ULTRAVISTADR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vhsMergeLog |
VHSDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vhsMergeLog |
VHSDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSDR6 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSDR7 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSv20120926 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vhsMergeLog |
VHSv20130417 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vhsMergeLog |
VHSv20140409 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSv20150108 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSv20160114 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSv20160507 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSv20170630 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSv20180419 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSv20201209 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vhsMergeLog |
VHSv20231101 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
videoMergeLog |
VIDEODR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
videoMergeLog |
VIDEODR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
videoMergeLog |
VIDEODR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
videoMergeLog |
VIDEODR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
videoMergeLog |
VIDEOv20100513 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
videoMergeLog |
VIDEOv20111208 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vikingMergeLog |
VIKINGDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vikingMergeLog |
VIKINGDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vikingMergeLog |
VIKINGDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vikingMergeLog |
VIKINGv20110714 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vikingMergeLog |
VIKINGv20111019 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vikingMergeLog |
VIKINGv20130417 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vikingMergeLog |
VIKINGv20140402 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vikingMergeLog |
VIKINGv20150421 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vikingMergeLog |
VIKINGv20151230 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vikingMergeLog |
VIKINGv20160406 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vikingMergeLog |
VIKINGv20161202 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vikingMergeLog |
VIKINGv20170715 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20160909 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20170124 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vmcMergeLog |
VMCDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vmcMergeLog |
VMCDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20110816 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vmcMergeLog |
VMCv20110909 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vmcMergeLog |
VMCv20120126 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vmcMergeLog |
VMCv20121128 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vmcMergeLog |
VMCv20130304 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vmcMergeLog |
VMCv20130805 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vmcMergeLog |
VMCv20140428 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20140903 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20150309 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20151218 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20160311 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20160822 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20170109 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20170411 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20171101 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20180702 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20181120 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20191212 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20210708 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20230816 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20240226 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog |
VMCv20250130 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcMergeLog, vmcSynopticMergeLog |
VMCDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vmcdeepMergeLog |
VMCDEEPv20240506 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vmcdeepMergeLog, vmcdeepSynopticMergeLog |
VMCDEEPv20230713 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vvvMergeLog |
VVVDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newJframe |
vvvMergeLog |
VVVv20100531 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vvvMergeLog |
VVVv20110718 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vvvMergeLog, vvvSynopticMergeLog |
VVVDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newJframe |
vvvPsfDaophotJKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
1 |
meta.code;em.IR.J |
newJframe |
vvvxMergeLog |
VVVXDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.J |
newKS_1frame |
vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this 1st Epoch Ks detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKs_1frame |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKs_1frame |
vvvxMergeLog |
VVVXDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKS_2frame |
vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this 2nd Epoch Ks detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKs_2frame |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKs_2frame |
vvvxMergeLog |
VVVXDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
sharksMergeLog |
SHARKSv20210222 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
sharksMergeLog |
SHARKSv20210421 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
ultravistaMergeLog, ultravistaRemeasMergeLog |
ULTRAVISTADR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vhsMergeLog |
VHSDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vhsMergeLog |
VHSDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSDR6 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSDR7 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSv20120926 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vhsMergeLog |
VHSv20130417 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vhsMergeLog |
VHSv20140409 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSv20150108 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSv20160114 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSv20160507 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSv20170630 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSv20180419 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSv20201209 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vhsMergeLog |
VHSv20231101 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
videoMergeLog |
VIDEODR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
videoMergeLog |
VIDEODR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
videoMergeLog |
VIDEODR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
videoMergeLog |
VIDEODR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
videoMergeLog |
VIDEOv20100513 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
videoMergeLog |
VIDEOv20111208 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vikingMergeLog |
VIKINGDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vikingMergeLog |
VIKINGDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vikingMergeLog |
VIKINGDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vikingMergeLog |
VIKINGv20110714 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vikingMergeLog |
VIKINGv20111019 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vikingMergeLog |
VIKINGv20130417 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vikingMergeLog |
VIKINGv20140402 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vikingMergeLog |
VIKINGv20150421 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vikingMergeLog |
VIKINGv20151230 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vikingMergeLog |
VIKINGv20160406 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vikingMergeLog |
VIKINGv20161202 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vikingMergeLog |
VIKINGv20170715 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20160909 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20170124 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vmcMergeLog |
VMCDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vmcMergeLog |
VMCDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20110816 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vmcMergeLog |
VMCv20110909 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vmcMergeLog |
VMCv20120126 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vmcMergeLog |
VMCv20121128 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vmcMergeLog |
VMCv20130304 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vmcMergeLog |
VMCv20130805 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vmcMergeLog |
VMCv20140428 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20140903 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20150309 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20151218 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20160311 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20160822 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20170109 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20170411 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20171101 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20180702 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20181120 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20191212 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20210708 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20230816 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20240226 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog |
VMCv20250130 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcMergeLog, vmcSynopticMergeLog |
VMCDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vmcdeepMergeLog |
VMCDEEPv20240506 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vmcdeepMergeLog, vmcdeepSynopticMergeLog |
VMCDEEPv20230713 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vvvMergeLog |
VVVDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newKsframe |
vvvMergeLog |
VVVv20100531 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vvvMergeLog |
VVVv20110718 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vvvMergeLog, vvvSynopticMergeLog |
VVVDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newKsframe |
vvvPsfDaophotJKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
1 |
meta.code;em.IR.K |
newKsframe |
vvvxMergeLog |
VVVXDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.K |
newlyIngested |
Multiframe |
SHARKSv20210222 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
SHARKSv20210421 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
ULTRAVISTADR4 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSDR1 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSDR2 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSDR3 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSDR4 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSDR5 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSDR6 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSDR7 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSv20120926 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSv20130417 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSv20140409 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSv20150108 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSv20160114 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSv20160507 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSv20170630 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSv20180419 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSv20201209 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VHSv20231101 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIDEODR2 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIDEODR3 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIDEODR4 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIDEODR5 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIDEOv20100513 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIDEOv20111208 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGDR2 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGDR3 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGDR4 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGv20110714 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGv20111019 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGv20130417 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGv20140402 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGv20150421 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGv20151230 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGv20160406 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGv20161202 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VIKINGv20170715 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCDEEPv20230713 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCDEEPv20240506 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCDR1 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCDR2 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCDR3 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCDR4 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCDR5 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20110816 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20110909 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20120126 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20121128 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20130304 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20130805 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20140428 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20140903 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20150309 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20151218 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20160311 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20160822 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20170109 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20170411 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20171101 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20180702 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20181120 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20191212 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20210708 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20230816 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20240226 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VMCv20250130 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VVVDR1 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VVVDR2 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VVVDR5 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VVVXDR1 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VVVv20100531 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
Multiframe |
VVVv20110718 |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newlyIngested |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Curation flag for internal use only (0=no, 1=yes) |
tinyint |
1 |
|
1 |
?? |
newNb118frame |
ultravistaMergeLog, ultravistaRemeasMergeLog |
ULTRAVISTADR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newY_1frame |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newY_1frame |
vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this 1st Epoch Y detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newY_2frame |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newY_2frame |
vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this 2nd Epoch Y detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
ultravistaMergeLog, ultravistaRemeasMergeLog |
ULTRAVISTADR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vhsMergeLog |
VHSDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vhsMergeLog |
VHSDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSDR6 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSDR7 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSv20120926 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vhsMergeLog |
VHSv20130417 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vhsMergeLog |
VHSv20140409 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSv20150108 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSv20160114 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSv20160507 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSv20170630 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSv20180419 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSv20201209 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vhsMergeLog |
VHSv20231101 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
videoMergeLog |
VIDEODR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
videoMergeLog |
VIDEODR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
videoMergeLog |
VIDEODR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
videoMergeLog |
VIDEODR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
videoMergeLog |
VIDEOv20100513 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
videoMergeLog |
VIDEOv20111208 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vikingMergeLog |
VIKINGDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vikingMergeLog |
VIKINGDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vikingMergeLog |
VIKINGDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vikingMergeLog |
VIKINGv20110714 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vikingMergeLog |
VIKINGv20111019 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vikingMergeLog |
VIKINGv20130417 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vikingMergeLog |
VIKINGv20140402 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vikingMergeLog |
VIKINGv20150421 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vikingMergeLog |
VIKINGv20151230 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vikingMergeLog |
VIKINGv20160406 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vikingMergeLog |
VIKINGv20161202 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vikingMergeLog |
VIKINGv20170715 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20160909 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20170124 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vmcMergeLog |
VMCDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vmcMergeLog |
VMCDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20110816 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vmcMergeLog |
VMCv20110909 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
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|
meta.code |
newYframe |
vmcMergeLog |
VMCv20120126 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
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|
meta.code |
newYframe |
vmcMergeLog |
VMCv20121128 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
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|
meta.code |
newYframe |
vmcMergeLog |
VMCv20130304 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vmcMergeLog |
VMCv20130805 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vmcMergeLog |
VMCv20140428 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20140903 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20150309 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20151218 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20160311 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20160822 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20170109 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20170411 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20171101 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20180702 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20181120 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20191212 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20210708 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20230816 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20240226 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog |
VMCv20250130 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vmcMergeLog, vmcSynopticMergeLog |
VMCDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vvvMergeLog |
VVVDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.IR.NIR |
newYframe |
vvvMergeLog |
VVVv20100531 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vvvMergeLog |
VVVv20110718 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newYframe |
vvvMergeLog, vvvSynopticMergeLog |
VVVDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZ_1frame |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZ_1frame |
vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this 1st Epoch Z detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZ_2frame |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZ_2frame |
vvvPsfDophotZYJHKsMergeLog |
VVVDR5 |
new/old flag (1/0) of this 2nd Epoch Z detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZframe |
videoMergeLog |
VIDEODR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
videoMergeLog |
VIDEODR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
videoMergeLog |
VIDEODR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZframe |
videoMergeLog |
VIDEODR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZframe |
videoMergeLog |
VIDEOv20100513 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
videoMergeLog |
VIDEOv20111208 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vikingMergeLog |
VIKINGDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vikingMergeLog |
VIKINGDR3 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vikingMergeLog |
VIKINGDR4 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZframe |
vikingMergeLog |
VIKINGv20110714 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vikingMergeLog |
VIKINGv20111019 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vikingMergeLog |
VIKINGv20130417 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vikingMergeLog |
VIKINGv20140402 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vikingMergeLog |
VIKINGv20150421 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZframe |
vikingMergeLog |
VIKINGv20151230 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZframe |
vikingMergeLog |
VIKINGv20160406 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZframe |
vikingMergeLog |
VIKINGv20161202 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZframe |
vikingMergeLog |
VIKINGv20170715 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZframe |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20160909 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vikingZY_selJ_RemeasMergeLog |
VIKINGZYSELJv20170124 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vvvMergeLog |
VVVDR2 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vvvMergeLog |
VVVDR5 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code;em.opt.I |
newZframe |
vvvMergeLog |
VVVv20100531 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vvvMergeLog |
VVVv20110718 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
newZframe |
vvvMergeLog, vvvSynopticMergeLog |
VVVDR1 |
new/old flag (1/0) of this detector image |
tinyint |
1 |
|
|
meta.code |
nFlag |
rosat_bsc, rosat_fsc |
ROSAT |
nearby sources affecting SASS flux determination |
varchar |
1 |
|
|
meta.code |
nFrames |
sharksVariability |
SHARKSv20210222 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
sharksVariability |
SHARKSv20210421 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
ultravistaVariability |
ULTRAVISTADR4 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
videoVariability |
VIDEODR2 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
videoVariability |
VIDEODR3 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
videoVariability |
VIDEODR4 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
videoVariability |
VIDEODR5 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
videoVariability |
VIDEOv20100513 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
videoVariability |
VIDEOv20111208 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGDR2 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGDR3 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGDR4 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGv20110714 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGv20111019 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGv20130417 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGv20140402 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGv20150421 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGv20151230 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGv20160406 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGv20161202 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vikingVariability |
VIKINGv20170715 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCDR1 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCDR2 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCDR3 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCDR4 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCDR5 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20110816 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20110909 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20120126 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20121128 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20130304 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20130805 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20140428 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20140903 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20150309 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20151218 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20160311 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20160822 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20170109 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20170411 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20171101 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20180702 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20181120 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20191212 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20210708 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20230816 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20240226 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcVariability |
VMCv20250130 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcdeepVariability |
VMCDEEPv20230713 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vmcdeepVariability |
VMCDEEPv20240506 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vvvVariability |
VVVDR1 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vvvVariability |
VVVDR2 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vvvVariability |
VVVDR5 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vvvVariability |
VVVv20100531 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vvvVariability |
VVVv20110718 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
nFrames |
vvvxVariability |
VVVXDR1 |
Number of frames with good detections used to calculate astrometric fits |
int |
4 |
|
0 |
meta.number |
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. |
ng |
ObjectThin |
PS1DR2 |
Number of single epoch detections in g filter. |
smallint |
2 |
|
-999 |
|
NGOOD |
spectra |
SIXDF |
number of good emission lines |
int |
4 |
|
|
|
ngood |
masterDR2 |
SKYMAPPER |
Number of observations used across all filters |
smallint |
2 |
|
|
meta.number |
ngood_min |
masterDR2 |
SKYMAPPER |
Minimum number of observations used in any filter (excluding filters with 0 observations) |
smallint |
2 |
|
|
meta.number |
nGoodMeasurements |
vvvVivaCatalogue |
VVVDR5 |
Number of good measurements found in the Ks pawprint data {catalogue TType keyword: NgoodMeasurements} |
smallint |
2 |
|
-9999 |
|
ngrp |
allwise_sc |
WISE |
Excess number of positionally associated duplicate resolution groups in which this extractions was included. Values of ngrp>0 indicate that the source was associated with more than one possible group. CAUTION: In the All-Sky Release Catalog and 3-Band Cryo Source Working Database, this column indicated the total number of groups with which a source was associated. In the AllWISE Catalog and Reject Table, ngrp is the total number of groups minus one. |
smallint |
2 |
|
|
|
ngrp |
wise_allskysc |
WISE |
Number of positionally associated duplicate resolution groups in which this extractions was included. |
smallint |
2 |
|
-9999 |
|
nhcon |
iras_psc |
IRAS |
Number of times observed (<25) |
tinyint |
1 |
|
|
meta.number |
Ni |
ravedr5Source |
RAVE |
[Ni/H] abundance of Ni |
real |
4 |
dex |
|
phys.abund.Z |
ni |
ObjectThin |
PS1DR2 |
Number of single epoch detections in i filter. |
smallint |
2 |
|
-999 |
|
Ni_N |
ravedr5Source |
RAVE |
Number of used spectral lines in calc. of [Ni/H] |
smallint |
2 |
|
|
meta.number |
nId |
iras_psc |
IRAS |
Number of positional associations (<25). |
tinyint |
1 |
|
|
meta.number |
night_key |
twomass_xsc |
TWOMASS |
key to night data record in "scan DB". |
smallint |
2 |
|
|
meta.id |
nightZPCat |
MultiframeDetector |
SHARKSv20210222 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
SHARKSv20210421 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
ULTRAVISTADR4 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSDR1 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSDR2 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSDR3 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSDR4 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSDR5 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSDR6 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSDR7 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSv20120926 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSv20130417 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSv20140409 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSv20150108 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSv20160114 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSv20160507 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSv20170630 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSv20180419 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSv20201209 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VHSv20231101 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIDEODR2 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIDEODR3 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIDEODR4 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIDEODR5 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIDEOv20100513 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIDEOv20111208 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGDR2 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGDR3 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGDR4 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGv20110714 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGv20111019 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGv20130417 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGv20140402 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGv20150421 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGv20151230 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGv20160406 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGv20161202 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VIKINGv20170715 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCDEEPv20230713 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCDEEPv20240506 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCDR1 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCDR2 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCDR3 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCDR4 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCDR5 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20110816 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20110909 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20120126 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20121128 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20130304 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20130805 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20140428 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20140903 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20150309 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20151218 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20160311 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20160822 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20170109 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20170411 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20171101 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20180702 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20181120 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20191212 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20210708 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20230816 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20240226 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VMCv20250130 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VVVDR1 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VVVDR2 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VVVDR5 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VVVXDR1 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VVVv20100531 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
MultiframeDetector |
VVVv20110718 |
Average photometric zero point for night {catalogue extension keyword: NIGHTZPT} |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
SHARKSv20210222 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
SHARKSv20210421 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
ULTRAVISTADR4 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSDR1 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSDR2 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSDR3 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSDR4 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSDR5 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSDR6 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSDR7 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSv20120926 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSv20130417 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSv20140409 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSv20150108 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSv20160114 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSv20160507 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSv20170630 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSv20180419 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSv20201209 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VHSv20231101 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIDEODR2 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIDEODR3 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIDEODR4 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIDEODR5 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIDEOv20100513 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIDEOv20111208 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGDR2 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGDR3 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGDR4 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGv20110714 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGv20111019 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGv20130417 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGv20140402 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGv20150421 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGv20151230 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGv20160406 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGv20161202 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VIKINGv20170715 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCDEEPv20230713 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCDEEPv20240506 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCDR1 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCDR2 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCDR3 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCDR4 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCDR5 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20110816 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20110909 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20120126 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20121128 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20130304 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20130805 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20140428 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20140903 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20150309 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20151218 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20160311 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20160822 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20170109 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20170411 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20171101 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20180702 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20181120 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20191212 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20210708 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20230816 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20240226 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VMCv20250130 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VVVDR1 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VVVDR2 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VVVDR5 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VVVXDR1 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VVVv20100531 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
PreviousMFDZP |
VVVv20110718 |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPCat |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Average photometric zero point for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
SHARKSv20210222 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
SHARKSv20210421 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
ULTRAVISTADR4 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSDR1 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSDR2 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSDR3 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSDR4 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSDR5 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSDR6 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSDR7 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSv20120926 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSv20130417 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSv20140409 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSv20150108 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSv20160114 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSv20160507 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSv20170630 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSv20180419 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSv20201209 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VHSv20231101 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIDEODR2 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIDEODR3 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIDEODR4 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIDEODR5 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIDEOv20100513 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIDEOv20111208 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGDR2 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGDR3 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGDR4 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGv20110714 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGv20111019 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGv20130417 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGv20140402 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGv20150421 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGv20151230 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGv20160406 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGv20161202 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VIKINGv20170715 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCDEEPv20230713 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCDEEPv20240506 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCDR1 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCDR2 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCDR3 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCDR4 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCDR5 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20110816 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20110909 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20120126 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20121128 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20130304 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20130805 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20140428 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20140903 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20150309 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20151218 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20160311 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20160822 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20170109 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20170411 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20171101 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20180702 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20181120 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20191212 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20210708 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20230816 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20240226 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VMCv20250130 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VVVDR1 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VVVDR2 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VVVDR5 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VVVXDR1 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VVVv20100531 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
MultiframeDetector |
VVVv20110718 |
Photometric zero point sigma for night {catalogue extension keyword: NIGHTZRR} <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
SHARKSv20210222 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
SHARKSv20210421 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
ULTRAVISTADR4 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSDR1 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSDR2 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSDR3 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSDR4 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSDR5 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSDR6 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSDR7 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSv20120926 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSv20130417 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSv20140409 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSv20150108 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSv20160114 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSv20160507 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSv20170630 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSv20180419 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSv20201209 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VHSv20231101 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIDEODR2 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIDEODR3 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIDEODR4 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIDEODR5 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIDEOv20100513 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIDEOv20111208 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGDR2 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGDR3 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGDR4 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGv20110714 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGv20111019 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGv20130417 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGv20140402 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGv20150421 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGv20151230 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGv20160406 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGv20161202 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VIKINGv20170715 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCDEEPv20230713 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCDEEPv20240506 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCDR1 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCDR2 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCDR3 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCDR4 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCDR5 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20110816 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20110909 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20120126 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20121128 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20130304 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20130805 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20140428 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20140903 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20150309 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20151218 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20160311 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20160822 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20170109 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20170411 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20171101 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20180702 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20181120 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20191212 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20210708 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20230816 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20240226 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VMCv20250130 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VVVDR1 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VVVDR2 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VVVDR5 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VVVXDR1 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VVVv20100531 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
PreviousMFDZP |
VVVv20110718 |
Photometric zero point sigma for night <0.05 mags for a good night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPErrCat |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Photometric zero point sigma for night |
real |
4 |
mags |
-0.9999995e9 |
?? |
nightZPNum |
MultiframeDetector |
SHARKSv20210222 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
SHARKSv20210421 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
ULTRAVISTADR4 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSDR1 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSDR2 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSDR3 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSDR4 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSDR5 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSDR6 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSDR7 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSv20120926 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSv20130417 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSv20140409 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSv20150108 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSv20160114 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSv20160507 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSv20170630 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSv20180419 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSv20201209 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VHSv20231101 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIDEODR2 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIDEODR3 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIDEODR4 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIDEODR5 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIDEOv20100513 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIDEOv20111208 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGDR2 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGDR3 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGDR4 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGv20110714 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGv20111019 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGv20130417 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGv20140402 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGv20150421 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGv20151230 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGv20160406 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGv20161202 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VIKINGv20170715 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCDEEPv20230713 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCDEEPv20240506 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCDR1 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCDR2 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCDR3 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCDR4 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCDR5 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20110816 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20110909 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20120126 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20121128 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20130304 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20130805 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20140428 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20140903 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20150309 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20151218 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20160311 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20160822 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20170109 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20170411 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20171101 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20180702 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20181120 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20191212 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20210708 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20230816 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20240226 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VMCv20250130 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VVVDR1 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VVVDR2 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VVVDR5 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VVVXDR1 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VVVv20100531 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
MultiframeDetector |
VVVv20110718 |
Number of ZP in band used to calculate nightZPCat {catalogue extension keyword: NIGHTNUM} |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
SHARKSv20210222 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
SHARKSv20210421 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
ULTRAVISTADR4 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSDR1 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSDR2 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSDR3 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSDR4 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSDR5 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSDR6 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSDR7 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSv20120926 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSv20130417 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSv20140409 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSv20150108 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSv20160114 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSv20160507 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSv20170630 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSv20180419 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSv20201209 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VHSv20231101 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIDEODR2 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIDEODR3 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIDEODR4 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIDEODR5 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIDEOv20100513 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIDEOv20111208 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGDR2 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGDR3 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGDR4 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGv20110714 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGv20111019 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGv20130417 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGv20140402 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGv20150421 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGv20151230 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGv20160406 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGv20161202 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VIKINGv20170715 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCDEEPv20230713 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCDEEPv20240506 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCDR1 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCDR2 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCDR3 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCDR4 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCDR5 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20110816 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20110909 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20120126 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20121128 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20130304 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20130805 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20140428 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20140903 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20150309 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20151218 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20160311 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20160822 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20170109 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20170411 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20171101 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20180702 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20181120 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20191212 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20210708 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20230816 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20240226 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VMCv20250130 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VVVDR1 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VVVDR2 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VVVDR5 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VVVXDR1 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VVVv20100531 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
PreviousMFDZP |
VVVv20110718 |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nightZPNum |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Number of ZP in band used to calculate nightZPCat |
int |
4 |
mags |
-99999999 |
?? |
nimaflags |
masterDR2 |
SKYMAPPER |
Total number of flagged pixels from bad, saturated, and crosstalk pixel masks across all observations |
int |
4 |
|
|
meta.code |
nInFrameset |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Number of frames in the frameSet linked in MapProvenance |
int |
4 |
|
|
|
nIters |
catwise_2020, catwise_prelim |
WISE |
number of chi-square-minimization iterations |
int |
4 |
|
|
|
nIters_pm |
catwise_2020, catwise_prelim |
WISE |
number of chi-square-minimization iterations |
int |
4 |
|
|
|
nJ |
vmcPsfCatalogue |
VMCDR3 |
Number of stars used to calculate the completeness in J {catalogue TType keyword: nJ} |
int |
4 |
|
-99999999 |
|
nJ |
vmcPsfCatalogue |
VMCDR4 |
Number of stars used to calculate the completeness in J {catalogue TType keyword: nJ} |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfCatalogue |
VMCv20140903 |
Number of stars used to calculate the completeness in J {catalogue TType keyword: nJ} |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfCatalogue |
VMCv20150309 |
Number of stars used to calculate the completeness in J {catalogue TType keyword: nJ} |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfCatalogue |
VMCv20151218 |
Number of stars used to calculate the completeness in J {catalogue TType keyword: nJ} |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfCatalogue |
VMCv20160311 |
Number of stars used to calculate the completeness in J {catalogue TType keyword: nJ} |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfCatalogue |
VMCv20160822 |
Number of stars used to calculate the completeness in J {catalogue TType keyword: nJ} |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfCatalogue |
VMCv20170109 |
Number of stars used to calculate the completeness in J {catalogue TType keyword: nJ} |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfCatalogue |
VMCv20170411 |
Number of stars used to calculate the completeness in J {catalogue TType keyword: nJ} |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfCatalogue |
VMCv20171101 |
Number of stars used to calculate the completeness in J {catalogue TType keyword: nJ} |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfSource |
VMCDR5 |
Number of stars used to calculate the completeness in J |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfSource |
VMCv20180702 |
Number of stars used to calculate the completeness in J |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfSource |
VMCv20181120 |
Number of stars used to calculate the completeness in J |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfSource |
VMCv20191212 |
Number of stars used to calculate the completeness in J |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfSource |
VMCv20210708 |
Number of stars used to calculate the completeness in J |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfSource |
VMCv20230816 |
Number of stars used to calculate the completeness in J |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfSource |
VMCv20240226 |
Number of stars used to calculate the completeness in J |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJ |
vmcPsfSource |
VMCv20250130 |
Number of stars used to calculate the completeness in J |
int |
4 |
|
-99999999 |
meta.number;em.IR.J |
nJEpochs |
vmcRRLyraeVariables |
VMCv20240226 |
Number of epochs in the J-band {catalogue TType keyword: NJ} |
int |
4 |
|
|
meta.number |
njitter |
Multiframe |
SHARKSv20210222 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
SHARKSv20210421 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
ULTRAVISTADR4 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSDR1 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSDR2 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSDR3 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSDR4 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSDR5 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSDR6 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSDR7 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSv20120926 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSv20130417 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSv20140409 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSv20150108 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSv20160114 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSv20160507 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSv20170630 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSv20180419 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSv20201209 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VHSv20231101 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIDEODR2 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIDEODR3 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIDEODR4 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIDEODR5 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIDEOv20100513 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIDEOv20111208 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGDR2 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGDR3 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGDR4 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGv20110714 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGv20111019 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGv20130417 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGv20140402 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGv20150421 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGv20151230 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGv20160406 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGv20161202 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VIKINGv20170715 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCDEEPv20230713 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCDEEPv20240506 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCDR1 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCDR2 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCDR3 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCDR4 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCDR5 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20110816 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20110909 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20120126 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20121128 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20130304 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20130805 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20140428 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20140903 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20150309 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20151218 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20160311 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20160822 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20170109 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20170411 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20171101 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20180702 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20181120 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20191212 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20210708 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20230816 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20240226 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VMCv20250130 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VVVDR1 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VVVDR2 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VVVDR5 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VVVXDR1 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VVVv20100531 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
Multiframe |
VVVv20110718 |
Number of jitter positions {image primary HDU keyword: NJITTER} |
smallint |
2 |
|
-9999 |
|
njitter |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Number of jitter positions |
smallint |
2 |
|
-9999 |
|
nKs |
vmcPsfCatalogue |
VMCDR3 |
Number of stars used to calculate the completeness in Ks {catalogue TType keyword: nKs} |
int |
4 |
|
-99999999 |
|
nKs |
vmcPsfCatalogue |
VMCDR4 |
Number of stars used to calculate the completeness in Ks {catalogue TType keyword: nKs} |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfCatalogue |
VMCv20140903 |
Number of stars used to calculate the completeness in Ks {catalogue TType keyword: nKs} |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfCatalogue |
VMCv20150309 |
Number of stars used to calculate the completeness in Ks {catalogue TType keyword: nKs} |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfCatalogue |
VMCv20151218 |
Number of stars used to calculate the completeness in Ks {catalogue TType keyword: nKs} |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfCatalogue |
VMCv20160311 |
Number of stars used to calculate the completeness in Ks {catalogue TType keyword: nKs} |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfCatalogue |
VMCv20160822 |
Number of stars used to calculate the completeness in Ks {catalogue TType keyword: nKs} |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfCatalogue |
VMCv20170109 |
Number of stars used to calculate the completeness in Ks {catalogue TType keyword: nKs} |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfCatalogue |
VMCv20170411 |
Number of stars used to calculate the completeness in Ks {catalogue TType keyword: nKs} |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfCatalogue |
VMCv20171101 |
Number of stars used to calculate the completeness in Ks {catalogue TType keyword: nKs} |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfSource |
VMCDR5 |
Number of stars used to calculate the completeness in Ks |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfSource |
VMCv20180702 |
Number of stars used to calculate the completeness in Ks |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfSource |
VMCv20181120 |
Number of stars used to calculate the completeness in Ks |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfSource |
VMCv20191212 |
Number of stars used to calculate the completeness in Ks |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfSource |
VMCv20210708 |
Number of stars used to calculate the completeness in Ks |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfSource |
VMCv20230816 |
Number of stars used to calculate the completeness in Ks |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfSource |
VMCv20240226 |
Number of stars used to calculate the completeness in Ks |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKs |
vmcPsfSource |
VMCv20250130 |
Number of stars used to calculate the completeness in Ks |
int |
4 |
|
-99999999 |
meta.number;em.IR.K |
nKsEpochs |
vmcRRLyraeVariables |
VMCv20240226 |
Number of epochs in the Ks-band {catalogue TType keyword: NKs} |
int |
4 |
|
|
meta.number |
nKsEpochs |
vmcRRlyraeVariables |
VMCDR4 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS_KS} |
int |
4 |
|
|
meta.number |
nKsEpochs |
vmcRRlyraeVariables |
VMCv20160822 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS_KS} |
int |
4 |
|
|
meta.number |
nKsEpochs |
vmcRRlyraeVariables |
VMCv20170109 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS_KS} |
int |
4 |
|
|
meta.number |
nKsEpochs |
vmcRRlyraeVariables |
VMCv20170411 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS_KS} |
int |
4 |
|
|
meta.number |
nKsEpochs |
vmcRRlyraeVariables |
VMCv20171101 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS_KS} |
int |
4 |
|
|
meta.number |
nKsEpochs |
vmcRRlyraeVariables |
VMCv20180702 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS_KS} |
int |
4 |
|
|
meta.number |
nKsEpochs |
vmcRRlyraeVariables |
VMCv20181120 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS_KS} |
int |
4 |
|
|
meta.number |
nKsEpochs |
vmcRRlyraeVariables |
VMCv20191212 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS_KS} |
int |
4 |
|
|
meta.number |
nKsEpochs |
vmcRRlyraeVariables |
VMCv20210708 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS_KS} |
int |
4 |
|
|
meta.number |
nKsEpochs |
vmcRRlyraeVariables |
VMCv20230816 |
Number of epochs in the Ks-band {catalogue TType keyword: N_EPOCHS_KS} |
int |
4 |
|
|
meta.number |
nLrs |
iras_psc |
IRAS |
Number of significant LRS spectra |
tinyint |
1 |
|
|
meta.number |
NMBEST |
spectra |
SIXDF |
emission lines for emission z |
int |
4 |
|
|
|
nMeasurements |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Number used in average. |
int |
4 |
|
|
|
noffsets |
Multiframe |
SHARKSv20210222 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
SHARKSv20210421 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
ULTRAVISTADR4 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSDR1 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSDR2 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSDR3 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSDR4 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSDR5 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSDR6 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSDR7 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSv20120926 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSv20130417 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSv20140409 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSv20150108 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSv20160114 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSv20160507 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSv20170630 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSv20180419 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSv20201209 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VHSv20231101 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIDEODR2 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIDEODR3 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIDEODR4 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIDEODR5 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIDEOv20100513 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIDEOv20111208 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGDR2 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGDR3 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGDR4 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGv20110714 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGv20111019 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGv20130417 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGv20140402 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGv20150421 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGv20151230 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGv20160406 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGv20161202 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VIKINGv20170715 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCDEEPv20230713 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCDEEPv20240506 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCDR1 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCDR2 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCDR3 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCDR4 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCDR5 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20110816 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20110909 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20120126 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20121128 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20130304 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20130805 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20140428 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20140903 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20150309 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20151218 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20160311 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20160822 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20170109 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20170411 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20171101 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20180702 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20181120 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20191212 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20210708 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20230816 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20240226 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VMCv20250130 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VVVDR1 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VVVDR2 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VVVDR5 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VVVXDR1 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VVVv20100531 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
Multiframe |
VVVv20110718 |
Number of offset positions {image primary HDU keyword: NOFFSETS} |
smallint |
2 |
|
-9999 |
|
noffsets |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Number of offset positions |
smallint |
2 |
|
-9999 |
|
NOISE_R |
spectra |
SIXDF |
R readout noise |
real |
4 |
|
|
|
NOISE_v |
spectra |
SIXDF |
V readout noise |
real |
4 |
|
|
|
nonperp |
sharksAstrometricInfo |
SHARKSv20210222 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
sharksAstrometricInfo |
SHARKSv20210421 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
ultravistaAstrometricInfo |
ULTRAVISTADR4 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vhsAstrometricInfo |
VHSDR6 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vhsAstrometricInfo |
VHSDR7 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vhsAstrometricInfo |
VHSv20170630 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vhsAstrometricInfo |
VHSv20180419 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vhsAstrometricInfo |
VHSv20201209 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vhsAstrometricInfo |
VHSv20231101 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
videoAstrometricInfo |
VIDEODR2 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
?? |
nonperp |
videoAstrometricInfo |
VIDEODR3 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
videoAstrometricInfo |
VIDEODR4 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
videoAstrometricInfo |
VIDEODR5 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
videoAstrometricInfo |
VIDEOv20111208 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
?? |
nonperp |
vikingAstrometricInfo |
VIKINGDR2 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
?? |
nonperp |
vikingAstrometricInfo |
VIKINGDR3 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vikingAstrometricInfo |
VIKINGDR4 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vikingAstrometricInfo |
VIKINGv20110714 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
?? |
nonperp |
vikingAstrometricInfo |
VIKINGv20111019 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
?? |
nonperp |
vikingAstrometricInfo |
VIKINGv20130417 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vikingAstrometricInfo |
VIKINGv20140402 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vikingAstrometricInfo |
VIKINGv20150421 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vikingAstrometricInfo |
VIKINGv20151230 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vikingAstrometricInfo |
VIKINGv20160406 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vikingAstrometricInfo |
VIKINGv20161202 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vikingAstrometricInfo |
VIKINGv20170715 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCDR1 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
?? |
nonperp |
vmcAstrometricInfo |
VMCDR2 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCDR3 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCDR4 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCDR5 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20110816 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
?? |
nonperp |
vmcAstrometricInfo |
VMCv20110909 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
?? |
nonperp |
vmcAstrometricInfo |
VMCv20120126 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
?? |
nonperp |
vmcAstrometricInfo |
VMCv20121128 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20130304 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20130805 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20140428 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20140903 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20150309 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20151218 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20160311 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20160822 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20170109 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20170411 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20171101 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20180702 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20181120 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20191212 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20210708 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20230816 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20240226 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcAstrometricInfo |
VMCv20250130 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcdeepAstrometricInfo |
VMCDEEPv20230713 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vmcdeepAstrometricInfo |
VMCDEEPv20240506 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vvvAstrometricInfo |
VVVDR1 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vvvAstrometricInfo |
VVVDR2 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
pos.posAng |
nonperp |
vvvAstrometricInfo |
VVVDR5 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nonperp |
vvvAstrometricInfo |
VVVv20110718 |
Non-perpendicularity of axes |
float |
8 |
degrees |
-0.9999995e9 |
?? |
nonperp |
vvvxAstrometricInfo |
VVVXDR1 |
Non-perpendicularity of axes |
float |
8 |
radians |
-0.9999995e9 |
pos.posAng |
nopt_mchs |
twomass_psc |
TWOMASS |
The number of USNO-A2.0 or Tycho 2 optical sources found within a 5" radius of the TWOMASS position. |
smallint |
2 |
|
|
meta.number |
normSoft |
MapCatalogueDetector |
SHARKSv20210222 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
SHARKSv20210421 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
ULTRAVISTADR4 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VHSDR7 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VHSv20201209 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VHSv20231101 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VMCDEEPv20230713 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VMCDEEPv20240506 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VMCDR5 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VMCv20191212 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VMCv20210708 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VMCv20230816 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VMCv20240226 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VMCv20250130 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VVVDR5 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
normSoft |
MapCatalogueDetector |
VVVXDR1 |
Normalised softening parameter (averaged for tiles) for luptitude calculation {catalogue TType keyword: NORMSOFT} |
float |
8 |
|
|
|
notes |
vmcCepheidVariables |
VMCDR3 |
Additional information, a means that the star was not used to derive the PL, PW and PLC relations. {catalogue TType keyword: Notes} |
varchar |
8 |
|
NONE |
meta.code.qual |
notes |
vmcCepheidVariables |
VMCDR4 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: Notes} |
varchar |
8 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20121128 |
Additional information, a means that the star was not used to derive the PL, PW and PLC relations. {catalogue TType keyword: Notes} |
varchar |
8 |
|
NONE |
meta.code.qual |
notes |
vmcCepheidVariables |
VMCv20140428 |
Additional information, a means that the star was not used to derive the PL, PW and PLC relations. {catalogue TType keyword: Notes} |
varchar |
8 |
|
NONE |
meta.code.qual |
notes |
vmcCepheidVariables |
VMCv20140903 |
Additional information, a means that the star was not used to derive the PL, PW and PLC relations. {catalogue TType keyword: Notes} |
varchar |
8 |
|
NONE |
meta.code.qual |
notes |
vmcCepheidVariables |
VMCv20150309 |
Additional information, a means that the star was not used to derive the PL, PW and PLC relations. {catalogue TType keyword: Notes} |
varchar |
8 |
|
NONE |
meta.code.qual |
notes |
vmcCepheidVariables |
VMCv20151218 |
Additional information, a means that the star was not used to derive the PL, PW and PLC relations. {catalogue TType keyword: Notes} |
varchar |
8 |
|
NONE |
meta.code.qual |
notes |
vmcCepheidVariables |
VMCv20160311 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: Notes} |
varchar |
8 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20160822 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: Notes} |
varchar |
8 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20170109 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: FLAG} |
varchar |
16 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20170411 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: FLAG} |
varchar |
16 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20171101 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: FLAG} |
varchar |
16 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20180702 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: FLAG} |
varchar |
16 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20181120 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: FLAG} |
varchar |
16 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20191212 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: FLAG} |
varchar |
16 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20210708 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: FLAG} |
varchar |
16 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20230816 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: FLAG} |
varchar |
16 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcCepheidVariables |
VMCv20240226 |
Additional information of flag assigned using the PW(V,Ks) as reference relation. {catalogue TType keyword: FLAG} |
varchar |
16 |
|
NONE |
meta.code.qual |
The notes have changed from the first data release of Cepheids pre-2016 to the second 2016 onwards. For Cepheids with a cuEventID=11199, have the following in notes: Additional information, a means that the star was not used to derive the PL, PW and PLC relations. For later data, (cuEventID>500000), the following is notes are used: Flag assigned using the PW(V,Ks) as reference relation. The first part of the table includes all stars with flag = 0 ordered by increasing period. The second part includes all stars with flag>0, sorted by increasing period. 0 = no remark; 1 = overluminous star with separation between VMC and OGLE III position larger than 0.2 arcsec; 2 = largely scattered or under-sampled light curve; 3 = Remarks OGLE III; 4 = Remarks VMC; 5 = Saturation; 10 = F-mode outliers without evident explanation; 11 = FO-mode outliers without evident explanation; 12 = V band lacking. |
notes |
vmcEclipsingBinaryVariables |
VMCDR4 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20140903 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20150309 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20151218 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20160311 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20160822 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20170109 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20170411 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20171101 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20180702 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20181120 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20191212 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20210708 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20230816 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20240226 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
notes |
vmcEclipsingBinaryVariables |
VMCv20250130 |
More details from EROS-2 ("cont.-like", "non-contact") or OGLEIII (checked by GRATIS "ch" or not "n/c" ) {catalogue TType keyword: TYPE} |
varchar |
16 |
|
NONE |
meta.code.qual |
The type of eclipsing binary. If the data is from EROS-2, the options are "cont.-like" or "non-contact" and if the data is from OGLEIII then the type is from a GRATIS checkand the options are "ch" or not "n/c". |
nPass |
RequiredFilters |
SHARKSv20210222 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
SHARKSv20210421 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
ULTRAVISTADR4 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSDR1 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSDR2 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSDR3 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSDR4 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSDR5 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSDR6 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSDR7 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSv20120926 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSv20130417 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSv20150108 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSv20160114 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSv20160507 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSv20170630 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSv20180419 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSv20201209 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VHSv20231101 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIDEODR2 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIDEODR3 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIDEODR4 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIDEODR5 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIDEOv20100513 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIDEOv20111208 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGDR2 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGDR3 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGDR4 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGv20110714 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGv20111019 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGv20130417 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGv20150421 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGv20151230 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGv20160406 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGv20161202 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VIKINGv20170715 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCDEEPv20230713 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCDEEPv20240506 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCDR1 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCDR3 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCDR4 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCDR5 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20110816 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20110909 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20120126 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20121128 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20130304 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20130805 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20140428 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20140903 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20150309 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20151218 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20160311 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20160822 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20170109 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20170411 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20171101 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20180702 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20181120 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20191212 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20210708 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20230816 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20240226 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VMCv20250130 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VSAQC |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VVVDR1 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VVVDR2 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VVVDR5 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VVVXDR1 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VVVv20100531 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
nPass |
RequiredFilters |
VVVv20110718 |
the number of passes that will be made |
smallint |
2 |
|
|
meta.number |
npoints |
machoLMCSource, machoSMCSource |
MACHO |
number of observations on the MACHO tile containing this star |
smallint |
2 |
|
|
|
nr |
ObjectThin |
PS1DR2 |
Number of single epoch detections in r filter. |
smallint |
2 |
|
-999 |
|
nRows |
ExternalProductCatalogue |
VMCv20250130 |
Number of rows in the file |
bigint |
8 |
|
-99999999 |
|
nStackDetections |
ObjectThin |
PS1DR2 |
Number of stack detections. |
smallint |
2 |
|
-999 |
|
nStackObjectRows |
ObjectThin |
PS1DR2 |
Number of independent StackObjectThin rows associated with this object. |
smallint |
2 |
|
-999 |
|
nSteps |
catwise_2020, catwise_prelim |
WISE |
number of steps in all iterations |
int |
4 |
|
|
|
nSteps_pm |
catwise_2020, catwise_prelim |
WISE |
number of steps in all iterations |
int |
4 |
|
|
|
ntr |
hipparcos_new_reduction |
GAIADR1 |
Number of field transits used |
int |
4 |
|
|
meta.id;obs.field |
nu_eff_used_in_astrometry |
gaia_source |
GAIAEDR3 |
Effective wavenumber of the source used in the astrometric solution |
real |
4 |
micron^-1 |
|
em.wavenumber |
num |
tycho2 |
GAIADR1 |
NUmber of positions used |
smallint |
2 |
|
|
meta.number |
num_harmonics_for_p1 |
cepheid, rrlyrae |
GAIADR1 |
Number of harmonics used to model P1 of the light curve |
int |
4 |
|
|
meta.number |
num_observations_processed |
phot_variable_time_series_g_fov_statistical_parameters |
GAIADR1 |
Number of processed G-band observations for variability analysis |
int |
4 |
|
|
meta.number |
numAxes |
MultiframeDetector |
SHARKSv20210222 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
SHARKSv20210421 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
ULTRAVISTADR4 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSDR1 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSDR2 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSDR3 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSDR4 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSDR5 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSDR6 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSDR7 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSv20120926 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSv20130417 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSv20140409 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSv20150108 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSv20160114 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSv20160507 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSv20170630 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSv20180419 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSv20201209 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VHSv20231101 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIDEODR2 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIDEODR3 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIDEODR4 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIDEODR5 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIDEOv20100513 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIDEOv20111208 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGDR2 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGDR3 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGDR4 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGv20110714 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGv20111019 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGv20130417 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGv20140402 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGv20150421 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGv20151230 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGv20160406 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGv20161202 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VIKINGv20170715 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCDEEPv20230713 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCDEEPv20240506 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCDR1 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCDR2 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCDR3 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCDR4 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCDR5 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20110816 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20110909 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20120126 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20121128 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20130304 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20130805 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20140428 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20140903 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20150309 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20151218 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20160311 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20160822 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20170109 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20170411 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20171101 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20180702 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20181120 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20191212 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20210708 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20230816 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20240226 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VMCv20250130 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VVVDR1 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VVVDR2 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VVVDR5 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VVVXDR1 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VVVv20100531 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
MultiframeDetector |
VVVv20110718 |
Number of data axes; eg. 2 |
tinyint |
1 |
|
0 |
meta.number |
numAxes |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Number of data axes; eg. 2 |
tinyint |
1 |
|
|
meta.number |
NumberBands |
vmcBackgroundSources |
VMCv20250130 |
Number of photometric bands in the SED {catalogue TType keyword: No_bands} |
smallint |
2 |
|
-9999 |
meta.number |
numberStk |
RequiredStack |
SHARKSv20210222 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
SHARKSv20210421 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
ULTRAVISTADR4 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSDR1 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSDR2 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSDR3 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSDR4 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSDR5 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSDR6 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSDR7 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSv20120926 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSv20130417 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSv20150108 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSv20160114 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSv20160507 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSv20170630 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSv20180419 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSv20201209 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VHSv20231101 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIDEODR2 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIDEODR3 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIDEODR4 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIDEODR5 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIDEOv20100513 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIDEOv20111208 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGDR2 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGDR3 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGDR4 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGv20110714 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGv20111019 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGv20130417 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGv20150421 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGv20151230 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGv20160406 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGv20161202 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VIKINGv20170715 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCDEEPv20230713 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCDEEPv20240506 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCDR1 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCDR3 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCDR4 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCDR5 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20110816 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20110909 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20120126 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20121128 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20130304 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20130805 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20140428 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20140903 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20150309 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20151218 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20160311 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20160822 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20170109 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20170411 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20171101 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20180702 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20181120 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20191212 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20210708 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20230816 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20240226 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VMCv20250130 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VSAQC |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VVVDR1 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VVVDR2 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VVVDR5 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VVVXDR1 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VVVv20100531 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numberStk |
RequiredStack |
VVVv20110718 |
Number of intermediate stacks. If default, stack all good quality stacks |
int |
4 |
|
-99999999 |
|
numDetectors |
Multiframe |
SHARKSv20210222 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
SHARKSv20210421 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
ULTRAVISTADR4 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSDR1 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSDR2 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSDR3 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSDR4 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSDR5 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSDR6 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSDR7 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSv20120926 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSv20130417 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSv20140409 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSv20150108 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSv20160114 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSv20160507 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSv20170630 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSv20180419 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSv20201209 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VHSv20231101 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIDEODR2 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIDEODR3 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIDEODR4 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIDEODR5 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIDEOv20100513 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIDEOv20111208 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGDR2 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGDR3 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGDR4 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGv20110714 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGv20111019 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGv20130417 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGv20140402 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGv20150421 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGv20151230 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGv20160406 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGv20161202 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VIKINGv20170715 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCDEEPv20230713 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCDEEPv20240506 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCDR1 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCDR2 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCDR3 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCDR4 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCDR5 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20110816 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20110909 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20120126 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20121128 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20130304 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20130805 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20140428 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20140903 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20150309 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20151218 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20160311 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20160822 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20170109 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20170411 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20171101 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20180702 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20181120 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20191212 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20210708 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20230816 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20240226 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VMCv20250130 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VVVDR1 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VVVDR2 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VVVDR5 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VVVXDR1 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VVVv20100531 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
Multiframe |
VVVv20110718 |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
0 |
?? |
numDetectors |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
The number of "detectors" (=image extensions in FITS file) |
tinyint |
1 |
|
|
?? |
numRms |
CurrentAstrometry |
SHARKSv20210222 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
SHARKSv20210421 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
ULTRAVISTADR4 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSDR1 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSDR2 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSDR3 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSDR4 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSDR5 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSDR6 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSDR7 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSv20120926 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSv20130417 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSv20140409 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSv20150108 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSv20160114 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSv20160507 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSv20170630 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSv20180419 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSv20201209 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VHSv20231101 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIDEODR2 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIDEODR3 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIDEODR4 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIDEODR5 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIDEOv20100513 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIDEOv20111208 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGDR2 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGDR3 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGDR4 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGv20110714 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGv20111019 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGv20130417 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGv20140402 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGv20150421 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGv20151230 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGv20160406 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGv20161202 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VIKINGv20170715 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCDEEPv20230713 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCDEEPv20240506 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCDR1 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCDR2 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCDR3 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCDR4 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCDR5 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20110816 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20110909 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20120126 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20121128 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20130304 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20130805 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20140428 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20140903 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20150309 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20151218 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20160311 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20160822 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20170109 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20170411 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20171101 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20180702 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20181120 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20191212 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20210708 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20230816 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20240226 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VMCv20250130 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VVVDR1 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VVVDR2 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VVVDR5 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VVVXDR1 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VVVv20100531 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
CurrentAstrometry |
VVVv20110718 |
No. of astrometric standards used in fit {image extension keyword: NUMBRMS} |
int |
4 |
|
-99999999 |
stat.fit.param |
numRms |
sharksCurrentAstrometry, ultravistaCurrentAstrometry, vhsCurrentAstrometry, videoCurrentAstrometry, vikingCurrentAstrometry, vmcCurrentAstrometry, vvvCurrentAstrometry |
VSAQC |
No. of astrometric standards used in fit |
int |
4 |
|
-99999999 |
stat.fit.param |
numZPCat |
MultiframeDetector |
SHARKSv20210222 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
SHARKSv20210421 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
ULTRAVISTADR4 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSDR1 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSDR2 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSDR3 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSDR4 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSDR5 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSDR6 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSDR7 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSv20120926 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSv20130417 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSv20140409 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSv20150108 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSv20160114 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSv20160507 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSv20170630 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSv20180419 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSv20201209 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VHSv20231101 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIDEODR2 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIDEODR3 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIDEODR4 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIDEODR5 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIDEOv20100513 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIDEOv20111208 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGDR2 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGDR3 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGDR4 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGv20110714 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGv20111019 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGv20130417 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGv20140402 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGv20150421 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGv20151230 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGv20160406 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGv20161202 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VIKINGv20170715 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCDEEPv20230713 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCDEEPv20240506 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCDR1 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCDR2 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCDR3 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCDR4 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCDR5 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20110816 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20110909 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20120126 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20121128 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20130304 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20130805 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20140428 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20140903 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20150309 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20151218 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20160311 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20160822 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20170109 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20170411 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20171101 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20180702 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20181120 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20191212 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20210708 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20230816 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20240226 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VMCv20250130 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VVVDR1 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VVVDR2 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VVVDR5 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VVVXDR1 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VVVv20100531 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
MultiframeDetector |
VVVv20110718 |
Number of standards used in determining photZPCat and photZPCatErr {catalogue extension keyword: NUMZPT} |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
SHARKSv20210222 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
SHARKSv20210421 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
ULTRAVISTADR4 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSDR1 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSDR2 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSDR3 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSDR4 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSDR5 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSDR6 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSDR7 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSv20120926 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSv20130417 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSv20140409 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSv20150108 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSv20160114 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSv20160507 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSv20170630 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSv20180419 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSv20201209 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VHSv20231101 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIDEODR2 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIDEODR3 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIDEODR4 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIDEODR5 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIDEOv20100513 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIDEOv20111208 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGDR2 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGDR3 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGDR4 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGv20110714 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGv20111019 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGv20130417 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGv20140402 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGv20150421 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGv20151230 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGv20160406 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGv20161202 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VIKINGv20170715 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCDEEPv20230713 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCDEEPv20240506 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCDR1 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCDR2 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCDR3 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCDR4 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCDR5 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20110816 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20110909 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20120126 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20121128 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20130304 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20130805 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20140428 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20140903 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20150309 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20151218 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20160311 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20160822 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20170109 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20170411 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20171101 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20180702 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20181120 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20191212 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20210708 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20230816 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20240226 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VMCv20250130 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VVVDR1 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VVVDR2 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VVVDR5 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VVVXDR1 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VVVv20100531 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
PreviousMFDZP |
VVVv20110718 |
Number of standards used in determining photZP and photZPErr |
int |
4 |
|
-99999999 |
|
numZPCat |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Number of standards used in determining photZPCat and photZPCatErr |
int |
4 |
|
-99999999 |
|
nuStep |
Multiframe |
SHARKSv20210222 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
SHARKSv20210421 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
ULTRAVISTADR4 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSDR1 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSDR2 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSDR3 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSDR4 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSDR5 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSDR6 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSDR7 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSv20120926 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSv20130417 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSv20140409 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSv20150108 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSv20160114 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSv20160507 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSv20170630 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSv20180419 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSv20201209 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VHSv20231101 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIDEODR2 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIDEODR3 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIDEODR4 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIDEODR5 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIDEOv20100513 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIDEOv20111208 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGDR2 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGDR3 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGDR4 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGv20110714 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGv20111019 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGv20130417 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGv20140402 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGv20150421 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGv20151230 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGv20160406 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGv20161202 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VIKINGv20170715 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCDEEPv20230713 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCDEEPv20240506 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCDR1 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCDR2 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCDR3 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCDR4 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCDR5 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20110816 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20110909 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20120126 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20121128 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20130304 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20130805 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20140428 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20140903 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20150309 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20151218 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20160311 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20160822 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20170109 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20170411 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20171101 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20180702 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20181120 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20191212 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20210708 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20230816 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20240226 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VMCv20250130 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VVVDR1 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VVVDR2 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VVVDR5 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VVVXDR1 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VVVv20100531 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
Multiframe |
VVVv20110718 |
Number of microstep positions {image primary HDU keyword: NUSTEP} |
tinyint |
1 |
|
0 |
|
nuStep |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Number of microstep positions |
tinyint |
1 |
|
0 |
|
nustep |
RequiredMosaic |
SHARKSv20210421 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
ULTRAVISTADR4 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSDR1 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSDR2 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSDR3 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSDR4 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSDR5 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSDR6 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSDR7 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSv20120926 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSv20130417 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSv20150108 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSv20160114 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSv20160507 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSv20170630 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSv20180419 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSv20201209 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VHSv20231101 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIDEODR2 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIDEODR3 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIDEODR4 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIDEODR5 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIDEOv20100513 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIDEOv20111208 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGDR2 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGDR3 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGDR4 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGv20110714 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGv20111019 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGv20130417 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGv20150421 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGv20151230 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGv20160406 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGv20161202 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VIKINGv20170715 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCDEEPv20230713 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCDEEPv20240506 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCDR1 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCDR3 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCDR4 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCDR5 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20110816 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20110909 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20120126 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20121128 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20130304 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20130805 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20140428 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20140903 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20150309 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20151218 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20160311 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20160822 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20170109 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20170411 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20171101 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20180702 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20181120 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20191212 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20210708 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20230816 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20240226 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VMCv20250130 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VVVDR1 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VVVDR2 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VVVDR5 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VVVXDR1 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VVVv20100531 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic |
VVVv20110718 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredMosaic, RequiredTile |
SHARKSv20210222 |
Amount of microstepping |
tinyint |
1 |
|
|
?? |
nustep |
RequiredStack |
SHARKSv20210222 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
SHARKSv20210421 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
ULTRAVISTADR4 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSDR1 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSDR2 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSDR3 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSDR4 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSDR5 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSDR6 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSDR7 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSv20120926 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSv20130417 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSv20150108 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSv20160114 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSv20160507 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSv20170630 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSv20180419 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSv20201209 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VHSv20231101 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIDEODR2 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIDEODR3 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIDEODR4 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIDEODR5 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIDEOv20100513 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIDEOv20111208 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGDR2 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGDR3 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGDR4 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGv20110714 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGv20111019 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGv20130417 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGv20150421 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGv20151230 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGv20160406 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGv20161202 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VIKINGv20170715 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCDEEPv20230713 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCDEEPv20240506 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCDR1 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCDR3 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCDR4 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCDR5 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20110816 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20110909 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20120126 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20121128 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20130304 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20130805 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20140428 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20140903 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20150309 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20151218 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20160311 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20160822 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20170109 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20170411 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20171101 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20180702 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20181120 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20191212 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20210708 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20230816 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20240226 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VMCv20250130 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VSAQC |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VVVDR1 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VVVDR2 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VVVDR5 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VVVXDR1 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VVVv20100531 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
nustep |
RequiredStack |
VVVv20110718 |
Amount of microstepping |
tinyint |
1 |
|
0 |
?? |
NVSS |
nvssSource |
NVSS |
Source name |
varchar |
14 |
|
|
meta.id;meta.main |
nY |
vmcPsfCatalogue |
VMCDR3 |
Number of stars used to calculate the completeness in Y {catalogue TType keyword: nY} |
int |
4 |
|
-99999999 |
|
nY |
vmcPsfCatalogue |
VMCDR4 |
Number of stars used to calculate the completeness in Y {catalogue TType keyword: nY} |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfCatalogue |
VMCv20140903 |
Number of stars used to calculate the completeness in Y {catalogue TType keyword: nY} |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfCatalogue |
VMCv20150309 |
Number of stars used to calculate the completeness in Y {catalogue TType keyword: nY} |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfCatalogue |
VMCv20151218 |
Number of stars used to calculate the completeness in Y {catalogue TType keyword: nY} |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfCatalogue |
VMCv20160311 |
Number of stars used to calculate the completeness in Y {catalogue TType keyword: nY} |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfCatalogue |
VMCv20160822 |
Number of stars used to calculate the completeness in Y {catalogue TType keyword: nY} |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfCatalogue |
VMCv20170109 |
Number of stars used to calculate the completeness in Y {catalogue TType keyword: nY} |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfCatalogue |
VMCv20170411 |
Number of stars used to calculate the completeness in Y {catalogue TType keyword: nY} |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfCatalogue |
VMCv20171101 |
Number of stars used to calculate the completeness in Y {catalogue TType keyword: nY} |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfSource |
VMCDR5 |
Number of stars used to calculate the completeness in Y |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfSource |
VMCv20180702 |
Number of stars used to calculate the completeness in Y |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfSource |
VMCv20181120 |
Number of stars used to calculate the completeness in Y |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfSource |
VMCv20191212 |
Number of stars used to calculate the completeness in Y |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfSource |
VMCv20210708 |
Number of stars used to calculate the completeness in Y |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfSource |
VMCv20230816 |
Number of stars used to calculate the completeness in Y |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfSource |
VMCv20240226 |
Number of stars used to calculate the completeness in Y |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
nY |
vmcPsfSource |
VMCv20250130 |
Number of stars used to calculate the completeness in Y |
int |
4 |
|
-99999999 |
meta.number;em.IR.NIR |
ny |
ObjectThin |
PS1DR2 |
Number of single epoch detections in y filter. |
smallint |
2 |
|
-999 |
|
nYEpochs |
vmcRRLyraeVariables |
VMCv20240226 |
Number of epochs in the Y-band {catalogue TType keyword: NY} |
int |
4 |
|
|
meta.number |
nz |
ObjectThin |
PS1DR2 |
Number of single epoch detections in z filter. |
smallint |
2 |
|
-999 |
|