S |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
S14 |
nvssSource |
NVSS |
Integrated 1.4GHz flux density of radio source |
real |
4 |
mJy |
|
phot.flux.density;em.radio.750-1500MHz |
S145Mag |
combo17CDFSSource |
COMBO17 |
Absolute restframe magnitude in 145/10 (synthetic narrow rectangular passband at 140-150 nm calculated from redshifted best_fit template, only calculated for objects classified as quasars) |
real |
4 |
mag |
|
|
S280Mag |
combo17CDFSSource |
COMBO17 |
Absolute restframe magnitude in 280/40 (calculated from redshifted best_fit template, depending on redshift and filter extrapolation outside the COMBO-17 filter set can be necessary, only calculated for objects classified as galaxies; synthetic UV continuum rectangular passband at 260-300 nm) |
real |
4 |
mag |
|
|
s_hp |
hipparcos_new_reduction |
GAIADR1 |
Scatter in Hipparcos magnitudes |
float |
8 |
mag |
|
stat.error;phot.mag;em.opt |
sadtAreaID |
MultiframeEsoKeys |
SHARKSv20210222 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
SHARKSv20210421 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
ULTRAVISTADR4 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSDR1 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSDR2 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSDR3 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSDR4 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSDR5 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSDR6 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20120926 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20130417 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20140409 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20150108 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20160114 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20160507 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20170630 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20180419 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20201209 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20231101 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VHSv20240731 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIDEODR2 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIDEODR3 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIDEODR4 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIDEODR5 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIDEOv20111208 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGDR2 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGDR3 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGDR4 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGv20110714 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGv20111019 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGv20130417 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGv20140402 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGv20150421 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGv20151230 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGv20160406 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGv20161202 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VIKINGv20170715 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCDEEPv20230713 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCDEEPv20240506 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCDR1 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCDR2 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCDR3 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCDR4 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCDR5 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20110816 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20110909 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20120126 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20121128 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20130304 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20130805 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20140428 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20140903 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20150309 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20151218 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20160311 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20160822 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20170109 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20170411 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20171101 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20180702 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20181120 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20191212 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20210708 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20230816 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VMCv20240226 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VSAQC |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VVVDR1 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VVVDR2 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VVVDR5 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VVVXDR1 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtAreaID |
MultiframeEsoKeys |
VVVv20110718 |
SADT Survey area ID {image primary HDU keyword: HIERARCH ESO OCS SADT AREA ID} |
int |
4 |
|
-99999999 |
|
sadtMaxJit |
MultiframeEsoKeys |
SHARKSv20210222 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
SHARKSv20210421 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
ULTRAVISTADR4 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSDR1 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSDR2 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSDR3 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSDR4 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSDR5 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSDR6 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20120926 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20130417 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20140409 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20150108 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20160114 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20160507 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20170630 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20180419 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20201209 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20231101 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VHSv20240731 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIDEODR2 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIDEODR3 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIDEODR4 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIDEODR5 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIDEOv20111208 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGDR2 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGDR3 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGDR4 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGv20110714 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGv20111019 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGv20130417 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGv20140402 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGv20150421 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGv20151230 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGv20160406 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGv20161202 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VIKINGv20170715 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCDEEPv20230713 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCDEEPv20240506 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCDR1 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCDR2 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCDR3 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCDR4 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCDR5 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20110816 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20110909 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20120126 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20121128 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20130304 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20130805 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20140428 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20140903 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20150309 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20151218 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20160311 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20160822 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20170109 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20170411 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20171101 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20180702 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20181120 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20191212 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20210708 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20230816 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VMCv20240226 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VSAQC |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VVVDR1 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VVVDR2 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VVVDR5 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VVVXDR1 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtMaxJit |
MultiframeEsoKeys |
VVVv20110718 |
SADT maximum jitter size {image primary HDU keyword: HIERARCH ESO OCS SADT MAXJIT} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
SHARKSv20210222 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
SHARKSv20210421 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
ULTRAVISTADR4 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSDR1 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSDR2 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSDR3 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSDR4 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSDR5 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSDR6 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20120926 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20130417 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20140409 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20150108 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20160114 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20160507 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20170630 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20180419 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20201209 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20231101 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VHSv20240731 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIDEODR2 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIDEODR3 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIDEODR4 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIDEODR5 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIDEOv20111208 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGDR2 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGDR3 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGDR4 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGv20110714 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGv20111019 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGv20130417 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGv20140402 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGv20150421 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGv20151230 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGv20160406 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGv20161202 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VIKINGv20170715 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCDEEPv20230713 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCDEEPv20240506 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCDR1 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCDR2 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCDR3 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCDR4 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCDR5 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20110816 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20110909 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20120126 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20121128 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20130304 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20130805 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20140428 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20140903 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20150309 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20151218 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20160311 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20160822 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20170109 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20170411 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20171101 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20180702 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20181120 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20191212 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20210708 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20230816 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VMCv20240226 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VSAQC |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VVVDR1 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VVVDR2 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VVVDR5 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VVVXDR1 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapX |
MultiframeEsoKeys |
VVVv20110718 |
SADT tile overlap in X {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPX} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
SHARKSv20210222 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
SHARKSv20210421 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
ULTRAVISTADR4 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSDR1 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSDR2 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSDR3 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSDR4 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSDR5 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSDR6 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20120926 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20130417 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20140409 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20150108 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20160114 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20160507 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20170630 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20180419 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20201209 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20231101 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VHSv20240731 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIDEODR2 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIDEODR3 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIDEODR4 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIDEODR5 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIDEOv20111208 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGDR2 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGDR3 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGDR4 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGv20110714 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGv20111019 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGv20130417 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGv20140402 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGv20150421 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGv20151230 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGv20160406 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGv20161202 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VIKINGv20170715 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCDEEPv20230713 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCDEEPv20240506 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCDR1 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCDR2 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCDR3 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCDR4 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCDR5 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20110816 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20110909 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20120126 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20121128 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20130304 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20130805 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20140428 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20140903 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20150309 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20151218 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20160311 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20160822 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20170109 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20170411 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20171101 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20180702 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20181120 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20191212 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20210708 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20230816 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VMCv20240226 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VSAQC |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VVVDR1 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VVVDR2 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VVVDR5 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VVVXDR1 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtOverlapY |
MultiframeEsoKeys |
VVVv20110718 |
SADT tile overlap in Y {image primary HDU keyword: HIERARCH ESO OCS SADT OVERLAPY} |
real |
4 |
arcsec |
-0.9999995e9 |
|
sadtPattern |
MultiframeEsoKeys |
SHARKSv20210222 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
SHARKSv20210421 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
ULTRAVISTADR4 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSDR1 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSDR2 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSDR3 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSDR4 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSDR5 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSDR6 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20120926 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20130417 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20140409 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20150108 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20160114 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20160507 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20170630 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20180419 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20201209 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20231101 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VHSv20240731 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIDEODR2 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIDEODR3 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIDEODR4 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIDEODR5 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIDEOv20111208 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGDR2 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGDR3 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGDR4 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGv20110714 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGv20111019 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGv20130417 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGv20140402 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGv20150421 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGv20151230 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGv20160406 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGv20161202 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VIKINGv20170715 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCDEEPv20230713 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCDEEPv20240506 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCDR1 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCDR2 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCDR3 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCDR4 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCDR5 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20110816 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20110909 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20120126 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20121128 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20130304 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20130805 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20140428 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20140903 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20150309 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20151218 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20160311 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20160822 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20170109 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20170411 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20171101 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20180702 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20181120 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20191212 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20210708 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20230816 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VMCv20240226 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VSAQC |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VVVDR1 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VVVDR2 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VVVDR5 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VVVXDR1 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtPattern |
MultiframeEsoKeys |
VVVv20110718 |
SADT pattern ID {image primary HDU keyword: HIERARCH ESO OCS SADT PATTERN} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
SHARKSv20210222 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
SHARKSv20210421 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
ULTRAVISTADR4 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSDR1 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSDR2 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSDR3 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSDR4 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSDR5 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSDR6 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20120926 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20130417 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20140409 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20150108 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20160114 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20160507 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20170630 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20180419 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20201209 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20231101 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VHSv20240731 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIDEODR2 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIDEODR3 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIDEODR4 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIDEODR5 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIDEOv20111208 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGDR2 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGDR3 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGDR4 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGv20110714 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGv20111019 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGv20130417 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGv20140402 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGv20150421 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGv20151230 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGv20160406 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGv20161202 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VIKINGv20170715 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCDEEPv20230713 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCDEEPv20240506 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCDR1 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCDR2 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCDR3 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCDR4 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCDR5 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20110816 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20110909 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20120126 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20121128 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20130304 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20130805 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20140428 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20140903 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20150309 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20151218 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20160311 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20160822 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20170109 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20170411 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20171101 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20180702 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20181120 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20191212 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20210708 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20230816 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VMCv20240226 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VSAQC |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VVVDR1 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VVVDR2 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VVVDR5 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VVVXDR1 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtSurveyID |
MultiframeEsoKeys |
VVVv20110718 |
SADT survey ID {image primary HDU keyword: HIERARCH ESO OCS SADT ID} |
varchar |
64 |
|
NONE |
|
sadtTileDec |
MultiframeEsoKeys |
SHARKSv20210222 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
SHARKSv20210421 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
ULTRAVISTADR4 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSDR1 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSDR2 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSDR3 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSDR4 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSDR5 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSDR6 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20120926 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20130417 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20140409 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20150108 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20160114 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20160507 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20170630 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20180419 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20201209 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20231101 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VHSv20240731 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIDEODR2 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIDEODR3 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIDEODR4 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIDEODR5 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIDEOv20111208 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGDR2 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGDR3 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGDR4 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGv20110714 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGv20111019 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGv20130417 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGv20140402 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGv20150421 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGv20151230 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGv20160406 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGv20161202 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VIKINGv20170715 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCDEEPv20230713 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCDEEPv20240506 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCDR1 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCDR2 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCDR3 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCDR4 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCDR5 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20110816 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20110909 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20120126 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20121128 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20130304 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20130805 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20140428 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20140903 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20150309 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20151218 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20160311 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20160822 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20170109 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20170411 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20171101 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20180702 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20181120 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20191212 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20210708 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20230816 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VMCv20240226 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VSAQC |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VVVDR1 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VVVDR2 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VVVDR5 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VVVXDR1 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileDec |
MultiframeEsoKeys |
VVVv20110718 |
SADT tile declination {image primary HDU keyword: HIERARCH ESO OCS SADT TILE DEC} |
real |
4 |
DDMMSS.TTT |
-0.9999995e9 |
|
sadtTileID |
MultiframeEsoKeys |
SHARKSv20210222 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
SHARKSv20210421 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
ULTRAVISTADR4 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSDR1 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSDR2 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSDR3 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSDR4 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSDR5 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSDR6 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20120926 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20130417 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20140409 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20150108 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20160114 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20160507 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20170630 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20180419 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20201209 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20231101 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VHSv20240731 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIDEODR2 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIDEODR3 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIDEODR4 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIDEODR5 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIDEOv20111208 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGDR2 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGDR3 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGDR4 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGv20110714 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGv20111019 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGv20130417 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGv20140402 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGv20150421 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGv20151230 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGv20160406 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGv20161202 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VIKINGv20170715 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCDEEPv20230713 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCDEEPv20240506 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCDR1 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCDR2 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCDR3 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCDR4 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCDR5 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20110816 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20110909 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20120126 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20121128 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20130304 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20130805 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20140428 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20140903 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20150309 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20151218 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20160311 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20160822 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20170109 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20170411 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20171101 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20180702 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20181120 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20191212 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20210708 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20230816 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VMCv20240226 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VSAQC |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VVVDR1 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VVVDR2 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VVVDR5 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VVVXDR1 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileID |
MultiframeEsoKeys |
VVVv20110718 |
SADT tile ID within survey area {image primary HDU keyword: HIERARCH ESO OCS SADT TILE ID} |
varchar |
64 |
|
NONE |
|
sadtTileOffAngle |
MultiframeEsoKeys |
SHARKSv20210222 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
SHARKSv20210421 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
ULTRAVISTADR4 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSDR1 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSDR2 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSDR3 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSDR4 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSDR5 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSDR6 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20120926 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20130417 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20140409 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20150108 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20160114 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20160507 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20170630 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20180419 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20201209 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20231101 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VHSv20240731 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIDEODR2 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIDEODR3 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIDEODR4 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIDEODR5 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIDEOv20111208 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGDR2 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGDR3 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGDR4 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGv20110714 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGv20111019 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGv20130417 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGv20140402 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGv20150421 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGv20151230 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGv20160406 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGv20161202 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VIKINGv20170715 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCDEEPv20230713 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCDEEPv20240506 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCDR1 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCDR2 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCDR3 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCDR4 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCDR5 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20110816 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20110909 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20120126 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20121128 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20130304 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20130805 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20140428 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20140903 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20150309 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20151218 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20160311 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20160822 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20170109 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20170411 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20171101 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20180702 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20181120 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20191212 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20210708 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20230816 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VMCv20240226 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VSAQC |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VVVDR1 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VVVDR2 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VVVDR5 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VVVXDR1 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileOffAngle |
MultiframeEsoKeys |
VVVv20110718 |
SADT tile rotator offset angle {image primary HDU keyword: HIERARCH ESO OCS SADT TILE OFFANGLE} |
real |
4 |
deg |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
SHARKSv20210222 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
SHARKSv20210421 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
ULTRAVISTADR4 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSDR1 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSDR2 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSDR3 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSDR4 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSDR5 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSDR6 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20120926 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20130417 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20140409 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20150108 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20160114 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20160507 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20170630 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20180419 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20201209 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20231101 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VHSv20240731 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIDEODR2 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIDEODR3 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIDEODR4 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIDEODR5 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIDEOv20111208 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGDR2 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGDR3 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGDR4 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGv20110714 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGv20111019 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGv20130417 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGv20140402 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGv20150421 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGv20151230 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGv20160406 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGv20161202 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VIKINGv20170715 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCDEEPv20230713 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCDEEPv20240506 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCDR1 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCDR2 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCDR3 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCDR4 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCDR5 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20110816 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20110909 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20120126 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20121128 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20130304 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20130805 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20140428 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20140903 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20150309 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20151218 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20160311 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20160822 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20170109 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20170411 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20171101 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20180702 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20181120 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20191212 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20210708 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20230816 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VMCv20240226 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VSAQC |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VVVDR1 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VVVDR2 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VVVDR5 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VVVXDR1 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
sadtTileRa |
MultiframeEsoKeys |
VVVv20110718 |
SADT tile RA {image primary HDU keyword: HIERARCH ESO OCS SADT TILE RA} |
real |
4 |
HHMMSS.TTT |
-0.9999995e9 |
|
satnum |
allwise_sc |
WISE |
Minimum sample at which saturation occurs in each band. Four character string, one character per band, that indicates the minimum SUTR sample in which any pixel in the profile-fitting area in all of the single-exposure images used to characterize this source was flagged as having reached the saturation level in the on-board WISE payload processing. If no pixels in a given band are flagged as saturated, the value for that band is "0". |
varchar |
4 |
|
|
|
satnum |
wise_allskysc |
WISE |
Minimum sample at which saturation occurs in each band. Four character string, one character per band, that indicates the minimum SUTR sample in which any pixel in the profile-fitting area in all of the single-exposure images used to characterize this source was flagged as having reached the saturation level in the on-board WISE payload processing. If no pixels in a given band are flagged as saturated, the value for that band is "0". |
char |
4 |
|
|
|
satnum |
wise_prelimsc |
WISE |
Minimum sample at which saturation occurs in each band Four character string, one character per band, that indicates the minimum SUTR sample in which any pixel in the profile-fitting area in all of the single-exposure images used to characterize this source was flagged as having reached the saturation level in the on-board WISE payload processing. If no pixels in a given band are flagged as saturated, the value for that band is "0". |
char |
4 |
|
|
|
saturatCorr |
sharksDetection |
SHARKSv20210222 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
sharksDetection |
SHARKSv20210421 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSDR1 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
vhsDetection |
VHSDR2 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
vhsDetection |
VHSDR3 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSDR4 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSDR5 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSDR6 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20120926 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20130417 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20140409 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20150108 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20160114 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20160507 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20170630 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20180419 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20201209 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20231101 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vhsDetection |
VHSv20240731 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
videoDetection |
VIDEODR2 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
videoDetection |
VIDEODR3 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
videoDetection |
VIDEODR4 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
videoDetection |
VIDEODR5 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
videoDetection |
VIDEOv20111208 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
vikingDetection |
VIKINGDR2 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
vikingDetection |
VIKINGDR3 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vikingDetection |
VIKINGDR4 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vikingDetection |
VIKINGv20110714 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
vikingDetection |
VIKINGv20111019 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
vikingDetection |
VIKINGv20130417 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vikingDetection |
VIKINGv20140402 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vikingDetection |
VIKINGv20150421 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vikingDetection |
VIKINGv20151230 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vikingDetection |
VIKINGv20160406 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vikingDetection |
VIKINGv20161202 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vikingDetection |
VIKINGv20170715 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCDR1 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
vmcDetection |
VMCDR2 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCDR3 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCDR4 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCDR5 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20110816 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
vmcDetection |
VMCv20110909 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
vmcDetection |
VMCv20120126 |
saturation correction |
real |
4 |
|
0.0 |
|
saturatCorr |
vmcDetection |
VMCv20121128 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20130304 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20130805 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20140428 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20140903 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20150309 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20151218 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20160311 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20160822 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20170109 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20170411 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20171101 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20180702 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20181120 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20191212 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20210708 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20230816 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcDetection |
VMCv20240226 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcdeepDetection |
VMCDEEPv20230713 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vmcdeepDetection |
VMCDEEPv20240506 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vvvDetection |
VVVDR1 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vvvDetection |
VVVDR2 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
saturatCorr |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
saturation correction |
real |
4 |
|
0.0 |
stat.param |
SC_CHI2PROB |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
XMM |
The Chi² probability (based on the null hypothesis) that the unique source SRCID as detected by any of the observations is constant, that is, the minimum value of the EPIC probabilities in each detection, EP_CHI2PROB, is given. |
real |
4 |
|
|
|
SC_CHI2PROB |
xmm3dr4 |
XMM |
The Chi² probability (based on the null hypothesis) that the unique source SRCID as detected by any of the observations is constant, that is, the minimum value of the EPIC probabilities in each detection, EP_CHI2PROB, is given. |
float |
8 |
|
|
|
SC_DEC |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean Declination in degrees (J2000) of all the detections of the source SRCID (see DEC) weighted by the positional errors POSERR. |
float |
8 |
degrees |
|
|
SC_DET_ML |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The total band detection likelihood of the source SRCID is the maximum of the likelihoods of all detections of this source (EP_8_DET_ML). |
real |
4 |
|
|
|
SC_DR_FIRST |
twoxmmi_dr3_v1_0 |
XMM |
This flag indicates in which catalogue in the 2XMM catalogue series (starting from 2XMM) this unique source first appeared. The flag is DR1 for 2XMM, DR2 for 2XMMi and DR3 for the present 2XMMi-DR3 catalogue. |
int |
4 |
|
|
|
SC_DR_LAST |
twoxmmi_dr3_v1_0 |
XMM |
This flag indicates in which catalogue in the 2XMM catalogue series (starting from 2XMM) the parameters of this unique source were last updated (e.g. due to the inclusion of one or more new detections which can add to, or even split, the source). The flag is DR1 for 2XMM, DR2 for 2XMMi and DR3 for the present 2XMMi-DR3 catalogue. |
int |
4 |
|
|
|
SC_EP_1_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean band 1 flux (0.2 - 0.5 keV) of all the detections of the source SRCID (see EP_1_FLUX) weighted by the errors (EP_1_FLUX_ERR), in erg/cm2/s. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_1_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean band 1 flux in SC_EP_1_FLUX. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_2_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean band 2 flux (0.5 - 1.0 keV) of all the detections of the source SRCID (see EP_2_FLUX) weighted by the errors (EP_2_FLUX_ERR), in erg/cm2/s. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_2_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean band 2 flux in SC_EP_2_FLUX. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_3_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean band 3 flux (1.0 - 2.0 keV) of all the detections of the source SRCID (see EP_3_FLUX) weighted by the errors (EP_3_FLUX_ERR), in erg/cm2/s. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_3_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean band 3 flux in SC_EP_3_FLUX. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_4_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean band 4 flux (2.0 - 4.5 keV) of all the detections of the source SRCID (see EP_4_FLUX) weighted by the errors (EP_4_FLUX_ERR), in erg/cm2/s. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_4_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean band 4 flux in SC_EP_4_FLUX. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_5_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean band 5 flux (4.5 - 12 keV) of all the detections of the source SRCID (see EP_5_FLUX) weighted by the errors (EP_5_FLUX_ERR), in erg/cm2/s. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_5_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean band 5 flux in SC_EP_5_FLUX. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_8_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean total band flux (0.2 - 12 keV) of all the detections of the source SRCID (see EP_8_FLUX) weighted by the errors (EP_8_FLUX_ERR), in erg/cm2/s. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_8_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean total band flux in SC_EP_8_FLUX. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_8_FMAX |
xmm3dr4 |
XMM |
The maximum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_8_FMAX_ERR |
xmm3dr4 |
XMM |
The error on the maximum EPIC band 8 flux (EP_8_FLUX_ERR) amongst any of the constituent detections of the unique source. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_8_FMIN |
xmm3dr4 |
XMM |
The minimum EPIC band 8 flux (EP_8_FLUX) amongst any of the constituent detections of the unique source. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_8_FMIN_ERR |
xmm3dr4 |
XMM |
The error on the minimum EPIC band 8 flux (EP_8_FLUX_ERR) amongst any of the constituent detections of the unique source. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_9_FLUX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean band 9 flux (0.5 - 4.5 keV) of all the detections of the source SRCID (see EP_9_FLUX) weighted by the errors (EP_9_FLUX_ERR), in erg/cm2/s. |
real |
4 |
erg/cm**2/s |
|
|
SC_EP_9_FLUX_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean band 9 flux in SC_EP_9_FLUX. |
real |
4 |
erg/cm**2/s |
|
|
SC_EXT_ML |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The total band detection likelihood of the extended source SRCID is the average of the extent likelihoods of all detections of this source (EP_EXTENT_ML). |
real |
4 |
|
|
|
SC_EXTENT |
twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The total band extent of the source SRCID is the weighted average of the EPIC extents of all detections of this source (EP_EXTENT). |
real |
4 |
arcsec |
|
|
SC_FVAR |
xmm3dr4 |
XMM |
The fractional excess variance of the unique source. It is the value corresponding to the exposure and instrument that shows the lowest probability of being constant (i.e. it is the PN_FVAR, M1_FVAR or M2_FVAR value corresponding to EP_CHI2PROB, SC_CHI2PROB). |
float |
8 |
|
|
|
SC_FVARERR |
xmm3dr4 |
XMM |
The error on the fractional excess variance of the unique source. |
float |
8 |
|
|
|
SC_HR1 |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean hardness ratio of the bands 1 and 2 of all the detections of the source SRCID (EP_HR1) weighted by the errors(EP_HR1_ERR). |
real |
4 |
|
|
|
SC_HR1_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean hardness ratio in SC_HR1. |
real |
4 |
|
|
|
SC_HR2 |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean hardness ratio of the bands 2 and 3 of all the detections of the source SRCID (EP_HR2) weighted by the errors(EP_HR2_ERR). |
real |
4 |
|
|
|
SC_HR2_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean hardness ratio in SC_HR2. |
real |
4 |
|
|
|
SC_HR3 |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean hardness ratio of the bands 3 and 4 of all the detections of the source SRCID (EP_HR3) weighted by the errors(EP_HR3_ERR). |
real |
4 |
|
|
|
SC_HR3_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean hardness ratio in SC_HR3. |
real |
4 |
|
|
|
SC_HR4 |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean hardness ratio of the bands 4 and 5 of all the detections of the source SRCID (EP_HR4) weighted by the errors(EP_HR4_ERR). |
real |
4 |
|
|
|
SC_HR4_ERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
Error on the weighted mean hardness ratio in SC_HR4. |
real |
4 |
|
|
|
SC_POSERR |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The error of the weighted mean position given in SC_RA and SC_DEC in arcseconds. |
real |
4 |
arcsec |
|
|
SC_RA |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
The mean Right Ascension in degrees (J2000) of all the detections of the source SRCID (see RA) weighted by the positional errors POSERR. |
float |
8 |
degrees |
|
|
SC_SUM_FLAG |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
XMM |
The summary flag for the unique source SRCID is taken to be the worst flag of all detections of this source (SUM_FLAG). |
int |
4 |
|
|
|
SC_SUM_FLAG |
xmm3dr4 |
XMM |
The summary flag for the unique source SRCID is taken to be the worst flag of all detections of this source (SUM_FLAG). |
smallint |
2 |
|
|
|
SC_VAR_FLAG |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
XMM |
The variability flag for the unique source SRCID is set to VAR_FLAG of the most variable detection of this source. |
varchar |
5 |
|
|
|
SC_VAR_FLAG |
xmm3dr4 |
XMM |
The variability flag for the unique source SRCID is set to VAR_FLAG of the most variable detection of this source (0=False, 1=True). |
bit |
1 |
|
|
|
scan |
twomass_psc |
TWOMASS |
The nightly scan number in which the source was detected. |
smallint |
2 |
|
|
meta.number |
scan |
twomass_scn |
TWOMASS |
Scan number (unique within date). |
smallint |
2 |
|
|
meta.number |
scan |
twomass_sixx2_scn |
TWOMASS |
scan number (unique within date) |
smallint |
2 |
|
|
|
scan |
twomass_xsc |
TWOMASS |
scan number (unique within date). |
smallint |
2 |
|
|
meta.number |
scan_direction_mean_k1 |
gaia_source |
GAIAEDR3 |
Mean position angle of scan directions across the source |
real |
4 |
degrees |
|
pos.posAng;stat.mean |
scan_direction_mean_k1 |
gaia_source, tgas_source |
GAIADR1 |
Mean position angle of scan directions across the source |
real |
4 |
degrees |
|
|
scan_direction_mean_k2 |
gaia_source |
GAIAEDR3 |
Mean position angle of scan directions across the source |
real |
4 |
degrees |
|
pos.posAng;stat.mean |
scan_direction_mean_k2 |
gaia_source, tgas_source |
GAIADR1 |
Mean position angle of scan directions across the source |
real |
4 |
degrees |
|
|
scan_direction_mean_k3 |
gaia_source |
GAIAEDR3 |
Mean position angle of scan directions across the source |
real |
4 |
degrees |
|
pos.posAng;stat.mean |
scan_direction_mean_k3 |
gaia_source, tgas_source |
GAIADR1 |
Mean position angle of scan directions across the source |
real |
4 |
degrees |
|
|
scan_direction_mean_k4 |
gaia_source |
GAIAEDR3 |
Mean position angle of scan directions across the source |
real |
4 |
degrees |
|
pos.posAng;stat.mean |
scan_direction_mean_k4 |
gaia_source, tgas_source |
GAIADR1 |
Mean position angle of scan directions across the source |
real |
4 |
degrees |
|
|
scan_direction_strength_k1 |
gaia_source |
GAIAEDR3 |
Degree of concentration of scan directions across the source |
real |
4 |
|
|
stat.value |
scan_direction_strength_k1 |
gaia_source, tgas_source |
GAIADR1 |
Degree of concentration of scan directions across the source |
real |
4 |
|
|
|
scan_direction_strength_k2 |
gaia_source |
GAIAEDR3 |
Degree of concentration of scan directions across the source |
real |
4 |
|
|
stat.value |
scan_direction_strength_k2 |
gaia_source, tgas_source |
GAIADR1 |
Degree of concentration of scan directions across the source |
real |
4 |
|
|
|
scan_direction_strength_k3 |
gaia_source |
GAIAEDR3 |
Degree of concentration of scan directions across the source |
real |
4 |
|
|
stat.value |
scan_direction_strength_k3 |
gaia_source, tgas_source |
GAIADR1 |
Degree of concentration of scan directions across the source |
real |
4 |
|
|
|
scan_direction_strength_k4 |
gaia_source |
GAIAEDR3 |
Degree of concentration of scan directions across the source |
real |
4 |
|
|
stat.value |
scan_direction_strength_k4 |
gaia_source, tgas_source |
GAIADR1 |
Degree of concentration of scan directions across the source |
real |
4 |
|
|
|
scan_key |
twomass_psc |
TWOMASS |
Unique identification number of the record in the Scan Information Table that corresponds to the survey scan in which this source was detected. |
int |
4 |
|
|
meta.id |
scan_key |
twomass_scn |
TWOMASS |
the unique identification number for this scan. |
int |
4 |
|
|
meta.id |
scan_key |
twomass_sixx2_xsc |
TWOMASS |
key to scan data record in "scan DB" |
int |
4 |
|
|
|
scan_key |
twomass_xsc |
TWOMASS |
key to scan data record in "scan DB". |
int |
4 |
|
|
meta.id |
scosID |
twompzPhotoz |
TWOMPZ |
SuperCOSMOS Source table (objID) {image primary HDU keyword: SCOS_objID} |
bigint |
8 |
|
-99999999 |
meta.id |
scosID |
wiseScosPhotoz, wiseScosPhotozRejects |
WISExSCOSPZ |
SuperCOSMOS Source table (objID) {image primary HDU keyword: objID} |
bigint |
8 |
|
-99999999 |
meta.id |
scosID |
wiseScosSvm |
WISExSCOSPZ |
SuperCOSMOS Source table (objID) {image primary HDU keyword: scos_objID} |
bigint |
8 |
|
-99999999 |
meta.id |
sd |
twomass_scn |
TWOMASS |
Scanning direction: "n" = north-going, "s" = south-going. |
varchar |
1 |
|
|
pos.posAng |
sd |
twomass_sixx2_scn |
TWOMASS |
direction of scan -- north/south-bound (n/s) |
varchar |
1 |
|
|
|
sdet |
twomass_sixx2_psc, twomass_sixx2_xsc |
TWOMASS |
# of scans in which src was detected in >=1 band |
smallint |
2 |
|
|
|
SDSS_CAMCOL |
mgcBrightSpec |
MGC |
SDSS camera column |
int |
4 |
|
|
|
SDSS_CLASS |
mgcBrightSpec |
MGC |
MGC translation of SDSS_TYPE |
smallint |
2 |
|
|
|
SDSS_DEC |
mgcBrightSpec |
MGC |
SDSS object declination in deg (J2000) |
float |
8 |
|
|
|
SDSS_EXTINC_G |
mgcBrightSpec |
MGC |
SDSS Galactic extinction correction in mag |
real |
4 |
|
|
|
SDSS_EXTINC_I |
mgcBrightSpec |
MGC |
SDSS Galactic extinction correction in mag |
real |
4 |
|
|
|
SDSS_EXTINC_R |
mgcBrightSpec |
MGC |
SDSS Galactic extinction correction in mag |
real |
4 |
|
|
|
SDSS_EXTINC_U |
mgcBrightSpec |
MGC |
SDSS Galactic extinction correction in mag |
real |
4 |
|
|
|
SDSS_EXTINC_Z |
mgcBrightSpec |
MGC |
SDSS Galactic extinction correction in mag |
real |
4 |
|
|
|
SDSS_FIELD |
mgcBrightSpec |
MGC |
SDSS field number |
int |
4 |
|
|
|
SDSS_MODMAG_G |
mgcBrightSpec |
MGC |
SDSS extinction corrected model magnitude |
real |
4 |
|
|
|
SDSS_MODMAG_I |
mgcBrightSpec |
MGC |
SDSS extinction corrected model magnitude |
real |
4 |
|
|
|
SDSS_MODMAG_R |
mgcBrightSpec |
MGC |
SDSS extinction corrected model magnitude |
real |
4 |
|
|
|
SDSS_MODMAG_U |
mgcBrightSpec |
MGC |
SDSS extinction corrected model magnitude |
real |
4 |
|
|
|
SDSS_MODMAG_Z |
mgcBrightSpec |
MGC |
SDSS extinction corrected model magnitude |
real |
4 |
|
|
|
SDSS_N |
mgcBrightSpec |
MGC |
Number of SDSS objects matched to MGC object |
int |
4 |
|
|
|
SDSS_OBJID |
mgcBrightSpec |
MGC |
SDSS PhotoObject ID |
bigint |
8 |
|
|
|
SDSS_PETMAG_G |
mgcBrightSpec |
MGC |
SDSS extinction corrected Petrosian magnitude |
real |
4 |
|
|
|
SDSS_PETMAG_I |
mgcBrightSpec |
MGC |
SDSS extinction corrected Petrosian magnitude |
real |
4 |
|
|
|
SDSS_PETMAG_R |
mgcBrightSpec |
MGC |
SDSS extinction corrected Petrosian magnitude |
real |
4 |
|
|
|
SDSS_PETMAG_U |
mgcBrightSpec |
MGC |
SDSS extinction corrected Petrosian magnitude |
real |
4 |
|
|
|
SDSS_PETMAG_Z |
mgcBrightSpec |
MGC |
SDSS extinction corrected Petrosian magnitude |
real |
4 |
|
|
|
SDSS_PETR50_G |
mgcBrightSpec |
MGC |
SDSS radius containing 50% Petrosian flux in arcsec |
real |
4 |
|
|
|
SDSS_PETR50_I |
mgcBrightSpec |
MGC |
SDSS radius containing 50% Petrosian flux in arcsec |
real |
4 |
|
|
|
SDSS_PETR50_R |
mgcBrightSpec |
MGC |
SDSS radius containing 50% Petrosian flux in arcsec |
real |
4 |
|
|
|
SDSS_PETR50_U |
mgcBrightSpec |
MGC |
SDSS radius containing 50% Petrosian flux in arcsec |
real |
4 |
|
|
|
SDSS_PETR50_Z |
mgcBrightSpec |
MGC |
SDSS radius containing 50% Petrosian flux in arcsec |
real |
4 |
|
|
|
SDSS_PSFMAG_G |
mgcBrightSpec |
MGC |
SDSS extinction corrected PSF magnitude |
real |
4 |
|
|
|
SDSS_PSFMAG_I |
mgcBrightSpec |
MGC |
SDSS extinction corrected PSF magnitude |
real |
4 |
|
|
|
SDSS_PSFMAG_R |
mgcBrightSpec |
MGC |
SDSS extinction corrected PSF magnitude |
real |
4 |
|
|
|
SDSS_PSFMAG_U |
mgcBrightSpec |
MGC |
SDSS extinction corrected PSF magnitude |
real |
4 |
|
|
|
SDSS_PSFMAG_Z |
mgcBrightSpec |
MGC |
SDSS extinction corrected PSF magnitude |
real |
4 |
|
|
|
SDSS_RA |
mgcBrightSpec |
MGC |
SDSS object right ascension in deg (J2000) |
float |
8 |
|
|
|
SDSS_RERUN |
mgcBrightSpec |
MGC |
SDSS rerun number |
int |
4 |
|
|
|
SDSS_RUN |
mgcBrightSpec |
MGC |
SDSS run number |
int |
4 |
|
|
|
SDSS_SPCLASS |
mgcBrightSpec |
MGC |
MGC translation of SDSS_SPECCLASS |
smallint |
2 |
|
|
|
SDSS_SPECCLASS |
mgcBrightSpec |
MGC |
SDSS spectroscopic classification |
smallint |
2 |
|
|
|
SDSS_TYPE |
mgcBrightSpec |
MGC |
SDSS morphological classification |
smallint |
2 |
|
|
|
SDSS_Z |
mgcBrightSpec |
MGC |
SDSS redshift |
real |
4 |
|
|
|
SDSS_ZQUAL |
mgcBrightSpec |
MGC |
SDSS redshift quality |
tinyint |
1 |
|
|
|
sdssClass |
first08Jul16Source, firstSource12Feb16 |
FIRST |
morphological classification in SDSS DR6 (s=stellar, g=nonstellar/galaxy) |
varchar |
1 |
|
|
|
sdssMag |
first08Jul16Source, firstSource12Feb16 |
FIRST |
SDSS i magnitude |
real |
4 |
mag |
|
|
sdssMatches |
first08Jul16Source |
FIRST |
number of matches within a fiducial radius (8 arcsec) with SDSS DR6 |
int |
4 |
|
|
|
sdssMatches |
firstSource12Feb16 |
FIRST |
number of matches within a fiducial radius (8 arcsec) with SDSS DR6 |
smallint |
2 |
|
|
|
sdssPrimary |
ultravistaSourceXDR13PhotoObj, ultravistaSourceXDR13PhotoObjAll |
ULTRAVISTADR4 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vhsSourceXDR13PhotoObj |
VHSv20201209 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vhsSourceXDR13PhotoObj |
VHSv20231101 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vhsSourceXDR13PhotoObj |
VHSv20240731 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vhsSourceXDR13PhotoObj, vhsSourceXDR13PhotoObjAll, vhsSourceXDR7PhotoObj, vhsSourceXDR7PhotoObjAll, vhsSourceXStripe82PhotoObjAll |
VHSv20180419 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
videoSourceXStripe82PhotoObjAll |
VIDEODR2 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
videoSourceXStripe82PhotoObjAll |
VIDEODR3 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
videoSourceXStripe82PhotoObjAll |
VIDEODR4 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
videoSourceXStripe82PhotoObjAll |
VIDEODR5 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
videoSourceXStripe82PhotoObjAll |
VIDEOv20100513 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
videoSourceXStripe82PhotoObjAll |
VIDEOv20111208 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vikingSourceXDR7PhotoObj |
VIKINGDR3 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vikingSourceXDR7PhotoObj |
VIKINGDR4 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vikingSourceXDR7PhotoObj |
VIKINGv20110714 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vikingSourceXDR7PhotoObj |
VIKINGv20111019 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vikingSourceXDR7PhotoObj |
VIKINGv20130417 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vikingSourceXDR7PhotoObj |
VIKINGv20140402 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vikingSourceXDR7PhotoObj |
VIKINGv20150421 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vikingSourceXDR7PhotoObj |
VIKINGv20151230 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vikingSourceXDR7PhotoObj |
VIKINGv20160406 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssPrimary |
vikingSourceXDR7PhotoObj, vikingSourceXDR7PhotoObjAll, vikingSourceXStripe82PhotoObjAll |
VIKINGDR2 |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
255 |
meta.code |
sdssSep |
first08Jul16Source, firstSource12Feb16 |
FIRST |
separation of the nearest match in SDSS DR6 from the FIRST position |
real |
4 |
arcsec |
|
|
sdssType |
ultravistaSourceXDR13PhotoObj, ultravistaSourceXDR13PhotoObjAll |
ULTRAVISTADR4 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vhsSourceXDR13PhotoObj |
VHSv20201209 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vhsSourceXDR13PhotoObj |
VHSv20231101 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vhsSourceXDR13PhotoObj |
VHSv20240731 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vhsSourceXDR13PhotoObj, vhsSourceXDR13PhotoObjAll, vhsSourceXDR7PhotoObj, vhsSourceXDR7PhotoObjAll, vhsSourceXStripe82PhotoObjAll |
VHSv20180419 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
videoSourceXStripe82PhotoObjAll |
VIDEODR2 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
videoSourceXStripe82PhotoObjAll |
VIDEODR3 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
videoSourceXStripe82PhotoObjAll |
VIDEODR4 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
videoSourceXStripe82PhotoObjAll |
VIDEODR5 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
videoSourceXStripe82PhotoObjAll |
VIDEOv20100513 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
videoSourceXStripe82PhotoObjAll |
VIDEOv20111208 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vikingSourceXDR7PhotoObj |
VIKINGDR3 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vikingSourceXDR7PhotoObj |
VIKINGDR4 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vikingSourceXDR7PhotoObj |
VIKINGv20110714 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vikingSourceXDR7PhotoObj |
VIKINGv20111019 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vikingSourceXDR7PhotoObj |
VIKINGv20130417 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vikingSourceXDR7PhotoObj |
VIKINGv20140402 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vikingSourceXDR7PhotoObj |
VIKINGv20150421 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vikingSourceXDR7PhotoObj |
VIKINGv20151230 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vikingSourceXDR7PhotoObj |
VIKINGv20160406 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sdssType |
vikingSourceXDR7PhotoObj, vikingSourceXDR7PhotoObjAll, vikingSourceXStripe82PhotoObjAll |
VIKINGDR2 |
SDSS type of neighbour: 3=galaxy; 6=star |
tinyint |
1 |
|
255 |
src.class |
sectionID |
FilterSections |
SHARKSv20210421 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
ULTRAVISTADR4 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSDR3 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSDR4 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSDR5 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSDR6 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSv20150108 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSv20160114 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSv20160507 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSv20170630 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSv20180419 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSv20201209 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSv20231101 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VHSv20240731 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VIDEODR4 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VIDEODR5 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VIKINGDR4 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VIKINGv20150421 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VIKINGv20151230 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VIKINGv20160406 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VIKINGv20161202 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VIKINGv20170715 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCDEEPv20230713 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCDEEPv20240506 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCDR3 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCDR4 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCDR5 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20140428 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20140903 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20150309 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20151218 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20160311 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20160822 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20170109 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20170411 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20171101 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20180702 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20181120 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20191212 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20210708 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20230816 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VMCv20240226 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VSAQC |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VVVDR5 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections |
VVVXDR1 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
sectionID |
FilterSections, SectionDetectors |
SHARKSv20210222 |
UID of section of focal plane with different filter |
tinyint |
1 |
|
|
|
seeing |
MultiframeDetector |
SHARKSv20210222 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
SHARKSv20210421 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
ULTRAVISTADR4 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSDR1 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSDR2 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSDR3 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSDR4 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSDR5 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSDR6 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20120926 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20130417 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20140409 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20150108 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20160114 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20160507 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20170630 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20180419 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20201209 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20231101 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VHSv20240731 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIDEODR2 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIDEODR3 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIDEODR4 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIDEODR5 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIDEOv20100513 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIDEOv20111208 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGDR2 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGDR3 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGDR4 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGv20110714 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGv20111019 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGv20130417 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGv20140402 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGv20150421 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGv20151230 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGv20160406 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGv20161202 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VIKINGv20170715 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCDEEPv20230713 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCDEEPv20240506 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCDR1 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCDR2 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCDR3 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCDR4 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCDR5 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20110816 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20110909 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20120126 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20121128 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20130304 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20130805 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20140428 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20140903 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20150309 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20151218 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20160311 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20160822 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20170109 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20170411 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20171101 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20180702 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20181120 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20191212 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20210708 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20230816 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VMCv20240226 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VVVDR1 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VVVDR2 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VVVDR5 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VVVXDR1 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VVVv20100531 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
MultiframeDetector |
VVVv20110718 |
Average FWHM {catalogue extension keyword: SEEING} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC). |
seeing |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Average FWHM |
real |
4 |
pixels |
-0.9999995e9 |
?? |
selection |
RequiredListDrivenProduct |
VHSv20130417 |
Selection SQL or filename containing list |
varchar |
1024 |
|
NONE |
|
selection |
RequiredListDrivenProduct |
VIKINGv20130417 |
Selection SQL or filename containing list |
varchar |
1024 |
|
NONE |
|
selection |
RequiredListDrivenProduct |
VMCv20130805 |
Selection SQL or filename containing list |
varchar |
1024 |
|
NONE |
|
selection |
RequiredMatchedApertureProduct |
SHARKSv20210222 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
SHARKSv20210421 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
ULTRAVISTADR4 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VHSv20201209 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VHSv20231101 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VHSv20240731 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VMCDEEPv20230713 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VMCDEEPv20240506 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VMCDR5 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VMCv20191212 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VMCv20210708 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VMCv20230816 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VMCv20240226 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VVVDR5 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
selection |
RequiredMatchedApertureProduct |
VVVXDR1 |
Selection SQL or filename containing list |
varchar |
1024 |
|
|
|
sep |
gaiaxwise_matches |
GAIAXWISE |
Angular separation between sources |
float |
8 |
arcsec |
|
|
SEP_1XMM |
twoxmm, twoxmm_v1_2 |
XMM |
The distance between this source and the matched 1XMM source (MATCH_1XMM) in arcseconds. |
real |
4 |
arcsec |
|
|
SEP_2XMMP |
twoxmm, twoxmm_v1_2 |
XMM |
The distance between this source and the matched 2XMMp source (MATCH_2XMMp) in arcseconds. |
real |
4 |
arcsec |
|
|
seqNo |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
sequential object number |
int |
4 |
|
|
meta.id |
seqNo |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca, glimpse_hrc_inter |
GLIMPSE |
sequential object number in the HRC |
int |
4 |
|
|
meta.id |
seqNo |
glimpse_mca_inter |
GLIMPSE |
sequential object number in the MCA |
int |
4 |
|
|
meta.id |
seqNo |
iras_psc |
IRAS |
sequential object number |
int |
4 |
|
|
meta.id |
seqNo |
nvssSource |
NVSS |
sequential object number |
int |
4 |
|
|
meta.id |
seqNo |
ogle3LpvLmcSource, ogle3LpvSmcSource, ogle4CepLmcSource, ogle4CepSmcSource, ogle4RRLyrLmcSource, ogle4RRLyrSmcSource |
OGLE |
sequential object number |
int |
4 |
|
|
meta.number |
seqNo |
rosat_bsc |
ROSAT |
sequential object number in the BSC |
int |
4 |
|
|
meta.id |
seqNo |
rosat_fsc |
ROSAT |
sequential object number in the FSC |
int |
4 |
|
|
meta.id |
SEQNUM |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Sequential number (unique object ID) |
int |
4 |
|
|
|
SEQNUM |
grs_ngpSource, grs_ranSource, grs_sgpSource |
TWODFGRS |
Assigned sequence number to this object; determines the FITS filename (SEQNUM.fits) |
int |
4 |
|
|
meta.id |
seqNum |
combo17CDFSSource |
COMBO17 |
Sequential number (unique object ID) |
int |
4 |
|
|
|
seqNum |
denisDR3Source |
DENIS |
Sequential number (unique object ID) |
int |
4 |
|
|
|
seqNum |
eros2LMCSource, eros2SMCSource, erosLMCSource, erosSMCSource |
EROS |
Sequential number (unique object ID) |
int |
4 |
|
|
|
seqNum |
machoLMCSource, machoSMCSource |
MACHO |
Sequential number (unique object ID) |
int |
4 |
|
|
|
seqNum |
mcps_lmcSource, mcps_smcSource |
MCPS |
Sequential number (unique object ID) |
int |
4 |
|
|
|
seqNum |
sharksDetection |
SHARKSv20210222 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
sharksDetection |
SHARKSv20210421 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
sharksSourceXDetectionBestMatch |
SHARKSv20210222 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
sharksSourceXDetectionBestMatch |
SHARKSv20210421 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
spitzer_smcSource |
SPITZER |
Sequential number (unique object ID) |
int |
4 |
|
|
|
seqNum |
twomass_sixx2_psc |
TWOMASS |
Sequential number (unique object ID) |
int |
4 |
|
|
|
seqNum |
ultravistaDetection |
ULTRAVISTADR4 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
ultravistaSourceXDetectionBestMatch |
ULTRAVISTADR4 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vhsDetection |
VHSDR2 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vhsDetection |
VHSDR3 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSDR4 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSDR5 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSDR6 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSv20120926 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSv20130417 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSv20140409 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSv20150108 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSv20160114 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSv20160507 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSv20170630 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSv20180419 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vhsDetection |
VHSv20201209 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vhsDetection |
VHSv20231101 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vhsDetection |
VHSv20240731 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
videoDetection |
VIDEODR2 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
videoDetection |
VIDEODR3 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
videoDetection |
VIDEODR4 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
videoDetection |
VIDEODR5 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
videoDetection |
VIDEOv20111208 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
videoDetection, videoListRemeasurement |
VIDEOv20100513 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
videoSourceXDetectionBestMatch |
VIDEODR2 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.id |
seqNum |
videoSourceXDetectionBestMatch |
VIDEODR3 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
videoSourceXDetectionBestMatch |
VIDEODR4 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
videoSourceXDetectionBestMatch |
VIDEODR5 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
videoSourceXDetectionBestMatch |
VIDEOv20100513 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.id |
seqNum |
videoSourceXDetectionBestMatch |
VIDEOv20111208 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.id |
seqNum |
vikingDetection |
VIKINGDR2 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vikingDetection |
VIKINGDR3 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vikingDetection |
VIKINGDR4 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vikingDetection |
VIKINGv20111019 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vikingDetection |
VIKINGv20130417 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vikingDetection |
VIKINGv20140402 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vikingDetection |
VIKINGv20150421 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vikingDetection |
VIKINGv20151230 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vikingDetection |
VIKINGv20160406 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vikingDetection |
VIKINGv20161202 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vikingDetection |
VIKINGv20170715 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGDR2 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.id |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGDR3 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGDR4 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGv20110714 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.id |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGv20111019 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.id |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGv20130417 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGv20140402 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGv20150421 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGv20151230 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGv20160406 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGv20161202 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vikingSourceXDetectionBestMatch |
VIKINGv20170715 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vmcDetection |
VMCDR1 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vmcDetection |
VMCDR2 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCDR3 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCDR4 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCDR5 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vmcDetection |
VMCv20110909 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vmcDetection |
VMCv20120126 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vmcDetection |
VMCv20121128 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20130304 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20130805 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20140428 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20140903 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20150309 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20151218 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20160311 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20160822 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20170109 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20170411 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20171101 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20180702 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20181120 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vmcDetection |
VMCv20191212 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vmcDetection |
VMCv20210708 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vmcDetection |
VMCv20230816 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vmcDetection |
VMCv20240226 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vmcdeepDetection |
VMCDEEPv20230713 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vmcdeepDetection |
VMCDEEPv20240506 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vvvDetection |
VVVDR1 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vvvDetection |
VVVDR2 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.number |
seqNum |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
|
meta.id |
seqNum |
vvvSourceXDetectionBestMatch |
VVVDR1 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vvvSourceXDetectionBestMatch |
VVVDR2 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vvvSourceXDetectionBestMatch |
VVVDR5 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.number |
seqNum |
vvvSourceXDetectionBestMatch |
VVVv20100531 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.id |
seqNum |
vvvSourceXDetectionBestMatch |
VVVv20110718 |
the running number of this detection {catalogue TType keyword: Sequence_number} The running number for ease of reference, in strict order of image detections. |
int |
4 |
|
-99999999 |
meta.id |
SerFit1DChi2 |
sharksDetection |
SHARKSv20210222 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
sharksDetection |
SHARKSv20210421 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSDR2 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSDR3 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSDR4 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSDR5 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSDR6 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20120926 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20130417 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20140409 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20150108 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20160114 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20160507 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20170630 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20180419 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20201209 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20231101 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection |
VHSv20240731 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
videoDetection |
VIDEODR2 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
|
SerFit1DChi2 |
videoDetection |
VIDEODR3 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
videoDetection |
VIDEODR4 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
videoDetection |
VIDEODR5 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
videoDetection |
VIDEOv20100513 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
|
SerFit1DChi2 |
videoDetection |
VIDEOv20111208 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
|
SerFit1DChi2 |
videoListRemeasurement |
VIDEOv20100513 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGDR2 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGDR3 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGDR4 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGv20111019 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGv20130417 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGv20140402 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGv20150421 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGv20151230 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGv20160406 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGv20161202 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection |
VIKINGv20170715 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit1DChi2 |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
sharksDetection |
SHARKSv20210222 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
sharksDetection |
SHARKSv20210421 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSDR2 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSDR3 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSDR4 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSDR5 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSDR6 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20120926 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20130417 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20140409 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20150108 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20160114 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20160507 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20170630 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20180419 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20201209 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20231101 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection |
VHSv20240731 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
videoDetection |
VIDEODR2 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
|
SerFit2DChi2 |
videoDetection |
VIDEODR3 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
videoDetection |
VIDEODR4 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
videoDetection |
VIDEODR5 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
videoDetection |
VIDEOv20100513 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
|
SerFit2DChi2 |
videoDetection |
VIDEOv20111208 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_chi2} |
real |
4 |
|
-0.9999995e9 |
|
SerFit2DChi2 |
videoListRemeasurement |
VIDEOv20100513 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGDR2 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGDR3 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGDR4 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGv20111019 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGv20130417 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGv20140402 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGv20150421 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGv20151230 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGv20160406 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGv20161202 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection |
VIKINGv20170715 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vmcdeepDetection |
VMCDEEPv20230713 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFit2DChi2 |
vmcdeepDetection |
VMCDEEPv20240506 |
Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2} standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerFitNu1D |
sharksDetection |
SHARKSv20210222 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
sharksDetection |
SHARKSv20210421 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSDR2 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSDR3 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSDR4 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSDR5 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSDR6 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20120926 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20130417 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20140409 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20150108 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20160114 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20160507 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20170630 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20180419 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20201209 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20231101 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection |
VHSv20240731 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
videoDetection |
VIDEODR2 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
|
SerFitNu1D |
videoDetection |
VIDEODR3 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
videoDetection |
VIDEODR4 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
videoDetection |
VIDEODR5 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
videoDetection |
VIDEOv20100513 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
|
SerFitNu1D |
videoDetection |
VIDEOv20111208 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
|
SerFitNu1D |
videoListRemeasurement |
VIDEOv20100513 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGDR2 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGDR3 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGDR4 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGv20111019 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGv20130417 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGv20140402 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGv20150421 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGv20151230 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGv20160406 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGv20161202 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection |
VIKINGv20170715 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vmcdeepDetection |
VMCDEEPv20230713 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu1D |
vmcdeepDetection |
VMCDEEPv20240506 |
No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
sharksDetection |
SHARKSv20210222 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
sharksDetection |
SHARKSv20210421 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSDR2 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSDR3 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSDR4 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSDR5 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSDR6 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20120926 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20130417 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20140409 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20150108 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20160114 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20160507 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20170630 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20180419 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20201209 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20231101 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection |
VHSv20240731 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
videoDetection |
VIDEODR2 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
|
SerFitNu2D |
videoDetection |
VIDEODR3 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
videoDetection |
VIDEODR4 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
videoDetection |
VIDEODR5 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
videoDetection |
VIDEOv20100513 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
|
SerFitNu2D |
videoDetection |
VIDEOv20111208 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_fit_nu} |
real |
4 |
|
-0.9999995e9 |
|
SerFitNu2D |
videoListRemeasurement |
VIDEOv20100513 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGDR2 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGDR3 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGDR4 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGv20111019 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGv20130417 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGv20140402 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGv20150421 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGv20151230 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGv20160406 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGv20161202 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection |
VIKINGv20170715 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vmcdeepDetection |
VMCDEEPv20230713 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFitNu2D |
vmcdeepDetection |
VMCDEEPv20240506 |
No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.dof |
SerFlux1D |
sharksDetection |
SHARKSv20210222 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
sharksDetection |
SHARKSv20210421 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSDR2 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux1D |
vhsDetection |
VHSDR3 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSDR4 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSDR5 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSDR6 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20120926 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20130417 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20140409 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20150108 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20160114 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20160507 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20170630 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20180419 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20201209 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20231101 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection |
VHSv20240731 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux1D |
videoDetection |
VIDEODR2 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
|
SerFlux1D |
videoDetection |
VIDEODR3 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
phot.count |
SerFlux1D |
videoDetection |
VIDEODR4 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
phot.count |
SerFlux1D |
videoDetection |
VIDEODR5 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
phot.count |
SerFlux1D |
videoDetection |
VIDEOv20100513 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
|
SerFlux1D |
videoDetection |
VIDEOv20111208 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
|
SerFlux1D |
videoListRemeasurement |
VIDEOv20100513 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux1D |
vikingDetection |
VIKINGDR2 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux1D |
vikingDetection |
VIKINGDR3 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vikingDetection |
VIKINGDR4 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vikingDetection |
VIKINGv20111019 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux1D |
vikingDetection |
VIKINGv20130417 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vikingDetection |
VIKINGv20140402 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vikingDetection |
VIKINGv20150421 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vikingDetection |
VIKINGv20151230 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vikingDetection |
VIKINGv20160406 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vikingDetection |
VIKINGv20161202 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vikingDetection |
VIKINGv20170715 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux1D |
vmcdeepDetection |
VMCDEEPv20230713 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux1D |
vmcdeepDetection |
VMCDEEPv20240506 |
1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
sharksDetection |
SHARKSv20210222 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
sharksDetection |
SHARKSv20210421 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSDR2 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux2D |
vhsDetection |
VHSDR3 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSDR4 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSDR5 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSDR6 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20120926 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20130417 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20140409 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20150108 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20160114 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20160507 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20170630 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20180419 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20201209 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20231101 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection |
VHSv20240731 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux2D |
videoDetection |
VIDEODR2 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
|
SerFlux2D |
videoDetection |
VIDEODR3 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
phot.count |
SerFlux2D |
videoDetection |
VIDEODR4 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
phot.count |
SerFlux2D |
videoDetection |
VIDEODR5 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
phot.count |
SerFlux2D |
videoDetection |
VIDEOv20100513 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
|
SerFlux2D |
videoDetection |
VIDEOv20111208 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_flux} |
real |
4 |
|
-0.9999995e9 |
|
SerFlux2D |
videoListRemeasurement |
VIDEOv20100513 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux2D |
vikingDetection |
VIKINGDR2 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux2D |
vikingDetection |
VIKINGDR3 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vikingDetection |
VIKINGDR4 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vikingDetection |
VIKINGv20111019 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux2D |
vikingDetection |
VIKINGv20130417 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vikingDetection |
VIKINGv20140402 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vikingDetection |
VIKINGv20150421 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vikingDetection |
VIKINGv20151230 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vikingDetection |
VIKINGv20160406 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vikingDetection |
VIKINGv20161202 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vikingDetection |
VIKINGv20170715 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count;em.opt |
SerFlux2D |
vmcdeepDetection |
VMCDEEPv20230713 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerFlux2D |
vmcdeepDetection |
VMCDEEPv20240506 |
2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
ADU |
-0.9999995e9 |
phot.count |
SerIdx1D |
sharksDetection |
SHARKSv20210222 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
sharksDetection |
SHARKSv20210421 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSDR2 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSDR3 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSDR4 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSDR5 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSDR6 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20120926 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20130417 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20140409 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20150108 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20160114 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20160507 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20170630 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20180419 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20201209 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20231101 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection |
VHSv20240731 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
videoDetection |
VIDEODR2 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
|
SerIdx1D |
videoDetection |
VIDEODR3 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
videoDetection |
VIDEODR4 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
videoDetection |
VIDEODR5 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
videoDetection |
VIDEOv20100513 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
|
SerIdx1D |
videoDetection |
VIDEOv20111208 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
|
SerIdx1D |
videoListRemeasurement |
VIDEOv20100513 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGDR2 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGDR3 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGDR4 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGv20111019 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGv20130417 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGv20140402 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGv20150421 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGv20151230 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGv20160406 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGv20161202 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection |
VIKINGv20170715 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vmcdeepDetection |
VMCDEEPv20230713 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx1D |
vmcdeepDetection |
VMCDEEPv20240506 |
Power law index {catalogue TType keyword: 1D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
sharksDetection |
SHARKSv20210222 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
sharksDetection |
SHARKSv20210421 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSDR2 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSDR3 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSDR4 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSDR5 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSDR6 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20120926 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20130417 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20140409 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20150108 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20160114 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20160507 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20170630 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20180419 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20201209 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20231101 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection |
VHSv20240731 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
videoDetection |
VIDEODR2 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
|
SerIdx2D |
videoDetection |
VIDEODR3 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
videoDetection |
VIDEODR4 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
videoDetection |
VIDEODR5 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
videoDetection |
VIDEOv20100513 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
|
SerIdx2D |
videoDetection |
VIDEOv20111208 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_index} |
real |
4 |
|
-0.9999995e9 |
|
SerIdx2D |
videoListRemeasurement |
VIDEOv20100513 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGDR2 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGDR3 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGDR4 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGv20111019 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGv20130417 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGv20140402 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGv20150421 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGv20151230 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGv20160406 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGv20161202 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection |
VIKINGv20170715 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vmcdeepDetection |
VMCDEEPv20230713 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerIdx2D |
vmcdeepDetection |
VMCDEEPv20240506 |
Power law index {catalogue TType keyword: 2D_Sersic_index} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerMag1D |
sharksDetection |
SHARKSv20210222 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
sharksDetection |
SHARKSv20210421 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSDR2 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag1D |
vhsDetection |
VHSDR3 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag1D |
vhsDetection |
VHSDR4 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSDR5 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSDR6 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSv20120926 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag1D |
vhsDetection |
VHSv20130417 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag1D |
vhsDetection |
VHSv20140409 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag1D |
vhsDetection |
VHSv20150108 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSv20160114 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSv20160507 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSv20170630 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSv20180419 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSv20201209 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSv20231101 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection |
VHSv20240731 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag1D |
videoDetection |
VIDEODR2 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
|
SerMag1D |
videoDetection |
VIDEODR3 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerMag1D |
videoDetection |
VIDEODR4 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
videoDetection |
VIDEODR5 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
videoDetection |
VIDEOv20100513 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
|
SerMag1D |
videoDetection |
VIDEOv20111208 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
|
SerMag1D |
videoListRemeasurement |
VIDEOv20100513 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag1D |
vikingDetection |
VIKINGDR2 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag1D |
vikingDetection |
VIKINGDR3 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag1D |
vikingDetection |
VIKINGDR4 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag1D |
vikingDetection |
VIKINGv20111019 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag1D |
vikingDetection |
VIKINGv20130417 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag1D |
vikingDetection |
VIKINGv20140402 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag1D |
vikingDetection |
VIKINGv20150421 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vikingDetection |
VIKINGv20151230 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vikingDetection |
VIKINGv20160406 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vikingDetection |
VIKINGv20161202 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vikingDetection |
VIKINGv20170715 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag1D |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag1D |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated 1D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
sharksDetection |
SHARKSv20210222 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
sharksDetection |
SHARKSv20210421 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSDR2 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag2D |
vhsDetection |
VHSDR3 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag2D |
vhsDetection |
VHSDR4 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSDR5 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSDR6 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSv20120926 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag2D |
vhsDetection |
VHSv20130417 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag2D |
vhsDetection |
VHSv20140409 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag2D |
vhsDetection |
VHSv20150108 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSv20160114 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSv20160507 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSv20170630 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSv20180419 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSv20201209 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSv20231101 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection |
VHSv20240731 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag2D |
videoDetection |
VIDEODR2 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
|
SerMag2D |
videoDetection |
VIDEODR3 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerMag2D |
videoDetection |
VIDEODR4 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
videoDetection |
VIDEODR5 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
videoDetection |
VIDEOv20100513 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
|
SerMag2D |
videoDetection |
VIDEOv20111208 |
SExtractor parameter |
real |
4 |
|
-0.9999995e9 |
|
SerMag2D |
videoListRemeasurement |
VIDEOv20100513 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag2D |
vikingDetection |
VIKINGDR2 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag2D |
vikingDetection |
VIKINGDR3 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag2D |
vikingDetection |
VIKINGDR4 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag2D |
vikingDetection |
VIKINGv20111019 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag2D |
vikingDetection |
VIKINGv20130417 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag2D |
vikingDetection |
VIKINGv20140402 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param |
SerMag2D |
vikingDetection |
VIKINGv20150421 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vikingDetection |
VIKINGv20151230 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vikingDetection |
VIKINGv20160406 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vikingDetection |
VIKINGv20161202 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vikingDetection |
VIKINGv20170715 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
PHOT_PROFILE |
SerMag2D |
vmcdeepDetection |
VMCDEEPv20230713 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerMag2D |
vmcdeepDetection |
VMCDEEPv20240506 |
Calibrated 2D Sersic flux [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
mag |
-0.9999995e9 |
stat.fit.param;phot.mag |
SerScaleLen1D |
sharksDetection |
SHARKSv20210222 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
sharksDetection |
SHARKSv20210421 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSDR2 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSDR3 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSDR4 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSDR5 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSDR6 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20120926 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20130417 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20140409 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20150108 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20160114 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20160507 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20170630 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20180419 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20201209 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20231101 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection |
VHSv20240731 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
videoDetection |
VIDEODR2 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
|
SerScaleLen1D |
videoDetection |
VIDEODR3 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
videoDetection |
VIDEODR4 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
videoDetection |
VIDEODR5 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
videoDetection |
VIDEOv20100513 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
|
SerScaleLen1D |
videoDetection |
VIDEOv20111208 |
SExtractor parameter {catalogue TType keyword: 1D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
|
SerScaleLen1D |
videoListRemeasurement |
VIDEOv20100513 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGDR2 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGDR3 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGDR4 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGv20111019 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGv20130417 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGv20140402 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGv20150421 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGv20151230 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGv20160406 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGv20161202 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection |
VIKINGv20170715 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vmcdeepDetection |
VMCDEEPv20230713 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen1D |
vmcdeepDetection |
VMCDEEPv20240506 |
Scale length {catalogue TType keyword: 1D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
sharksDetection |
SHARKSv20210222 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
sharksDetection |
SHARKSv20210421 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
ultravistaDetection |
ULTRAVISTADR4 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSDR2 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSDR3 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSDR4 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSDR5 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSDR6 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20120926 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20130417 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20140409 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20150108 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20160114 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20160507 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20170630 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20180419 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20201209 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20231101 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection |
VHSv20240731 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
videoDetection |
VIDEODR2 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
|
SerScaleLen2D |
videoDetection |
VIDEODR3 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
videoDetection |
VIDEODR4 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
videoDetection |
VIDEODR5 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
videoDetection |
VIDEOv20100513 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
|
SerScaleLen2D |
videoDetection |
VIDEOv20111208 |
SExtractor parameter {catalogue TType keyword: 2D_Sersic_scale_len} |
real |
4 |
|
-0.9999995e9 |
|
SerScaleLen2D |
videoListRemeasurement |
VIDEOv20100513 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGDR2 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGDR3 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGDR4 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGv20111019 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGv20130417 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGv20140402 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGv20150421 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGv20151230 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGv20160406 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGv20161202 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection |
VIKINGv20170715 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vmcdeepDetection |
VMCDEEPv20230713 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SerScaleLen2D |
vmcdeepDetection |
VMCDEEPv20240506 |
Scale length {catalogue TType keyword: 2D_Sersic_scale_len} [For numerical stability the Sersic fits will use the previously derived x-y coordinates] |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
SERSIC |
mgcGalaxyStruct |
MGC |
Sersic Index (=4 for de Vaucouleurs profile) |
real |
4 |
|
99.99 |
|
SERSIC_KAPPA |
mgcGalaxyStruct |
MGC |
Sersic profile coefficient |
real |
4 |
|
|
|
SERSICm |
mgcGalaxyStruct |
MGC |
Sersic Index error (-) |
real |
4 |
|
99.99 |
|
SERSICp |
mgcGalaxyStruct |
MGC |
Sersic Index error (+) |
real |
4 |
|
99.99 |
|
ses1_100 |
iras_psc |
IRAS |
Number of seconds-confirmed nearby small extended sources (100 micron). |
tinyint |
1 |
|
|
instr.param |
ses1_12 |
iras_psc |
IRAS |
Number of seconds-confirmed nearby small extended sources (12 micron). |
tinyint |
1 |
|
|
instr.param |
ses1_25 |
iras_psc |
IRAS |
Number of seconds-confirmed nearby small extended sources (25 micron). |
tinyint |
1 |
|
|
instr.param |
ses1_60 |
iras_psc |
IRAS |
Number of seconds-confirmed nearby small extended sources (60 micron). |
tinyint |
1 |
|
|
instr.param |
ses2_100 |
iras_psc |
IRAS |
Number of nearby weeks-confirmed small extended sources (100 micron). |
tinyint |
1 |
|
|
meta.code |
ses2_12 |
iras_psc |
IRAS |
Number of nearby weeks-confirmed small extended sources (12 micron). |
tinyint |
1 |
|
|
meta.code |
ses2_25 |
iras_psc |
IRAS |
Number of nearby weeks-confirmed small extended sources (25 micron). |
tinyint |
1 |
|
|
meta.code |
ses2_60 |
iras_psc |
IRAS |
Number of nearby weeks-confirmed small extended sources (60 micron). |
tinyint |
1 |
|
|
meta.code |
setupID |
RegionFieldLinks |
SHARKSv20210421 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
ULTRAVISTADR4 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VHSv20201209 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VHSv20231101 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VHSv20240731 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VMCDEEPv20230713 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VMCDEEPv20240506 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VMCDR5 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VMCv20191212 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VMCv20210708 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VMCv20230816 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VMCv20240226 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VVVDR5 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks |
VVVXDR1 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RegionFieldLinks, RequiredMosaic |
SHARKSv20210222 |
UID of top level setup. |
int |
4 |
|
-99999999 |
|
setupID |
RequiredMapAverages |
SHARKSv20210222 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
SHARKSv20210421 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
ULTRAVISTADR4 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VHSv20201209 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VHSv20231101 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VHSv20240731 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VMCDEEPv20230713 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VMCDEEPv20240506 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VMCDR5 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VMCv20191212 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VMCv20210708 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VMCv20230816 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VMCv20240226 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VVVDR5 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMapAverages |
VVVXDR1 |
the setupID of the averaging process |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
SHARKSv20210222 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
SHARKSv20210421 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
ULTRAVISTADR4 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VHSv20201209 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VHSv20231101 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VHSv20240731 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VMCDEEPv20230713 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VMCDEEPv20240506 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VMCDR5 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VMCv20191212 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VMCv20210708 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VMCv20230816 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VMCv20240226 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VVVDR5 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
setupID |
RequiredMosaicTopLevel |
VVVXDR1 |
the unique setup ID. Probably one per programme, but just in case |
int |
4 |
|
|
meta.id;meta.main |
SEX_FLAG |
mgcGalaxyStruct |
MGC |
SExtractor Flag |
int |
4 |
Integer |
|
|
SG |
target |
SIXDF |
SSS star/galaxy flag 1=galaxy 2=star 3=unclass 4=noise |
smallint |
2 |
|
|
|
sharp |
smashdr2_deep, smashdr2_object |
SMASH |
Average DAOPHOT sharp value, measurement of peakiness |
real |
4 |
|
|
|
sharp |
smashdr2_source |
SMASH |
DAOPHOT sharp value, measurement of peakiness |
real |
4 |
|
|
|
sharp |
vvvPsfDaophotJKsSource |
VVVDR5 |
Sharpness of the gaussian [-1,1] {catalogue TType keyword: sharp} |
real |
4 |
|
|
stat.fit.goodness |
SHARPL15 |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Sharpness |
float |
8 |
|
99.999 |
|
SHARPL24 |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Sharpness |
float |
8 |
|
99.999 |
|
SHARPN3 |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Sharpness |
float |
8 |
|
99.999 |
|
SHARPS11 |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Sharpness |
float |
8 |
|
99.999 |
|
SHARPS7 |
akari_lmc_psa_v1, akari_lmc_psc_v1 |
AKARI |
Sharpness |
float |
8 |
|
99.999 |
|
shortName |
Filter |
SHARKSv20210222 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
SHARKSv20210421 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
ULTRAVISTADR4 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSDR1 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSDR2 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSDR3 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSDR4 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSDR5 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSDR6 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSv20120926 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSv20130417 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSv20150108 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSv20160114 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSv20160507 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSv20170630 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSv20180419 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSv20201209 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSv20231101 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VHSv20240731 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIDEODR2 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIDEODR3 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIDEODR4 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIDEODR5 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIDEOv20100513 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIDEOv20111208 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGDR2 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGDR3 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGDR4 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGv20110714 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGv20111019 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGv20130417 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGv20150421 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGv20151230 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGv20160406 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGv20161202 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VIKINGv20170715 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCDEEPv20230713 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCDEEPv20240506 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCDR1 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCDR3 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCDR4 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCDR5 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20110816 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20110909 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20120126 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20121128 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20130304 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20130805 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20140428 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20140903 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20150309 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20151218 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20160311 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20160822 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20170109 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20170411 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20171101 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20180702 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20181120 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20191212 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20210708 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20230816 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VMCv20240226 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VSAQC |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VVVDR1 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VVVDR2 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VVVDR5 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VVVXDR1 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VVVv20100531 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
Filter |
VVVv20110718 |
Short identification name for the filter |
varchar |
10 |
|
|
?? |
shortName |
FilterExtinctionCoefficients |
EXTINCT |
Short name of the filter |
varchar |
8 |
|
|
meta.id |
shortName |
FilterSections |
SHARKSv20210222 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
SHARKSv20210421 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
ULTRAVISTADR4 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSDR3 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSDR4 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSDR5 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSDR6 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSv20150108 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSv20160114 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSv20160507 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSv20170630 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSv20180419 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSv20201209 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSv20231101 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VHSv20240731 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VIDEODR4 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VIDEODR5 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VIKINGDR4 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VIKINGv20150421 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VIKINGv20151230 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VIKINGv20160406 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VIKINGv20161202 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VIKINGv20170715 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCDEEPv20230713 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCDEEPv20240506 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCDR3 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCDR4 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCDR5 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20140428 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20140903 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20150309 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20151218 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20160311 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20160822 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20170109 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20170411 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20171101 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20180702 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20181120 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20191212 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20210708 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20230816 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VMCv20240226 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VSAQC |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VVVDR5 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
FilterSections |
VVVXDR1 |
Short identification name for the filter section |
varchar |
10 |
|
|
?? |
shortName |
vmcRRLyraeLightCurves |
VMCv20240226 |
Filter name |
varchar |
2 |
|
|
instr.bandpass |
Si |
ravedr5Source |
RAVE |
[Si/H] abundance of Si |
real |
4 |
dex |
|
phys.abund.Z |
Si_N |
ravedr5Source |
RAVE |
Number of used spectral lines in calc. of [Si/H] |
smallint |
2 |
|
|
meta.number |
siga |
sharksAstrometricInfo |
SHARKSv20210222 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
sharksAstrometricInfo |
SHARKSv20210421 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
ultravistaAstrometricInfo |
ULTRAVISTADR4 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vhsAstrometricInfo |
VHSDR6 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vhsAstrometricInfo |
VHSv20170630 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vhsAstrometricInfo |
VHSv20180419 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vhsAstrometricInfo |
VHSv20201209 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vhsAstrometricInfo |
VHSv20231101 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vhsAstrometricInfo |
VHSv20240731 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
videoAstrometricInfo |
VIDEODR2 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
siga |
videoAstrometricInfo |
VIDEODR3 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
videoAstrometricInfo |
VIDEODR4 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
videoAstrometricInfo |
VIDEODR5 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
videoAstrometricInfo |
VIDEOv20111208 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
siga |
vikingAstrometricInfo |
VIKINGDR2 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
siga |
vikingAstrometricInfo |
VIKINGDR3 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vikingAstrometricInfo |
VIKINGDR4 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vikingAstrometricInfo |
VIKINGv20110714 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
siga |
vikingAstrometricInfo |
VIKINGv20111019 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
siga |
vikingAstrometricInfo |
VIKINGv20130417 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vikingAstrometricInfo |
VIKINGv20140402 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vikingAstrometricInfo |
VIKINGv20150421 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vikingAstrometricInfo |
VIKINGv20151230 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vikingAstrometricInfo |
VIKINGv20160406 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vikingAstrometricInfo |
VIKINGv20161202 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vikingAstrometricInfo |
VIKINGv20170715 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCDR1 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
siga |
vmcAstrometricInfo |
VMCDR2 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCDR3 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCDR4 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCDR5 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20110816 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
siga |
vmcAstrometricInfo |
VMCv20110909 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
siga |
vmcAstrometricInfo |
VMCv20120126 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
siga |
vmcAstrometricInfo |
VMCv20121128 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20130304 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20130805 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20140428 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20140903 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20150309 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20151218 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20160311 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20160822 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20170109 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20170411 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20171101 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20180702 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20181120 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20191212 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20210708 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20230816 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcAstrometricInfo |
VMCv20240226 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcdeepAstrometricInfo |
VMCDEEPv20230713 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vmcdeepAstrometricInfo |
VMCDEEPv20240506 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vvvAstrometricInfo |
VVVDR1 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vvvAstrometricInfo |
VVVDR2 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vvvAstrometricInfo |
VVVDR5 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
siga |
vvvAstrometricInfo |
VVVv20110718 |
Error on coefficient a |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigd |
sharksAstrometricInfo |
SHARKSv20210222 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
sharksAstrometricInfo |
SHARKSv20210421 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
ultravistaAstrometricInfo |
ULTRAVISTADR4 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vhsAstrometricInfo |
VHSDR6 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vhsAstrometricInfo |
VHSv20170630 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vhsAstrometricInfo |
VHSv20180419 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vhsAstrometricInfo |
VHSv20201209 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vhsAstrometricInfo |
VHSv20231101 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vhsAstrometricInfo |
VHSv20240731 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
videoAstrometricInfo |
VIDEODR2 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigd |
videoAstrometricInfo |
VIDEODR3 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
videoAstrometricInfo |
VIDEODR4 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
videoAstrometricInfo |
VIDEODR5 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
videoAstrometricInfo |
VIDEOv20111208 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigd |
vikingAstrometricInfo |
VIKINGDR2 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigd |
vikingAstrometricInfo |
VIKINGDR3 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vikingAstrometricInfo |
VIKINGDR4 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vikingAstrometricInfo |
VIKINGv20110714 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigd |
vikingAstrometricInfo |
VIKINGv20111019 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigd |
vikingAstrometricInfo |
VIKINGv20130417 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vikingAstrometricInfo |
VIKINGv20140402 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vikingAstrometricInfo |
VIKINGv20150421 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vikingAstrometricInfo |
VIKINGv20151230 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vikingAstrometricInfo |
VIKINGv20160406 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vikingAstrometricInfo |
VIKINGv20161202 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vikingAstrometricInfo |
VIKINGv20170715 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCDR1 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigd |
vmcAstrometricInfo |
VMCDR2 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCDR3 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCDR4 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCDR5 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20110816 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigd |
vmcAstrometricInfo |
VMCv20110909 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigd |
vmcAstrometricInfo |
VMCv20120126 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigd |
vmcAstrometricInfo |
VMCv20121128 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20130304 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20130805 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20140428 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20140903 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20150309 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20151218 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20160311 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20160822 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20170109 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20170411 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20171101 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20180702 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20181120 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20191212 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20210708 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20230816 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcAstrometricInfo |
VMCv20240226 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcdeepAstrometricInfo |
VMCDEEPv20230713 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vmcdeepAstrometricInfo |
VMCDEEPv20240506 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vvvAstrometricInfo |
VVVDR1 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vvvAstrometricInfo |
VVVDR2 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vvvAstrometricInfo |
VVVDR5 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
stat.fit;stat.stdev |
sigd |
vvvAstrometricInfo |
VVVv20110718 |
Error on coefficient d |
float |
8 |
arcsec |
-0.9999995e9 |
?? |
sigDec |
sharksVariability |
SHARKSv20210222 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
sharksVariability |
SHARKSv20210421 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
ultravistaVariability |
ULTRAVISTADR4 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vhsSourceRemeasurement |
VHSDR1 |
Uncertainty in Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigDec |
videoSourceRemeasurement |
VIDEOv20100513 |
Uncertainty in Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigDec |
videoVariability |
VIDEODR2 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
videoVariability |
VIDEODR3 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
videoVariability |
VIDEODR4 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
videoVariability |
VIDEODR5 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
videoVariability |
VIDEOv20100513 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
videoVariability |
VIDEOv20111208 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingSourceRemeasurement |
VIKINGv20110714 |
Uncertainty in Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigDec |
vikingSourceRemeasurement |
VIKINGv20111019 |
Uncertainty in Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigDec |
vikingVariability |
VIKINGDR2 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGDR3 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGDR4 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGv20110714 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGv20111019 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGv20130417 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGv20140402 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGv20150421 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGv20151230 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGv20160406 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGv20161202 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vikingVariability |
VIKINGv20170715 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcSourceRemeasurement |
VMCv20110816 |
Uncertainty in Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigDec |
vmcSourceRemeasurement |
VMCv20110909 |
Uncertainty in Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigDec |
vmcVariability |
VMCDR1 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCDR2 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCDR3 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCDR4 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCDR5 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20110816 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20110909 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20120126 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20121128 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20130304 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20130805 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20140428 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20140903 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20150309 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20151218 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20160311 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20160822 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20170109 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20170411 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20171101 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20180702 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20181120 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20191212 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20210708 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20230816 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcVariability |
VMCv20240226 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcdeepVariability |
VMCDEEPv20230713 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vmcdeepVariability |
VMCDEEPv20240506 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vvvSourceRemeasurement |
VVVv20100531 |
Uncertainty in Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigDec |
vvvSourceRemeasurement |
VVVv20110718 |
Uncertainty in Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigDec |
vvvVariability |
VVVDR1 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vvvVariability |
VVVDR2 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vvvVariability |
VVVDR5 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vvvVariability |
VVVv20100531 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigDec |
vvvVariability |
VVVv20110718 |
Uncertainty in mean Dec |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigdec |
allwise_sc |
WISE |
One-sigma uncertainty in declination coordinate from the non-moving source extraction. |
float |
8 |
arcsec |
|
|
sigdec |
catwise_2020, catwise_prelim |
WISE |
uncertainty in dec (arcsec) |
real |
4 |
arcsec |
|
|
sigdec |
wise_allskysc |
WISE |
One-sigma uncertainty in declination coordinate |
real |
4 |
arcsec |
|
|
sigdec |
wise_prelimsc |
WISE |
One-sigma uncertainty in declination coordinate CAUTION: The declination uncertainty is overestimated for the majority of sources in the Preliminary Release Source Catalog. Sigdec was computed by adding 0.5 arcsec in quadrature to the extraction measurement uncertainty to reflect the impact of the declination bias error known to affect a fraction of source fainter than W1~13.0 mag |
real |
4 |
arcsec |
|
|
sigdec_pm |
allwise_sc |
WISE |
One-sigma uncertainty in declination from the profile-fitting measurement model that includes motion. This column is null if the motion-fit failed to converge or was not attempted. |
float |
8 |
arcsec |
|
|
sigdec_pm |
catwise_2020, catwise_prelim |
WISE |
uncertainty in dec_pm |
real |
4 |
arcsec |
|
|
sigDecCen |
ultravistaSourceRemeasurement |
ULTRAVISTADR4 |
Uncertainty in Dec of centroid |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error;pos.eq.dec |
sigDecCen |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20160909 |
Uncertainty in Dec of centroid |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error;pos.eq.dec |
sigDecCen |
vikingZY_selJ_SourceRemeasurement |
VIKINGZYSELJv20170124 |
Uncertainty in Dec of centroid |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error;pos.eq.dec |
sigMuDec |
sharksVariability |
SHARKSv20210222 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
sharksVariability |
SHARKSv20210421 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
ultravistaVariability |
ULTRAVISTADR4 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
videoVariability |
VIDEODR2 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
videoVariability |
VIDEODR3 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
videoVariability |
VIDEODR4 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
videoVariability |
VIDEODR5 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
videoVariability |
VIDEOv20100513 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
videoVariability |
VIDEOv20111208 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGDR2 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGDR3 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGDR4 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGv20110714 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGv20111019 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGv20130417 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGv20140402 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGv20150421 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGv20151230 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGv20160406 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGv20161202 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vikingVariability |
VIKINGv20170715 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCDR1 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCDR2 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCDR3 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCDR4 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCDR5 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20110816 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20110909 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20120126 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20121128 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20130304 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20130805 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20140428 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20140903 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20150309 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20151218 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20160311 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20160822 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20170109 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20170411 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20171101 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20180702 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20181120 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20191212 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20210708 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20230816 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcVariability |
VMCv20240226 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcdeepVariability |
VMCDEEPv20230713 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vmcdeepVariability |
VMCDEEPv20240506 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vvvVariability |
VVVDR1 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vvvVariability |
VVVDR2 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vvvVariability |
VVVDR5 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vvvVariability |
VVVv20100531 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuDec |
vvvVariability |
VVVv20110718 |
Error on proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
sharksVariability |
SHARKSv20210222 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
sharksVariability |
SHARKSv20210421 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
ultravistaVariability |
ULTRAVISTADR4 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
videoVariability |
VIDEODR2 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
videoVariability |
VIDEODR3 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
videoVariability |
VIDEODR4 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
videoVariability |
VIDEODR5 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
videoVariability |
VIDEOv20100513 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
videoVariability |
VIDEOv20111208 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGDR2 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGDR3 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGDR4 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGv20110714 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGv20111019 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGv20130417 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGv20140402 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGv20150421 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGv20151230 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGv20160406 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGv20161202 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vikingVariability |
VIKINGv20170715 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCDR1 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCDR2 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCDR3 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCDR4 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCDR5 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20110816 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20110909 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20120126 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20121128 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20130304 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20130805 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20140428 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20140903 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20150309 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20151218 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20160311 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20160822 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20170109 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20170411 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20171101 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20180702 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20181120 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20191212 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20210708 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20230816 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcVariability |
VMCv20240226 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcdeepVariability |
VMCDEEPv20230713 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vmcdeepVariability |
VMCDEEPv20240506 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vvvVariability |
VVVDR1 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vvvVariability |
VVVDR2 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vvvVariability |
VVVDR5 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vvvVariability |
VVVv20100531 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigMuRa |
vvvVariability |
VVVv20110718 |
Error on proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
stat.error |
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. |
sigPMDec |
catwise_2020, catwise_prelim |
WISE |
uncertainty in PMDec |
real |
4 |
arcsec/yr |
|
|
sigpmdec |
allwise_sc |
WISE |
Uncertainty in the Dec motion estimated for this source. This column is null if the motion fit failed to converge or was not attempted. |
int |
4 |
mas/year |
|
|
sigPMRA |
catwise_2020, catwise_prelim |
WISE |
uncertainty in PMRA |
real |
4 |
arcsec/yr |
|
|
sigpmra |
allwise_sc |
WISE |
Uncertainty in the RA motion estimation. This column is null if the motion fit failed to converge or was not attempted. |
int |
4 |
mas/year |
|
|
sigRa |
sharksVariability |
SHARKSv20210222 |
Uncertainty in mean RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigRa |
sharksVariability |
SHARKSv20210421 |
Uncertainty in mean RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigRa |
ultravistaVariability |
ULTRAVISTADR4 |
Uncertainty in mean RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigRa |
vhsSourceRemeasurement |
VHSDR1 |
Uncertainty in RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigRa |
videoSourceRemeasurement |
VIDEOv20100513 |
Uncertainty in RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigRa |
videoVariability |
VIDEODR2 |
Uncertainty in mean RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigRa |
videoVariability |
VIDEODR3 |
Uncertainty in mean RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigRa |
videoVariability |
VIDEODR4 |
Uncertainty in mean RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigRa |
videoVariability |
VIDEODR5 |
Uncertainty in mean RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigRa |
videoVariability |
VIDEOv20100513 |
Uncertainty in mean RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigRa |
videoVariability |
VIDEOv20111208 |
Uncertainty in mean RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigRa |
vikingSourceRemeasurement |
VIKINGv20110714 |
Uncertainty in RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigRa |
vikingSourceRemeasurement |
VIKINGv20111019 |
Uncertainty in RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
sigRa |
vikingVariability |
VIKINGDR2 |
Uncertainty in mean RA |
real |
4 |
Degrees |
-0.9999995e9 |
stat.error |
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. |
sigRa |
vikingVariability |
VIKINGDR3 |
Uncertainty in mean RA |
|