D |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
D_MODULUS |
mgcGalaxyStruct |
MGC |
B proper distance to the object (h=1) |
real |
4 |
Mpc |
|
|
darkID |
Multiframe |
WSA |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
ID_FRAME |
darkID |
Multiframe |
WSACalib |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
ID_FRAME |
darkID |
Multiframe |
WSATransit |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
ID_FRAME |
databaseName |
ExternalSurvey |
WSA |
The name of the database within the WSA |
varchar |
16 |
|
|
ID_DATABASE |
databaseName |
ExternalSurvey |
WSACalib |
The name of the database within the WSA |
varchar |
16 |
|
|
ID_DATABASE |
databaseName |
ExternalSurvey |
WSATransit |
The name of the database within the WSA |
varchar |
16 |
|
|
ID_DATABASE |
dataScale |
MultiframeDetector |
WSA |
Scaling of pixel values {image extension keyword: BSCALE} |
real |
4 |
|
1.0 |
?? |
dataScale |
MultiframeDetector |
WSACalib |
Scaling of pixel values {image extension keyword: BSCALE} |
real |
4 |
|
1.0 |
?? |
dataScale |
MultiframeDetector |
WSATransit |
Scaling of pixel values {image extension keyword: BSCALE} |
real |
4 |
|
1.0 |
?? |
dataZero |
MultiframeDetector |
WSA |
Zeropoint of pixel values {image extension keyword: BZERO} |
real |
4 |
|
0.0 |
?? |
dataZero |
MultiframeDetector |
WSACalib |
Zeropoint of pixel values {image extension keyword: BZERO} |
real |
4 |
|
0.0 |
?? |
dataZero |
MultiframeDetector |
WSATransit |
Zeropoint of pixel values {image extension keyword: BZERO} |
real |
4 |
|
0.0 |
?? |
date |
twomass_psc, twomass_xsc |
2MASS |
The observation reference date for this source expressed in ISO standard format. (YYYY-MM-DD) |
datetime |
8 |
yyyy-mm-dd |
|
TIME_DATE |
date |
twomass_scn |
2MASS |
The observation reference date for this scan expressed in ISO standard format. (YYYY-MM-DD) |
datetime |
8 |
yyyy-mm-dd |
|
TIME_DATE |
dateEnd |
Multiframe |
WSA |
Date and time (UTC) of end of the observation {image primary HDU keyword: DATE-END} |
datetime |
8 |
|
12-31-9999 |
TIME_DATE |
dateEnd |
Multiframe |
WSACalib |
Date and time (UTC) of end of the observation {image primary HDU keyword: DATE-END} |
datetime |
8 |
|
12-31-9999 |
TIME_DATE |
dateEnd |
Multiframe |
WSATransit |
Date and time (UTC) of end of the observation {image primary HDU keyword: DATE-END} |
datetime |
8 |
|
12-31-9999 |
TIME_DATE |
dateObs |
Multiframe |
WSA |
Date and time (UTC) of start of the observation {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
TIME_DATE |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
WSACalib |
Date and time (UTC) of start of the observation {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
TIME_DATE |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dateObs |
Multiframe |
WSATransit |
Date and time (UTC) of start of the observation {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
TIME_DATE |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dbName |
Release |
WSA |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
WSACalib |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbName |
Release |
WSATransit |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbNamePrefix |
Survey |
WSA |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
WSACalib |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
dbNamePrefix |
Survey |
WSATransit |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
deblend |
UKIDSSDetection |
WSA |
Placeholder flag for parent or part of deblended deconstruct (redundant since only deblended images are kept) |
int |
4 |
|
|
CODE_MISC |
deblend |
calDetection |
WSACalib |
Placeholder flag for parent or part of deblended deconstruct (redundant since only deblended images are kept) {catalogue TType keyword: Parent_or_child} |
int |
4 |
|
|
CODE_MISC |
This CASU pipeline processing source extraction flag is a placeholder only, and is always set to zero. If you need to know when a particular image detection is a component of a deblend or not, test bit 4 of attribute ppErrBits (see corresponding glossary entry) which is set by WFAU's post-processing software based on testing the areal profiles aprof2-8 (these are set by CASU to -1 for deblended components, or positive values for non-deblended detections). We encode this in an information bit of ppErrBits for convenience when querying the detection and source tables. |
deblend |
calListRemeasurement |
WSACalib |
placeholder flag for parent or part of deblended deconstruct (redundant since only deblended images are kept) {catalogue TType keyword: Parent_or_child} |
int |
4 |
|
|
CODE_MISC |
deblend |
dxsDetection, gcsDetection, gpsDetection, lasDetection |
WSA |
Placeholder flag for parent or part of deblended deconstruct (redundant since only deblended images are kept) {catalogue TType keyword: Parent_or_child} |
int |
4 |
|
|
CODE_MISC |
This CASU pipeline processing source extraction flag is a placeholder only, and is always set to zero. If you need to know when a particular image detection is a component of a deblend or not, test bit 4 of attribute ppErrBits (see corresponding glossary entry) which is set by WFAU's post-processing software based on testing the areal profiles aprof2-8 (these are set by CASU to -1 for deblended components, or positive values for non-deblended detections). We encode this in an information bit of ppErrBits for convenience when querying the detection and source tables. |
deblend |
dxsListRemeasurement, gcsListRemeasurement, gpsListRemeasurement, lasListRemeasurement, udsListRemeasurement |
WSA |
placeholder flag for parent or part of deblended deconstruct (redundant since only deblended images are kept) {catalogue TType keyword: Parent_or_child} |
int |
4 |
|
|
CODE_MISC |
deblend |
ptsDetection |
WSATransit |
Placeholder flag for parent or part of deblended deconstruct (redundant since only deblended images are kept) {catalogue TType keyword: Parent_or_child} |
int |
4 |
|
|
CODE_MISC |
This CASU pipeline processing source extraction flag is a placeholder only, and is always set to zero. If you need to know when a particular image detection is a component of a deblend or not, test bit 4 of attribute ppErrBits (see corresponding glossary entry) which is set by WFAU's post-processing software based on testing the areal profiles aprof2-8 (these are set by CASU to -1 for deblended components, or positive values for non-deblended detections). We encode this in an information bit of ppErrBits for convenience when querying the detection and source tables. |
deblend |
udsDetection |
WSA |
Not available in SE output {catalogue TType keyword: Parent_or_child} |
int |
4 |
|
-99999999 |
|
DEC |
twoxmm |
XMM |
Corrected Declination of the detection in degrees (J2000) after statistical correlation of the emldetect coordinates, RA_UNC and DEC_UNC, with the USNO B1.0 optical source catalogue using the SAS task eposcorr. In case where the cross-correlation is determined to be unreliable no correction is applied and this value is therefore the same as DEC_UNC. |
float |
8 |
degrees |
|
|
dec |
RequiredMosaic |
WSA |
Declination of mosaic centre |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
RequiredMosaic |
WSACalib |
Declination of mosaic centre |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
RequiredMosaic |
WSATransit |
Declination of mosaic centre |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
RequiredStack |
WSA |
Declination of stack centre |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
RequiredStack |
WSACalib |
Declination of stack centre |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
RequiredStack |
WSATransit |
Declination of stack centre |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
dxsJKsource, gcsPointSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, lasExtendedSource, lasPointSource, lasYJHKsource, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, UKIDSSDetection |
WSA |
Celestial Declination |
float |
8 |
Degrees |
|
POS_EQ_DEC_MAIN |
dec |
calDetection, calListRemeasurement, calSource, calSourceRemeasurement, calSynopticSource |
WSACalib |
Celestial Declination |
float |
8 |
Degrees |
|
POS_EQ_DEC_MAIN |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
calMergeLog, calSynopticMergeLog |
WSACalib |
Declination of field centre |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
calVariability |
WSACalib |
Mean Declination |
float |
8 |
Degrees |
|
POS_EQ_DEC_MAIN |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
dxsDetection, dxsListRemeasurement, dxsSource, dxsSourceRemeasurement, gcsDetection, gcsListRemeasurement, gcsSource, gcsSourceRemeasurement, gpsDetection, gpsListRemeasurement, gpsSource, gpsSourceRemeasurement, lasDetection, lasListRemeasurement, lasSource, lasSourceRemeasurement, udsDetection, udsListRemeasurement, udsSource, udsSourceRemeasurement |
WSA |
Celestial Declination |
float |
8 |
Degrees |
|
POS_EQ_DEC_MAIN |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
dxsJKmergeLog, dxsMergeLog, gcsMergeLog, gcsZYJHKmergeLog, gpsJHKmergeLog, gpsMergeLog, lasMergeLog, lasYJHKmergeLog, udsMergeLog |
WSA |
Declination of field centre |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
dxsVariability, udsVariability |
WSA |
Mean Declination |
float |
8 |
Degrees |
|
POS_EQ_DEC_MAIN |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
dec |
firstSource |
FIRST |
J2000 Celestial Declination |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca, glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Declination (J2000) |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
iras_psc |
IRAS |
J2000 Celestial Declination |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
mgcDetection |
MGC |
Object declination (J2000) |
float |
8 |
deg |
|
|
dec |
nvssSource |
NVSS |
J2000 Celestial Declination |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
ptsDetection |
WSATransit |
Celestial Declination |
float |
8 |
Degrees |
|
POS_EQ_DEC_MAIN |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
rosat_bsc, rosat_fsc |
ROSAT |
Declination (decimal degrees; J2000) |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
twomass_psc |
2MASS |
J2000 declination with respect to the ICRS |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
twomass_scn |
2MASS |
Declination of scan center for equinox J2000. |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
twomass_xsc |
2MASS |
Declination (J2000 decimal deg) based on peak pixel. |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
ukirtFSstars |
WSA |
Declination of star at Equinox J2000.0 |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
ukirtFSstars |
WSACalib |
Declination of star at Equinox J2000.0 |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec_1 |
twomass_scn |
2MASS |
J2000 declination of the eastern corner at start of scan. |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec_2 |
twomass_scn |
2MASS |
J2000 declination of the western corner at start of scan. |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec_3 |
twomass_scn |
2MASS |
J2000 declination of the eastern corner at end of scan. |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec_4 |
twomass_scn |
2MASS |
J2000 declination of the western corner at end of scan. |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec_err |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca, glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Error in Declination |
float |
8 |
arcsec |
|
ERROR |
DEC_UNC |
twoxmm |
XMM |
Declination of the source in degrees (J2000) as determined by the SAS task emldetect by fitting a detection simultaneously in all cameras and energy bands. |
float |
8 |
degrees |
|
|
decB1950 |
mgcDetection |
MGC |
Object declination (B1950) |
float |
8 |
deg |
|
|
decBase |
Multiframe |
WSA |
Declination of base position {image primary HDU keyword: DECBASE} |
float |
8 |
degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
decBase |
Multiframe |
WSACalib |
Declination of base position {image primary HDU keyword: DECBASE} |
float |
8 |
degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
decBase |
Multiframe |
WSATransit |
Declination of base position {image primary HDU keyword: DECBASE} |
float |
8 |
degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
decCentre |
StdFieldInfo |
WSA |
Declination of field centre |
float |
8 |
degrees |
|
POS_EQ_RA_MAIN |
decCentre |
StdFieldInfo |
WSACalib |
Declination of field centre |
float |
8 |
degrees |
|
POS_EQ_RA_MAIN |
decExtent |
RequiredMosaic |
WSA |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
WSACalib |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decExtent |
RequiredMosaic |
WSATransit |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decMoon |
Multiframe |
WSA |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
decMoon |
Multiframe |
WSACalib |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
decMoon |
Multiframe |
WSATransit |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
decMoonTopo |
Multiframe |
WSA |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
decMoonTopo |
Multiframe |
WSACalib |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
decMoonTopo |
Multiframe |
WSATransit |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
decTelOff |
Multiframe |
WSA |
Declination telescope offset {image primary HDU keyword: TDECOFF} |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_DEC_OFF |
decTelOff |
Multiframe |
WSACalib |
Declination telescope offset {image primary HDU keyword: TDECOFF} |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_DEC_OFF |
decTelOff |
Multiframe |
WSATransit |
Declination telescope offset {image primary HDU keyword: TDECOFF} |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_DEC_OFF |
decurtainRange |
MultiframeDetector |
WSA |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
WSACalib |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtainRange |
MultiframeDetector |
WSATransit |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtFlag |
MultiframeDetector |
WSA |
De-curtaining flag {image extension keyword: DECURTN} |
varchar |
32 |
|
NONE |
?? |
decurtFlag |
MultiframeDetector |
WSACalib |
De-curtaining flag {image extension keyword: DECURTN} |
varchar |
32 |
|
NONE |
?? |
decurtFlag |
MultiframeDetector |
WSATransit |
De-curtaining flag {image extension keyword: DECURTN} |
varchar |
32 |
|
NONE |
?? |
delPropData |
SurveyProgrammes |
WSA |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
WSACalib |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
delPropData |
SurveyProgrammes |
WSATransit |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
density |
twomass_xsc |
2MASS |
Coadd log(density) of stars with k<14 mag. |
real |
4 |
|
|
PHYS_DENSITY_NUMBER |
deprecated |
Multiframe |
WSA |
Code for a current (=0) or deprecated (!=0) multiframe |
tinyint |
1 |
|
0 |
CODE_MISC |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete MSBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 27 | Deprecated because frame is flagged as part of a summit-rejected MSB | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the GPS) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | 127 | Unwanted frame ingested. | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
WSACalib |
Code for a current (=0) or deprecated (!=0) multiframe |
tinyint |
1 |
|
0 |
CODE_MISC |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete MSBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 27 | Deprecated because frame is flagged as part of a summit-rejected MSB | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the GPS) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | 127 | Unwanted frame ingested. | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
Multiframe |
WSATransit |
Code for a current (=0) or deprecated (!=0) multiframe |
tinyint |
1 |
|
0 |
CODE_MISC |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete MSBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 27 | Deprecated because frame is flagged as part of a summit-rejected MSB | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the GPS) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | 127 | Unwanted frame ingested. | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
MultiframeDetector |
WSA |
Code for a current (=0) or deprecated (!=0) multiframe detector |
tinyint |
1 |
|
0 |
CODE_MISC |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete MSBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 27 | Deprecated because frame is flagged as part of a summit-rejected MSB | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the GPS) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | 127 | Unwanted frame ingested. | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
MultiframeDetector |
WSACalib |
Code for a current (=0) or deprecated (!=0) multiframe detector |
tinyint |
1 |
|
0 |
CODE_MISC |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete MSBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 27 | Deprecated because frame is flagged as part of a summit-rejected MSB | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the GPS) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | 127 | Unwanted frame ingested. | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
MultiframeDetector |
WSATransit |
Code for a current (=0) or deprecated (!=0) multiframe detector |
tinyint |
1 |
|
0 |
CODE_MISC |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete MSBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 27 | Deprecated because frame is flagged as part of a summit-rejected MSB | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the GPS) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | 127 | Unwanted frame ingested. | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
UKIDSSDetection |
WSA |
Code for a current (=0) or deprecated (!=0) detection |
tinyint |
1 |
|
0 |
CODE_MISC |
deprecated |
calDetection, calListRemeasurement |
WSACalib |
Code for a current (=0) or deprecated (!=0) detection |
tinyint |
1 |
|
0 |
CODE_MISC |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete MSBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 27 | Deprecated because frame is flagged as part of a summit-rejected MSB | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the GPS) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | 127 | Unwanted frame ingested. | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
calMergeLog, calSynopticMergeLog |
WSACalib |
frame set deprecation flag (1=deprecated) |
tinyint |
1 |
|
|
CODE_MISC |
deprecated |
dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsDetection, udsListRemeasurement |
WSA |
Code for a current (=0) or deprecated (!=0) detection |
tinyint |
1 |
|
0 |
CODE_MISC |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete MSBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 27 | Deprecated because frame is flagged as part of a summit-rejected MSB | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the GPS) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | 127 | Unwanted frame ingested. | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
deprecated |
dxsJKmergeLog, dxsMergeLog, gcsMergeLog, gcsZYJHKmergeLog, gpsJHKmergeLog, gpsMergeLog, lasMergeLog, lasYJHKmergeLog, udsMergeLog |
WSA |
frame set deprecation flag (1=deprecated) |
tinyint |
1 |
|
|
CODE_MISC |
deprecated |
ptsDetection |
WSATransit |
Code for a current (=0) or deprecated (!=0) detection |
tinyint |
1 |
|
0 |
CODE_MISC |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete MSBs) | 7 | Undefined values of critical catalogue attributes for stacks | 8 | Seeing=0.0 for a stack | 9 | High value of sky that compromises the depth, or otherwise invalid sky level (e.g. sky < 0) | 10 | Seeing outside specified maximum | 11 | Photometric zeropoint too bright | 12 | Average stellar ellipticity too high (> 0.25) | 13 | Depth (as calculated from sky noise and 5sigma detection in fixed aperture) is too shallow compared to overall histogram distribution (i.e. shallower than ~0.5mag wrt the modal value) OR sky noise is too high given the sky level | 14 | AperCor3 outlying in aperCor3 versus seeing distribution | 15 | Pipeline MAGZPT inconsistent between image PHDU, extension HDUs and/or catalogue extension HDUs (from attributes photZP, photZPExt and photZPCat) | 16 | Difference in detector sky level wrt to mean of all 4 detectors is outlying in the distribution of the same. | 18 | Provenance indicates that a constituent frame of a combined frame product includes a deprecated frame. | 19 | Inconsistent provenance for a stack or leav product indicating something wrong with the image product (usually screwed up FITS keywords confusing the pipeline) | 20 | Detector number counts indicate some problem (loads of crud images) | 21 | 5-sigma depth of detector frame more than 0.4mag brighter than modal value for a given filter/project/exposure time | 22 | Basic astrometry check (pixel size and/or aspect ratio) indicates something is wrong with the image | 26 | Deprecated because frame is flagged as ignored in pipeline processing | 27 | Deprecated because frame is flagged as part of a summit-rejected MSB | 40 | Science (*stack) frame is not part of a survey (e.g. high latitude sky frames in the GPS) | 60 | Eyeball check deprecation - trailed | 61 | Eyeball check deprecation - multiple bad channels | 62 | Eyeball check deprecation - Moon ghost | 63 | Eyeball check deprecation - Sky subtraction problem | 64 | Eyeball check deprecation - Disaster (catchall category for the indescribable) | 65 | Eyeball check deprecation - Empty detector frame | 66 | Eyeball check deprecation - Flat field problem | 67 | Eyeball check deprecation - Malfunction in crosstalk correction | 70 | Eyeball check deprecation, but this is the best that can be done so should not be reobserved (e.g. very bright star in FOV) | 80 | Deprecated because observation (MSB,object,filter) has been repeated later (shallow surveys only). The latest duplicate in each case is kept | 81 | Deprecated because observation (MSB,object,filter) has been repeated in a later Semester (shallow surveys only). The deepest duplicate in each case is kept | 99 | Manually deprecated because of some DFS issue (e.g. pipeline screw-up) | 100 | Multiframe deprecated because all detectors have been previously deprecated (and the MF not already deprecated) | 101 | MultiframeDetectors deprecated because parent Multiframe is deprecated (and the MFD not already deprecated) | 102 | *Detection deprecated because parent MFD deprecated | 103 | MultiframeDetector of a stack deprecated because all constituent frames of the same detector are deprecated | 110 | Intermediate stack frame photometry found to be poor wrt run of all stacks in a deep field | 111 | Stack replaced by a filtered version | 127 | Unwanted frame ingested. | ≥128 | Frame deprecated because reprocessing supercedes it | Note: for deprecation values of 128 or greater, the most significant bit of the byte has been set in order to preserve the deprecation value set by any previous quality control flagging run on the previous processed version. |
description |
CurationTask |
WSA |
description in words for this task |
varchar |
256 |
|
|
NOTE |
description |
CurationTask |
WSACalib |
description in words for this task |
varchar |
256 |
|
|
NOTE |
description |
CurationTask |
WSATransit |
description in words for this task |
varchar |
256 |
|
|
NOTE |
description |
ExternalSurvey |
WSA |
A brief description of the survey |
varchar |
256 |
|
|
NOTE |
description |
ExternalSurvey |
WSACalib |
A brief description of the survey |
varchar |
256 |
|
|
NOTE |
description |
ExternalSurvey |
WSATransit |
A brief description of the survey |
varchar |
256 |
|
|
NOTE |
description |
Filter |
WSA |
a concise description of the filter |
varchar |
256 |
|
|
NOTE |
description |
Filter |
WSACalib |
a concise description of the filter |
varchar |
256 |
|
|
NOTE |
description |
Filter |
WSATransit |
a concise description of the filter |
varchar |
256 |
|
|
NOTE |
description |
Programme |
WSA |
a concise description of the programme |
varchar |
256 |
|
|
NOTE |
description |
Programme |
WSACalib |
a concise description of the programme |
varchar |
256 |
|
|
NOTE |
description |
Programme |
WSATransit |
a concise description of the programme |
varchar |
256 |
|
|
NOTE |
description |
Release |
WSA |
a brief description of the release |
varchar |
256 |
|
|
NOTE |
description |
Release |
WSACalib |
a brief description of the release |
varchar |
256 |
|
|
NOTE |
description |
Release |
WSATransit |
a brief description of the release |
varchar |
256 |
|
|
NOTE |
description |
RequiredMosaic |
WSACalib |
Description of the product |
varchar |
256 |
|
|
?? |
description |
RequiredMosaic |
WSATransit |
Description of the product |
varchar |
256 |
|
|
?? |
description |
RequiredMosaic, RequiredStack |
WSA |
Description of the product |
varchar |
256 |
|
|
?? |
description |
Survey |
WSA |
A concise description of the survey |
varchar |
512 |
|
|
?? |
description |
Survey |
WSACalib |
A concise description of the survey |
varchar |
512 |
|
|
?? |
description |
Survey |
WSATransit |
A concise description of the survey |
varchar |
512 |
|
|
?? |
designation |
twomass_psc |
2MASS |
Sexagesimal, equatorial position-based source name in the form: hhmmssss+ddmmsss[ABC...]. |
varchar |
17 |
|
|
NAME |
designation |
twomass_xsc |
2MASS |
Source designation formed from sexigesimal coordinates. |
varchar |
17 |
|
|
NAME |
detCols |
MultiframeDetector |
WSA |
Number of detector columns {image extension keyword: DCOLUMNS} |
smallint |
2 |
pixels |
|
NUMBER |
detCols |
MultiframeDetector |
WSACalib |
Number of detector columns {image extension keyword: DCOLUMNS} |
smallint |
2 |
pixels |
|
NUMBER |
detCols |
MultiframeDetector |
WSATransit |
Number of detector columns {image extension keyword: DCOLUMNS} |
smallint |
2 |
pixels |
|
NUMBER |
detectionTable |
Programme |
WSA |
Table name of detections |
varchar |
64 |
|
|
?? |
detectionTable |
Programme |
WSACalib |
Table name of detections |
varchar |
64 |
|
|
?? |
detectionTable |
Programme |
WSATransit |
Table name of detections |
varchar |
64 |
|
|
?? |
detectorTemp |
MultiframeDetector |
WSA |
Detector array temperature {image extension keyword: DET_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
?? |
detectorTemp |
MultiframeDetector |
WSACalib |
Detector array temperature {image extension keyword: DET_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
?? |
detectorTemp |
MultiframeDetector |
WSATransit |
Detector array temperature {image extension keyword: DET_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
?? |
detectorType |
MultiframeDetector |
WSA |
Detector array used, eg. Aladdin {image extension keyword: DETECTOR} |
varchar |
16 |
|
NONE |
INST_ID |
detectorType |
MultiframeDetector |
WSACalib |
Detector array used, eg. Aladdin {image extension keyword: DETECTOR} |
varchar |
16 |
|
NONE |
INST_ID |
detectorType |
MultiframeDetector |
WSATransit |
Detector array used, eg. Aladdin {image extension keyword: DETECTOR} |
varchar |
16 |
|
NONE |
INST_ID |
detHeaterLevel |
Multiframe |
WSA |
Det heater level (in percent) {image primary HDU keyword: DET_HTP} |
real |
4 |
|
-0.9999995e9 |
|
detHeaterLevel |
Multiframe |
WSACalib |
Det heater level (in percent) {image primary HDU keyword: DET_HTP} |
real |
4 |
|
-0.9999995e9 |
|
detHeaterLevel |
Multiframe |
WSATransit |
Det heater level (in percent) {image primary HDU keyword: DET_HTP} |
real |
4 |
|
-0.9999995e9 |
|
DETID |
twoxmm |
XMM |
A consecutive number which identifies each entry (detection) in the catalogue. |
int |
4 |
|
|
|
detRows |
MultiframeDetector |
WSA |
Number of detector rows {image extension keyword: DROWS} |
smallint |
2 |
pixels |
|
NUMBER |
detRows |
MultiframeDetector |
WSACalib |
Number of detector rows {image extension keyword: DROWS} |
smallint |
2 |
pixels |
|
NUMBER |
detRows |
MultiframeDetector |
WSATransit |
Number of detector rows {image extension keyword: DROWS} |
smallint |
2 |
pixels |
|
NUMBER |
detTempAlt |
Multiframe |
WSA |
DET_TEMP alternate sensor {image primary HDU keyword: DETTEMPB} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
detTempAlt |
Multiframe |
WSACalib |
DET_TEMP alternate sensor {image primary HDU keyword: DETTEMPB} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
detTempAlt |
Multiframe |
WSATransit |
DET_TEMP alternate sensor {image primary HDU keyword: DETTEMPB} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
detTempSetPt |
Multiframe |
WSA |
Det temperature setpoint {image primary HDU keyword: DETTEMPS} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
detTempSetPt |
Multiframe |
WSACalib |
Det temperature setpoint {image primary HDU keyword: DETTEMPS} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
detTempSetPt |
Multiframe |
WSATransit |
Det temperature setpoint {image primary HDU keyword: DETTEMPS} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
deviceID |
MultiframeDetector |
WSA |
Device UID identifying every IR device {image extension keyword: DETECTID} |
varchar |
32 |
|
|
ID_PLATE |
deviceID |
MultiframeDetector |
WSACalib |
Device UID identifying every IR device {image extension keyword: DETECTID} |
varchar |
32 |
|
|
ID_PLATE |
deviceID |
MultiframeDetector |
WSATransit |
Device UID identifying every IR device {image extension keyword: DETECTID} |
varchar |
32 |
|
|
ID_PLATE |
dewPoint |
Multiframe |
WSA |
Dewpoint {image primary HDU keyword: DEWPOINT} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
dewPoint |
Multiframe |
WSACalib |
Dewpoint {image primary HDU keyword: DEWPOINT} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
dewPoint |
Multiframe |
WSATransit |
Dewpoint {image primary HDU keyword: DEWPOINT} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
dFlag |
rosat_bsc, rosat_fsc |
ROSAT |
complex diffuse emission pattern |
varchar |
1 |
|
|
CODE_MISC |
dfsIDString |
Programme |
WSA |
The description used within the data flow system (ie. the value of the appropriate FITS keyword) |
varchar |
64 |
|
|
?? |
dfsIDString |
Programme |
WSACalib |
The description used within the data flow system (ie. the value of the appropriate FITS keyword) |
varchar |
64 |
|
|
?? |
dfsIDString |
Programme |
WSATransit |
The description used within the data flow system (ie. the value of the appropriate FITS keyword) |
varchar |
64 |
|
|
?? |
dhsVersion |
Multiframe |
WSA |
Data handling version {image primary HDU keyword: DHSVER} |
varchar |
32 |
|
NONE |
|
dhsVersion |
Multiframe |
WSACalib |
Data handling version {image primary HDU keyword: DHSVER} |
varchar |
32 |
|
NONE |
|
dhsVersion |
Multiframe |
WSATransit |
Data handling version {image primary HDU keyword: DHSVER} |
varchar |
32 |
|
NONE |
|
disc_100 |
iras_psc |
IRAS |
Discrepant Fluxes flag (100 micron) |
tinyint |
1 |
|
|
REMARKS |
disc_12 |
iras_psc |
IRAS |
Discrepant Fluxes flag (12 micron) |
tinyint |
1 |
|
|
REMARKS |
disc_25 |
iras_psc |
IRAS |
Discrepant Fluxes flag (25 micron) |
tinyint |
1 |
|
|
REMARKS |
disc_60 |
iras_psc |
IRAS |
Discrepant Fluxes flag (60 micron) |
tinyint |
1 |
|
|
REMARKS |
DISK_I |
mgcGalaxyStruct |
MGC |
Disk Inclination (0=face-on) |
real |
4 |
|
99.99 |
|
DISK_Im |
mgcGalaxyStruct |
MGC |
Disk Inclination error (-) |
real |
4 |
|
99.99 |
|
DISK_Ip |
mgcGalaxyStruct |
MGC |
Disk Inclination error (+) |
real |
4 |
|
99.99 |
|
DISK_PA |
mgcGalaxyStruct |
MGC |
Disk Position Angle |
real |
4 |
|
99.99 |
|
DISK_PAm |
mgcGalaxyStruct |
MGC |
Disk Position Angle error (-) |
real |
4 |
|
99.99 |
|
DISK_PAp |
mgcGalaxyStruct |
MGC |
Disk Position Angle error (+) |
real |
4 |
|
99.99 |
|
dist_edge_ew |
twomass_psc |
2MASS |
The distance from the source to the nearest East or West scan edge. |
int |
4 |
arcsec |
|
INST_PLATE_DIST |
dist_edge_ew |
twomass_xsc |
2MASS |
The distance from the source to the nearest East or West scan edge. |
smallint |
2 |
arcsec |
|
INST_PLATE_DIST |
dist_edge_flg |
twomass_psc |
2MASS |
Two character flag that specifies to which scan edges a source lies closest, and to which edges the dist_edge_ns and dist_edge_ew values refer. |
varchar |
2 |
|
|
INST_PLATE_DIST |
dist_edge_flg |
twomass_xsc |
2MASS |
flag indicating which edges ([n|s][e|w]) are nearest to src. |
varchar |
2 |
|
|
INST_PLATE_DIST |
dist_edge_ns |
twomass_psc, twomass_xsc |
2MASS |
The distance from the source to the nearest North or South scan edge. |
int |
4 |
arcsec |
|
INST_PLATE_DIST |
DIST_NN |
twoxmm |
XMM |
The distance to the nearest detection. An internal threshold of 6 arseconds (before positional fitting) is used for splitting a source into two. |
real |
4 |
arcsec |
|
|
dist_opt |
twomass_psc |
2MASS |
Distance separating TWOMASS source position and associated optical source within 5". |
real |
4 |
arcsec |
|
INST_PLATE_DIST |
distanceMins |
calSourceNeighbours, calSourceXSynopticSource, calSourceXtwomass_psc, calSourceXukirtFSstars |
WSACalib |
Angular separation between neighbours |
real |
4 |
arcminutes |
|
POS_ANG_DIST_GENERAL |
distanceMins |
dxsSourceNeighbours, dxsSourceXDR7PhotoObj, dxsSourceXDetection, dxsSourceXStripe82PhotoObjAll, dxsSourceXtwomass_psc, dxsSourceXtwoxmm, gcsSourceNeighbours, gcsSourceXDR5PhotoObj, gcsSourceXDR7PhotoObj, gcsSourceXtwomass_psc, gcsSourceXtwoxmm, gpsSourceNeighbours, gpsSourceXglimpse1_hrc, gpsSourceXglimpse1_mca, gpsSourceXglimpse2_hrc, gpsSourceXglimpse2_mca, gpsSourceXglimpse_hrc_inter, gpsSourceXglimpse_mca_inter, gpsSourceXtwomass_psc, gpsSourceXtwoxmm, lasSourceNeighbours, lasSourceXDR2PhotoObj, lasSourceXDR3PhotoObj, lasSourceXDR5PhotoObj, lasSourceXDR5PhotoObjAll, lasSourceXDR7PhotoObj, lasSourceXDR7PhotoObjAll, lasSourceXSegueDR6PhotoObj, lasSourceXSegueDR6PhotoObjAll, lasSourceXStripe82PhotoObjAll, lasSourceXfirstSource, lasSourceXiras_psc, lasSourceXmgcDetection, lasSourceXnvssSource, lasSourceXrosat_bsc, lasSourceXrosat_fsc, lasSourceXtwomass_psc, lasSourceXtwomass_xsc, lasSourceXtwoxmm |
WSA |
Angular separation between neighbours |
real |
4 |
arcminutes |
|
POS_ANG_DIST_GENERAL |
distortMap |
CurrentAstrometry |
WSACalib |
filename of 2d non-linear distortion map |
varchar |
256 |
|
NONE |
ID_FILE |
distortMap |
CurrentAstrometry |
WSATransit |
filename of 2d non-linear distortion map |
varchar |
256 |
|
NONE |
ID_FILE |
distortMap |
CurrentAstrometry, PreviousAstrometry |
WSA |
filename of 2d non-linear distortion map |
varchar |
256 |
|
NONE |
ID_FILE |
ditherOffsetX |
MultiframeDetector |
WSA |
Dither offset X {image extension keyword: CIR_XOFF} |
real |
4 |
|
-0.9999995e9 |
POS_OFFSET |
ditherOffsetX |
MultiframeDetector |
WSACalib |
Dither offset X {image extension keyword: CIR_XOFF} |
real |
4 |
|
-0.9999995e9 |
POS_OFFSET |
ditherOffsetX |
MultiframeDetector |
WSATransit |
Dither offset X {image extension keyword: CIR_XOFF} |
real |
4 |
|
-0.9999995e9 |
POS_OFFSET |
ditherOffsetY |
MultiframeDetector |
WSA |
Dither offset Y {image extension keyword: CIR_YOFF} |
real |
4 |
|
-0.9999995e9 |
POS_OFFSET |
ditherOffsetY |
MultiframeDetector |
WSACalib |
Dither offset Y {image extension keyword: CIR_YOFF} |
real |
4 |
|
-0.9999995e9 |
POS_OFFSET |
ditherOffsetY |
MultiframeDetector |
WSATransit |
Dither offset Y {image extension keyword: CIR_YOFF} |
real |
4 |
|
-0.9999995e9 |
POS_OFFSET |
domeTemp |
Multiframe |
WSA |
Dome temperature {image primary HDU keyword: DOMETEMP} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
domeTemp |
Multiframe |
WSACalib |
Dome temperature {image primary HDU keyword: DOMETEMP} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
domeTemp |
Multiframe |
WSATransit |
Dome temperature {image primary HDU keyword: DOMETEMP} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
dualFilterID |
RequiredMosaic |
WSACalib |
SEX extraction tool option to run in dual image mode UID of dual image filter (assigned in WSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
0 |
INST_FILTER_CODE |
dualFilterID |
RequiredMosaic |
WSATransit |
SEX extraction tool option to run in dual image mode UID of dual image filter (assigned in WSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
0 |
INST_FILTER_CODE |
dualFilterID |
RequiredMosaic, RequiredStack |
WSA |
SEX extraction tool option to run in dual image mode UID of dual image filter (assigned in WSA: 1=Z,2=Y,3=J,4=H,5=K,6=H2,7=Br,8=blank) |
tinyint |
1 |
|
0 |
INST_FILTER_CODE |
dum |
rosat_bsc, rosat_fsc |
ROSAT |
dummy flag |
varchar |
1 |
|
|
CODE_MISC |
dup_src |
twomass_psc, twomass_xsc |
2MASS |
Duplicate source flag. |
smallint |
2 |
|
|
CODE_MISC |