D |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
darkID |
[nspid]Multiframe |
WSA NonSurvey |
UID of library calibration dark frame {image extension keyword: DARKCOR} |
bigint |
8 |
|
-99999999 |
obs.field |
databaseName |
[nspid]ExternalSurvey |
WSA NonSurvey |
The name of the database within the WSA |
varchar |
16 |
|
|
meta.id;meta.dataset |
dataScale |
[nspid]MultiframeDetector |
WSA NonSurvey |
Scaling of pixel values {image extension keyword: BSCALE} |
real |
4 |
|
1.0 |
?? |
dataZero |
[nspid]MultiframeDetector |
WSA NonSurvey |
Zeropoint of pixel values {image extension keyword: BZERO} |
real |
4 |
|
0.0 |
?? |
dateEnd |
[nspid]Multiframe |
WSA NonSurvey |
Date and time (UTC) of end of the observation {image primary HDU keyword: DATE-END} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
dateObs |
[nspid]Multiframe |
WSA NonSurvey |
Date and time (UTC) of start of the observation {image primary HDU keyword: DATE-OBS} |
datetime |
8 |
|
12-31-9999 |
time.epoch |
The date and time is written in the specific SQL Server datetime format: YYYY-MM-DD HH:MM:SS.s |
dbName |
[nspid]Release |
WSA NonSurvey |
the name of the SQL Server database containing this release |
varchar |
128 |
|
|
?? |
dbNamePrefix |
[nspid]Survey |
WSA NonSurvey |
A string that prefixes all database names released for this survey |
varchar |
32 |
|
|
?? |
deblend |
[nspid]Detection |
WSA NonSurvey |
Not available in SE output {catalogue TType keyword: Parent_or_child} |
int |
4 |
|
-99999999 |
|
deblend |
[nspid]Detection |
WSA NonSurvey |
Placeholder flag for parent or part of deblended deconstruct (redundant since only deblended images are kept) {catalogue TType keyword: Parent_or_child} |
int |
4 |
|
-99999999 |
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 |
[nspid]UKIDSSDetection |
WSA NonSurvey |
Placeholder flag for parent or part of deblended deconstruct (redundant since only deblended images are kept) |
int |
4 |
|
-99999999 |
CODE_MISC |
dec |
[nspid]Detection, [nspid]Source, [nspid]SynopticSource |
WSA NonSurvey |
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 |
[nspid]DxsSource, [nspid]ExtendedSource, [nspid]GcsPointSource, [nspid]GpsPointSource, [nspid]JHKsource, [nspid]JKsource, [nspid]LasPointSource, [nspid]PointSource, [nspid]SatelliteDetection, [nspid]UKIDSSDetection, [nspid]UdsSource, [nspid]YJHKsource, [nspid]ZYJHKsource |
WSA NonSurvey |
Celestial Declination |
float |
8 |
Degrees |
|
POS_EQ_DEC_MAIN |
dec |
[nspid]FSstars |
WSA NonSurvey |
Declination of star at Equinox J2000.0 |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
[nspid]JHKmergeLog, [nspid]JKmergeLog, [nspid]MergeLog, [nspid]SynopticMergeLog, [nspid]YJHKmergeLog, [nspid]ZYJHKmergeLog |
WSA NonSurvey |
Declination of field centre |
float |
8 |
degrees |
|
POS_EQ_DEC_MAIN |
dec |
[nspid]MapApertureIDshighzQsoMap |
WSA NonSurvey |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
[nspid]MapRemeasAver |
WSA NonSurvey |
Averaged Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
[nspid]MapRemeasurement |
WSA NonSurvey |
Celestial Declination |
float |
8 |
Degrees |
|
pos.eq.dec;meta.main |
Celestial Declination as computed in the processing pipeline, accurate to of order 0.1 arcsec. Note that original catalogue data has only r*4 storage precision, accurate only to ≈ 50mas. RA and Dec in the database are derived more precisely from WCS in the header and x and y attributes. |
dec |
[nspid]Orphan |
WSA NonSurvey |
Celestial Declination |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
dec |
[nspid]QsoCatalogue |
WSA NonSurvey |
J2000 declination with respect to the ICRS {catalogue TType keyword: dec} |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
[nspid]RequiredMosaic, [nspid]RequiredRegion |
WSA NonSurvey |
Declination of mosaic centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
[nspid]RequiredStack |
WSA NonSurvey |
Declination of stack centre |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
dec |
[nspid]Variability |
WSA NonSurvey |
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_WISE |
[nspid]QsoCatalogue |
WSA NonSurvey |
WISE J2000 declination {catalogue TType keyword: dec_WISE} |
float |
8 |
degrees |
|
pos.eq.ra |
decBase |
[nspid]Multiframe |
WSA NonSurvey |
Declination of base position {image primary HDU keyword: DECBASE} |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decCentre |
[nspid]StdFieldInfo |
WSA NonSurvey |
Declination of field centre |
float |
8 |
degrees |
|
pos.eq.ra;meta.main |
decErr |
[nspid]MapRemeasAver |
WSA NonSurvey |
Error in averaged Celestial Declination |
float |
8 |
pixels |
|
|
decExtent |
[nspid]RequiredMosaic, [nspid]RequiredRegion |
WSA NonSurvey |
The angular extent in Dec of the mosaic image |
real |
4 |
degrees |
|
?? |
decMoon |
[nspid]Multiframe |
WSA NonSurvey |
Geocentric J2000 FK5 Mean Declination of the Moon |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decMoonTopo |
[nspid]Multiframe |
WSA NonSurvey |
Apparent topocentric Declination of the Moon (including precession, nutation, and annual aberration) |
float |
8 |
degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
decStr |
[nspid]QsoCatalogue |
WSA NonSurvey |
J2000 declination with respect to the ICRS {catalogue TType keyword: dec_dms} |
varchar |
16 |
|
|
pos.eq.dec |
decTelOff |
[nspid]Multiframe |
WSA NonSurvey |
Declination telescope offset {image primary HDU keyword: TDECOFF} |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff |
decurtainRange |
[nspid]MultiframeDetector |
WSA NonSurvey |
Range of decurtain correction {image extension keyword: CURTNRNG} |
real |
4 |
|
-0.9999995e9 |
?? |
decurtFlag |
[nspid]MultiframeDetector |
WSA NonSurvey |
De-curtaining flag {image extension keyword: DECURTN} |
varchar |
32 |
|
NONE |
?? |
delPropData |
[nspid]SurveyProgrammes |
WSA NonSurvey |
Logical flag indicating that proprietary data should be removed on release (1=yes; 0=no) |
tinyint |
1 |
|
|
?? |
deltaMag |
[nspid]MapRemeasurement |
WSA NonSurvey |
sum of magnitude corrections for faster processing |
real |
4 |
|
0.0 |
stat.param |
deprecated |
[nspid]Detection, [nspid]SatelliteDetection |
WSA NonSurvey |
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 |
[nspid]JHKmergeLog, [nspid]JKmergeLog, [nspid]MergeLog, [nspid]SynopticMergeLog, [nspid]YJHKmergeLog, [nspid]ZYJHKmergeLog |
WSA NonSurvey |
frame set deprecation flag (1=deprecated) |
tinyint |
1 |
|
|
CODE_MISC |
deprecated |
[nspid]MapFrameStatus |
WSA NonSurvey |
Code for a current (=0) or deprecated (!=0) |
tinyint |
1 |
|
0 |
CODE_MISC |
deprecated |
[nspid]MapRemeasAver, [nspid]MapRemeasurement |
WSA NonSurvey |
Code for a current (=0) or deprecated (!=0) detection |
tinyint |
1 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete 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 |
[nspid]Multiframe |
WSA NonSurvey |
Code for a current (=0) or deprecated (!=0) multiframe |
tinyint |
1 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete 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 |
[nspid]MultiframeDetector |
WSA NonSurvey |
Code for a current (=0) or deprecated (!=0) multiframe detector |
tinyint |
1 |
|
0 |
meta.code |
The deprecation attribute in all tables indicates if the record in question (be it an image or catalogue detection record) has been deprecated by some curation process in the archive. All data having deprecated=0 are nominally good data; the following flags indicate a quality issue and any data having those flags should not be used for scientific purposes (in many instances, deprecated data will be deleted from public survey released database products): Flag | Meaning | 1 | Stack frames that have no catalogue or other frameTypes deprecated at ingest (e.g. because a reprocessed frame supercedes it) | 2 | Dead detector frames | 3 | Undefined and or non-sensible critical image metadata attributes | 4 | Sky subtraction not OK (via pipeline sky sub scale factor) NB. not used from October 2005 onwards | 5 | Incorrect combination of expTime,numExp,numInts for survey specific projects | 6 | Incorrect frame complements within groups/nights (for incomplete 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 |
[nspid]UKIDSSDetection |
WSA NonSurvey |
Code for a current (=0) or deprecated (!=0) detection |
tinyint |
1 |
|
0 |
CODE_MISC |
description |
[nspid]CurationTask |
WSA NonSurvey |
description in words for this task |
varchar |
256 |
|
|
meta.note |
description |
[nspid]ExternalProduct |
WSA NonSurvey |
Description of the product set |
varchar |
256 |
|
|
?? |
description |
[nspid]ExternalSurvey |
WSA NonSurvey |
A brief description of the survey |
varchar |
256 |
|
|
meta.note |
description |
[nspid]Filter |
WSA NonSurvey |
a concise description of the filter |
varchar |
256 |
|
|
meta.note |
description |
[nspid]Programme |
WSA NonSurvey |
a concise description of the programme |
varchar |
256 |
|
|
meta.note |
description |
[nspid]Release |
WSA NonSurvey |
a brief description of the release |
varchar |
256 |
|
|
meta.note |
description |
[nspid]RequiredMapAverages |
WSA NonSurvey |
Description of type of averaging required |
varchar |
64 |
|
NONE |
|
description |
[nspid]RequiredMatchedApertureProduct |
WSA NonSurvey |
description of the matched aperture product |
varchar |
256 |
|
|
?? |
description |
[nspid]RequiredMergeLogMultiEpoch, [nspid]RequiredMosaic, [nspid]RequiredStack |
WSA NonSurvey |
Description of the product |
varchar |
256 |
|
|
?? |
description |
[nspid]RequiredMosaicTopLevel |
WSA NonSurvey |
Description of the set of mosaics |
varchar |
256 |
|
|
?? |
description |
[nspid]Survey |
WSA NonSurvey |
A concise description of the survey |
varchar |
512 |
|
|
?? |
desig |
[nspid]QsoCatalogue |
WSA NonSurvey |
Designation {catalogue TType keyword: desig} |
varchar |
32 |
|
|
meta.id |
detCols |
[nspid]MultiframeDetector |
WSA NonSurvey |
Number of detector columns {image extension keyword: DCOLUMNS} |
smallint |
2 |
pixels |
|
meta.number |
detectionTable |
[nspid]Programme |
WSA NonSurvey |
Table name of detections |
varchar |
64 |
|
|
?? |
detectorTemp |
[nspid]MultiframeDetector |
WSA NonSurvey |
Detector array temperature {image extension keyword: DET_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
?? |
detectorType |
[nspid]MultiframeDetector |
WSA NonSurvey |
Detector array used, eg. Aladdin {image extension keyword: DETECTOR} |
varchar |
16 |
|
NONE |
meta.id;instr |
detedgeinnerpos1Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DETEDGEINNERPOS1 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos1NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DETEDGEINNERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos1NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DETEDGEINNERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos1NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DETEDGEINNERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos2Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DETEDGEINNERPOS2 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos2NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DETEDGEINNERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos2NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DETEDGEINNERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos2NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DETEDGEINNERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos3Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DETEDGEINNERPOS3 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos3NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DETEDGEINNERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos3NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DETEDGEINNERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos3NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DETEDGEINNERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos4Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DETEDGEINNERPOS4 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos4NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DETEDGEINNERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos4NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DETEDGEINNERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeinnerpos4NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DETEDGEINNERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos1Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DETEDGEOUTERPOS1 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos1NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DETEDGEOUTERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos1NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DETEDGEOUTERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos1NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DETEDGEOUTERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos2Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DETEDGEOUTERPOS2 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos2NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DETEDGEOUTERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos2NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DETEDGEOUTERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos2NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DETEDGEOUTERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos3Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DETEDGEOUTERPOS3 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos3NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DETEDGEOUTERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos3NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DETEDGEOUTERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos3NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DETEDGEOUTERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos4Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DETEDGEOUTERPOS4 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos4NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DETEDGEOUTERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos4NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DETEDGEOUTERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detedgeouterpos4NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DETEDGEOUTERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
detHeaterLevel |
[nspid]Multiframe |
WSA NonSurvey |
Det heater level (in percent) {image primary HDU keyword: DET_HTP} |
real |
4 |
|
-0.9999995e9 |
|
detRows |
[nspid]MultiframeDetector |
WSA NonSurvey |
Number of detector rows {image extension keyword: DROWS} |
smallint |
2 |
pixels |
|
meta.number |
detTempAlt |
[nspid]Multiframe |
WSA NonSurvey |
DET_TEMP alternate sensor {image primary HDU keyword: DETTEMPB} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
detTempSetPt |
[nspid]Multiframe |
WSA NonSurvey |
Det temperature setpoint {image primary HDU keyword: DETTEMPS} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
deviceID |
[nspid]MultiframeDetector |
WSA NonSurvey |
Device UID identifying every IR device {image extension keyword: DETECTID} |
varchar |
32 |
|
|
obs.field |
dewPoint |
[nspid]Multiframe |
WSA NonSurvey |
Dewpoint {image primary HDU keyword: DEWPOINT} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
phys.temperature |
dfsIDString |
[nspid]Programme |
WSA NonSurvey |
The description used within the data flow system (ie. the value of the appropriate FITS keyword) |
varchar |
64 |
|
|
?? |
dhsVersion |
[nspid]Multiframe |
WSA NonSurvey |
Data handling version {image primary HDU keyword: DHSVER} |
varchar |
32 |
|
NONE |
|
directory |
[nspid]ExternalProduct |
WSA NonSurvey |
Name of directory which these data reside in |
varchar |
32 |
|
|
|
distanceMins |
[nspid]SourceNeighbours, [nspid]SourceXDR2PhotoObj, [nspid]SourceXDR3PhotoObj, [nspid]SourceXDR5PhotoObj, [nspid]SourceXDR5PhotoObjAll, [nspid]SourceXDR7PhotoObj, [nspid]SourceXDR7PhotoObjAll, [nspid]SourceXDR9PhotoObj, [nspid]SourceXDR9PhotoObjAll, [nspid]SourceXDetection, [nspid]SourceXDr13PhotoObj, [nspid]SourceXDr9PhotoObj, [nspid]SourceXGR6PhotoObjAll, [nspid]SourceXSSASource, [nspid]SourceXStripe82PhotoObjAll, [nspid]SourceXSynopticSource, [nspid]SourceXallwise_sc, [nspid]SourceXfirstSource, [nspid]SourceXglimpse1_hrc, [nspid]SourceXglimpse1_mca, [nspid]SourceXglimpse2_hrc, [nspid]SourceXglimpse2_mca, [nspid]SourceXglimpse_hrc_inter, [nspid]SourceXglimpse_mca_inter, [nspid]SourceXiras_psc, [nspid]SourceXmgcDetection, [nspid]SourceXnvssSource, [nspid]SourceXrosat_bsc, [nspid]SourceXrosat_fsc, [nspid]SourceXtwomass_psc, [nspid]SourceXtwomass_xsc, [nspid]SourceXtwompzPhotoz, [nspid]SourceXtwoxmm, [nspid]SourceXukirtFSstars, [nspid]SourceXwiseScosPhotoz, [nspid]SourceXwise_allskysc |
WSA NonSurvey |
Angular separation between neighbours |
real |
4 |
arcminutes |
|
POS_ANG_DIST_GENERAL |
distortCorr |
[nspid]MapRemeasurement |
WSA NonSurvey |
distortion correction |
real |
4 |
|
0.0 |
stat.fit.param |
distortMap |
[nspid]CurrentAstrometry, [nspid]PreviousAstrometry |
WSA NonSurvey |
filename of 2d non-linear distortion map |
varchar |
256 |
|
NONE |
meta.id;meta.file |
dithedgeinnerpos1Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DITHEDGEINNERPOS1 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos1NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DITHEDGEINNERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos1NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DITHEDGEINNERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos1NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DITHEDGEINNERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos2Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DITHEDGEINNERPOS2 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos2NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DITHEDGEINNERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos2NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DITHEDGEINNERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos2NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DITHEDGEINNERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos3Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DITHEDGEINNERPOS3 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos3NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DITHEDGEINNERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos3NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DITHEDGEINNERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos3NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DITHEDGEINNERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos4Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DITHEDGEINNERPOS4 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos4NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DITHEDGEINNERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos4NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DITHEDGEINNERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeinnerpos4NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DITHEDGEINNERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos1Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DITHEDGEOUTERPOS1 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos1NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DITHEDGEOUTERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos1NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DITHEDGEOUTERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos1NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DITHEDGEOUTERPOS1 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos2Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DITHEDGEOUTERPOS2 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos2NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DITHEDGEOUTERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos2NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DITHEDGEOUTERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos2NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DITHEDGEOUTERPOS2 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos3Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DITHEDGEOUTERPOS3 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos3NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DITHEDGEOUTERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos3NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DITHEDGEOUTERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos3NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DITHEDGEOUTERPOS3 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos4Const |
[nspid]AstrometricInfo |
WSA NonSurvey |
Offset of halfspace along the unit normal vector describing the DITHEDGEOUTERPOS4 detector boundary. If the detector boundary is straight, with no distortion this is zero. |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos4NormX |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector X-coordinate of the halfspace describing the DITHEDGEOUTERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos4NormY |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Y-coordinate of the halfspace describing the DITHEDGEOUTERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
dithedgeouterpos4NormZ |
[nspid]AstrometricInfo |
WSA NonSurvey |
Cartesian unit normal vector Z-coordinate of the halfspace describing the DITHEDGEOUTERPOS4 detector boundary (see Budavari et al. 2010,) |
float |
8 |
|
-0.9999995e9 |
?? |
ditherOffsetX |
[nspid]MultiframeDetector |
WSA NonSurvey |
Dither offset X {image extension keyword: CIR_XOFF} |
real |
4 |
|
-0.9999995e9 |
pos;arith.diff |
ditherOffsetY |
[nspid]MultiframeDetector |
WSA NonSurvey |
Dither offset Y {image extension keyword: CIR_YOFF} |
real |
4 |
|
-0.9999995e9 |
pos;arith.diff |
domeTemp |
[nspid]Multiframe |
WSA NonSurvey |
Dome temperature {image primary HDU keyword: DOMETEMP} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
phys.temperature |
doNotUseOBinfo |
[nspid]Programme |
WSA NonSurvey |
Don't use OB info in multi-epoch frame assignment. |
tinyint |
1 |
|
0 |
|
dragTerm |
[nspid]SatelliteOrbits |
WSA NonSurvey |
BSTAR drag term |
float |
8 |
|
|
|
dualFilterID |
[nspid]RequiredMosaic |
WSA NonSurvey |
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 |
meta.code;instr.filter |