F |
|---|
| Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
|---|
| faintLim |
Plate |
SSA |
Faint limit for selected refstars |
real |
4 |
|
|
PHOT_MAG_LIMIT |
| fastGuiderMode |
Multiframe |
WSA |
Fast guider mode {image primary HDU keyword: FGMODE} |
varchar |
32 |
|
NONE |
|
| fCor_100 |
iras_psc |
IRAS |
Flux correction factor applied (times 1000, 100 micron) |
smallint |
2 |
|
|
INST_CORR-FACTOR |
| fCor_12 |
iras_psc |
IRAS |
Flux correction factor applied (times 1000, 12 micron) |
smallint |
2 |
|
|
INST_CORR-FACTOR |
| fCor_25 |
iras_psc |
IRAS |
Flux correction factor applied (times 1000, 25 micron) |
smallint |
2 |
|
|
INST_CORR-FACTOR |
| fCor_60 |
iras_psc |
IRAS |
Flux correction factor applied (times 1000, 60 micron) |
smallint |
2 |
|
|
INST_CORR-FACTOR |
| ffZp |
Plate |
SSA |
Field-to-field zeropoint |
real |
4 |
mag |
|
PHOT_ZPT |
| fg_flg |
twomass_xsc |
2MASS |
flux-growth convergence flag. |
varchar |
6 |
|
|
CODE_MISC |
| field1 |
iras_asc |
IRAS |
object field #1 (magnitude/other) |
smallint |
2 |
|
|
ID_FIELD |
| field2 |
iras_asc |
IRAS |
object field #2 (magnitude/other) |
smallint |
2 |
|
|
ID_FIELD |
| field3 |
iras_asc |
IRAS |
object field #3 (size/other) |
smallint |
2 |
|
|
ID_FIELD |
| fieldID |
CurrentStdStarInfo, calMultiEpochLog, PreviousStdStarInfo, StdFieldInfo |
WSA |
field ID, |
int |
4 |
|
|
ID_FIELD |
| fieldID |
Field |
SSA |
Unique identifier of survey field (fieldNum and systemID combo) |
int |
4 |
|
|
ID_FIELD |
| fieldID |
Plate |
SSA |
Unique survey field identifier |
int |
4 |
|
|
ID_FIELD |
| fieldID |
rosat_bsc, rosat_fsc |
ROSAT |
identification number of SASS field |
varchar |
8 |
|
|
ID_FIELD |
| fieldName |
CurrentStdStarInfo, PreviousStdStarInfo, StdFieldInfo |
WSA |
reference name of field |
varchar |
16 |
|
NONE |
???? |
| fieldName |
firstSource |
FIRST |
Name of the coadded image containing the source (encodes the position of the field center). |
varchar |
12 |
|
|
ID_IMAGE |
| fieldNum |
Field |
SSA |
ESO/SRC or Palomar survey system field number |
smallint |
2 |
|
|
ID_FIELD |
| fieldOfView |
Survey |
SSA |
The nominal field of view of each survey plate |
real |
4 |
degrees |
|
INST_DET_SIZE |
| fileName |
Multiframe |
WSA |
the filename for the multiframe, eg. server:/path/filename.fit |
varchar |
256 |
|
|
ID_FILE |
| fileTimeStamp |
Multiframe |
WSA |
Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness |
bigint |
8 |
|
|
?? |
| filter1 |
RequiredDiffImage |
WSA |
UID of WFCAM narrow band (primary) filter |
tinyint |
1 |
|
|
INST_FILTER_CODE |
| filter2 |
RequiredDiffImage |
WSA |
UID of WFCAM broad band (reference) filter to be subtracted |
tinyint |
1 |
|
|
INST_FILTER_CODE |
| filterComm |
Plate |
SSA |
Filter type, eg. "Schott glass", "Red plexiglass"... |
varchar |
16 |
|
|
INST_FILTER_CODE |
| filterID |
CurrentNightlyExt |
WSA |
the internal WSA filter UID {image primary HDU keyword: FILTER} |
tinyint |
1 |
|
|
INST_FILTER_CODE |
| filterID |
CurrentZP, DetectorSetUp, MultiframeSetUp, PreviousNightlyExt, PreviousZP |
WSA |
the internal WSA filter UID |
tinyint |
1 |
|
|
INST_FILTER_CODE |
| filterID |
Filter |
WSA |
UID of filter, defined as above |
tinyint |
1 |
|
|
INST_FILTER_CODE |
| filterID |
calDetection, commDetection, dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, Multiframe, udsDetection, udsListRemeasurement |
WSA |
UID of combined filter (assigned in WSA) |
tinyint |
1 |
|
|
INST_FILTER_CODE |
| filterID |
MultiframeDetector |
WSA |
UID of combined filter (assigned in WSA) over the lifetime of WFCAM {image primary HDU keyword: FILTER} |
tinyint |
1 |
|
|
INST_FILTER_CODE |
| filterID |
Plate |
SSA |
Filter identifier, eg. OG590, RG715, 2444... |
varchar |
8 |
|
|
INST_FILTER_CODE |
| filterID |
RequiredFilters |
WSA |
the unique filter ID number |
tinyint |
1 |
|
|
INST_FILTER_CODE |
| filterID |
RequiredMosaic, RequiredStack |
WSA |
UID of WFCAM filter |
tinyint |
1 |
|
|
INST_FILTER_CODE |
| filterName |
Multiframe |
WSA |
WFCAM combined filter name {image primary HDU keyword: FILTER} |
varchar |
8 |
|
|
?? |
| finalTask |
RequiredCurationTask |
WSA |
is this task the final one before release (0=no; 1=yes)? |
tinyint |
1 |
|
|
?? |
| fInt |
firstSource |
FIRST |
integrated flux densities |
real |
4 |
mJy |
|
PHOT_FLUX_RADIO_1.4G |
| flatID |
Multiframe |
WSA |
UID of library calibration flatfield frame {image extension keyword: FLATCOR} |
bigint |
8 |
|
-99999999 |
ID_FRAME |
| flux_100 |
iras_psc |
IRAS |
Averaged non-color corrected 100 micron flux density |
real |
4 |
Jansky (1.0E-26 W/m**2/Hz) |
|
PHOT_FLUX_IR_100 |
| flux_12 |
iras_psc |
IRAS |
Averaged non-color corrected 12 micron flux density |
real |
4 |
Jansky (1.0E-26 W/m**2/Hz) |
|
PHOT_FLUX_IR_12 |
| flux_25 |
iras_psc |
IRAS |
Averaged non-color corrected 25 micron flux density |
real |
4 |
Jansky (1.0E-26 W/m**2/Hz) |
|
PHOT_FLUX_IR_25 |
| flux_60 |
iras_psc |
IRAS |
Averaged non-color corrected 60 micron flux density |
real |
4 |
Jansky (1.0E-26 W/m**2/Hz) |
|
PHOT_FLUX_IR_60 |
| fMaj |
firstSource |
FIRST |
major axes derived from the elliptical Gaussian model for the source before deconvolution. |
real |
4 |
arcsec |
|
EXTENSION_FWHM_MAJ |
| fMin |
firstSource |
FIRST |
minor axes derived from the elliptical Gaussian model for the source before deconvolution. |
real |
4 |
arcsec |
|
EXTENSION_FWHM_MIN |
| focus |
twomass_scn |
2MASS |
Focus setting of telescope at beginning of scan. |
smallint |
2 |
|
|
TEL_FOCAL-LENGTH |
| focusFiltOff |
Multiframe |
WSA |
Focus filter offset {image primary HDU keyword: FOC_FOFF} |
real |
4 |
millimetres |
-0.9999995e9 |
INST_PARAM |
| focusInstFiltOff |
Multiframe |
WSA |
focus offset for inst. filter {image primary HDU keyword: TEL_FOFF} |
real |
4 |
millimetres |
-0.9999995e9 |
INST_PARAM |
| focusNominOff |
Multiframe |
WSA |
Offset from nominal focus position {image primary HDU keyword: FOC_OFF} |
real |
4 |
millimetres |
-0.9999995e9 |
INST_PARAM |
| focusNX |
Plate |
SSA |
No. of scan focus points in X |
tinyint |
1 |
|
|
INST_PARAM |
| focusNY |
Plate |
SSA |
No. of scan focus points in Y |
tinyint |
1 |
|
|
INST_PARAM |
| focusOffset |
Multiframe |
WSA |
Focus offset {image primary HDU keyword: FOC_OFFS} |
real |
4 |
millimetres |
-0.9999995e9 |
INST_PARAM |
| focusPos |
Multiframe |
WSA |
Focus position {image primary HDU keyword: FOC_POSN} |
real |
4 |
millimetres |
-0.9999995e9 |
INST_PARAM |
| focusSerial |
Multiframe |
WSA |
Serial number in focus scan {image primary HDU keyword: FOC_I} |
int |
4 |
|
-99999999 |
?? |
| focusZero |
Multiframe |
WSA |
Focus zero-point position {image primary HDU keyword: FOC_ZERO} |
real |
4 |
millimetres |
-0.9999995e9 |
INST_PARAM |
| fPA |
firstSource |
FIRST |
position angle (east of north) derived from the elliptical Gaussian model for the source before deconvolution. |
real |
4 |
degrees |
|
POS_POS-ANG |
| fPeak |
firstSource |
FIRST |
peak flux densities |
real |
4 |
mJy |
|
PHOT_FLUX_RADIO_1.4G |
| fQual_100 |
iras_psc |
IRAS |
100 micron flux density quality. |
smallint |
2 |
|
|
CODE_QUALITY |
| fQual_12 |
iras_psc |
IRAS |
12 micron flux density quality. |
smallint |
2 |
|
|
CODE_QUALITY |
| fQual_25 |
iras_psc |
IRAS |
25 micron flux density quality. |
smallint |
2 |
|
|
CODE_QUALITY |
| fQual_60 |
iras_psc |
IRAS |
60 micron flux density quality. |
smallint |
2 |
|
|
CODE_QUALITY |
| frameSetID |
calMergeLogEpochs, calMultiEpochLog, commMergeLog, dxsMergeLog, gcsMergeLog, gpsMergeLog, lasMergeLog, udsMergeLog |
WSA |
frame set ID, unique over the whole WSA via programme ID prefix, assigned by merging procedure |
bigint |
8 |
|
|
ID_FIELD |
| Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, lasSource.frameSetID references lasMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
| frameSetID |
calSourceEpochs, commSource, dxsSource, gcsSource, gpsSource, lasSource, udsSource |
WSA |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
REFER_CODE |
| Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, lasSource.frameSetID references lasMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived. |
| frameSetID |
dxsSourceRemeasurement, gcsSourceRemeasurement, gpsSourceRemeasurement, lasSourceRemeasurement, udsSourceRemeasurement |
WSA |
UID of the set of frames that this merged source comes from |
bigint |
8 |
|
|
REFER_CODE |
| frameSetTolerance |
Programme |
WSA |
The match tolerance for different passband frames |
real |
4 |
Degrees |
|
?? |
| frameTable |
Programme |
WSA |
Name of table containing frame metadata |
varchar |
64 |
|
|
?? |
| frameType |
Multiframe |
WSA |
The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc).
A multiframe can have a combination of different types. |
varchar |
64 |
|
normal |
meta.code.class |
The frame types and their abbreviations are:
| arc = "arc" | bias = "bias" | calibration = "cali" | catalogue = "cat" | confidence = "conf" | | dark = "dark" | difference = "diff" | flat = "flat" | interleaved = "leav" | mosaic = "mosaic" | | sky = "sky" | stack = "stack" | tile = "tile" | default value = "normal" | |
| frinID |
Multiframe |
WSA |
UID of library calibration fringe frame |
bigint |
8 |
|
-99999999 |
ID_FRAME |
| fSclen |
Plate |
SSA |
Scale size for iterative filter application |
tinyint |
1 |
|
|
REDUCT_PARAM |
| fsTemp |
Multiframe |
WSA |
CCC 1st stage temperature {image primary HDU keyword: FS_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
| fThresh |
Plate |
SSA |
Sky filtering parameter |
tinyint |
1 |
|
|
REDUCT_PARAM |
