C |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
C1 |
mgcGalaxyStruct |
MGC |
Concentration index alpha=1 |
real |
4 |
|
99.99 |
|
C2 |
mgcGalaxyStruct |
MGC |
Concentration index alpha=2 |
real |
4 |
|
99.99 |
|
C3 |
mgcGalaxyStruct |
MGC |
Concentration index alpha=3 |
real |
4 |
|
99.99 |
|
C4 |
mgcGalaxyStruct |
MGC |
Concentration index alpha=4 |
real |
4 |
|
99.99 |
|
c_strat |
twomass_scn |
2MASS |
Flag indicating the calibration strategy for this night's data. |
smallint |
2 |
|
|
CODE_MISC |
c_strat |
twomass_sixx2_scn |
2MASS |
calibration strategy, north only (0=old, 1=new) |
smallint |
2 |
|
|
|
camNum |
MultiframeDetector |
WSA |
Number of WFCAM camera (1, 2, 3 or 4) {image extension keyword: CAMNUM} |
int |
4 |
|
|
obs.field |
camNum |
MultiframeDetector |
WSACalib |
Number of WFCAM camera (1, 2, 3 or 4) {image extension keyword: CAMNUM} |
int |
4 |
|
|
obs.field |
camNum |
MultiframeDetector |
WSATransit |
Number of WFCAM camera (1, 2, 3 or 4) {image extension keyword: CAMNUM} |
int |
4 |
|
|
obs.field |
camNum |
MultiframeDetector |
WSAUHS |
Number of WFCAM camera (1, 2, 3 or 4) {image extension keyword: CAMNUM} |
int |
4 |
|
|
obs.field |
camPower |
MultiframeDetector |
WSA |
Camera power (On|Off) {image extension keyword: CAMPOWER} |
varchar |
3 |
|
--- |
?? |
camPower |
MultiframeDetector |
WSACalib |
Camera power (On|Off) {image extension keyword: CAMPOWER} |
varchar |
3 |
|
--- |
?? |
camPower |
MultiframeDetector |
WSATransit |
Camera power (On|Off) {image extension keyword: CAMPOWER} |
varchar |
3 |
|
--- |
?? |
camPower |
MultiframeDetector |
WSAUHS |
Camera power (On|Off) {image extension keyword: CAMPOWER} |
varchar |
3 |
|
--- |
?? |
camReadOut |
MultiframeDetector |
WSA |
Camera readout (CDS|NDR|SAR|RRR) {image extension keyword: READOUT} |
varchar |
3 |
|
--- |
?? |
camReadOut |
MultiframeDetector |
WSACalib |
Camera readout (CDS|NDR|SAR|RRR) {image extension keyword: READOUT} |
varchar |
3 |
|
--- |
?? |
camReadOut |
MultiframeDetector |
WSATransit |
Camera readout (CDS|NDR|SAR|RRR) {image extension keyword: READOUT} |
varchar |
3 |
|
--- |
?? |
camReadOut |
MultiframeDetector |
WSAUHS |
Camera readout (CDS|NDR|SAR|RRR) {image extension keyword: READOUT} |
varchar |
3 |
|
--- |
?? |
camRole |
MultiframeDetector |
WSA |
Camera role (master|slave|unsync) {image extension keyword: CAMROLE} |
varchar |
8 |
|
NONE |
?? |
camRole |
MultiframeDetector |
WSACalib |
Camera role (master|slave|unsync) {image extension keyword: CAMROLE} |
varchar |
8 |
|
NONE |
?? |
camRole |
MultiframeDetector |
WSATransit |
Camera role (master|slave|unsync) {image extension keyword: CAMROLE} |
varchar |
8 |
|
NONE |
?? |
camRole |
MultiframeDetector |
WSAUHS |
Camera role (master|slave|unsync) {image extension keyword: CAMROLE} |
varchar |
8 |
|
NONE |
?? |
cat |
twomass_sixx2_psc, twomass_sixx2_scn, twomass_sixx2_xsc |
2MASS |
Catalog indicator 1=catalog, 0=not catalog |
smallint |
2 |
|
|
|
catalogueID |
MapFrameStatus |
WSAUHS |
Unique identifier for catalogue |
bigint |
8 |
|
-99999999 |
meta_id;meta_main |
catalogueID |
lasMapRemeasAver, MapFrameStatus |
WSA |
Unique identifier for catalogue |
bigint |
8 |
|
-99999999 |
meta_id;meta_main |
catalogueID |
MapProvenance |
WSA |
the UID of the component frame |
bigint |
8 |
|
|
obs.field |
catalogueID |
MapProvenance |
WSAUHS |
the UID of the component frame |
bigint |
8 |
|
|
obs.field |
catalogueID |
lasMapAverageWeights |
WSA |
Unique identifier for input catalogue |
bigint |
8 |
|
-99999999 |
meta_id |
catalogueID |
lasMapRemeasurement |
WSA |
Unique identifier for catalogue {catalogue extension keyword: CATLGID} |
bigint |
8 |
|
-99999999 |
meta_id;meta_main |
catalogueSchema |
Programme |
WSA |
Script file that describes the catalogue schema |
varchar |
64 |
|
|
?? |
catalogueSchema |
Programme |
WSACalib |
Script file that describes the catalogue schema |
varchar |
64 |
|
|
?? |
catalogueSchema |
Programme |
WSATransit |
Script file that describes the catalogue schema |
varchar |
64 |
|
|
?? |
catalogueSchema |
Programme |
WSAUHS |
Script file that describes the catalogue schema |
varchar |
64 |
|
|
?? |
catCreationDate |
MultiframeDetector |
WSA |
Creation date/time of catalogue file {catalogue extension keyword: DATE} |
datetime |
8 |
MM-DD-YYYY:hh:mm:ss.sss |
12-31-9999 |
?? |
catCreationDate |
MultiframeDetector |
WSACalib |
Creation date/time of catalogue file {catalogue extension keyword: DATE} |
datetime |
8 |
MM-DD-YYYY:hh:mm:ss.sss |
12-31-9999 |
?? |
catCreationDate |
MultiframeDetector |
WSATransit |
Creation date/time of catalogue file {catalogue extension keyword: DATE} |
datetime |
8 |
MM-DD-YYYY:hh:mm:ss.sss |
12-31-9999 |
?? |
catCreationDate |
MultiframeDetector |
WSAUHS |
Creation date/time of catalogue file {catalogue extension keyword: DATE} |
datetime |
8 |
MM-DD-YYYY:hh:mm:ss.sss |
12-31-9999 |
?? |
catName |
MapFrameStatus |
WSA |
the filename of the associated catalogue MEF, eg. server:/path/filename_list.fits |
varchar |
256 |
|
NONE |
ID_CATALOG |
catName |
MapFrameStatus |
WSAUHS |
the filename of the associated catalogue MEF, eg. server:/path/filename_list.fits |
varchar |
256 |
|
NONE |
ID_CATALOG |
catName |
Multiframe |
WSA |
the filename of the associated catalogue MEF, eg. server:/path/filename.fits |
varchar |
256 |
|
|
meta.id;meta.dataset |
catName |
Multiframe |
WSACalib |
the filename of the associated catalogue MEF, eg. server:/path/filename.fits |
varchar |
256 |
|
|
meta.id;meta.dataset |
catName |
Multiframe |
WSATransit |
the filename of the associated catalogue MEF, eg. server:/path/filename.fits |
varchar |
256 |
|
|
meta.id;meta.dataset |
catName |
Multiframe |
WSAUHS |
the filename of the associated catalogue MEF, eg. server:/path/filename.fits |
varchar |
256 |
|
|
meta.id;meta.dataset |
catName |
iras_assoc_cats |
IRAS |
Source Name |
varchar |
32 |
|
|
ID_MAIN |
catNo |
iras_asc, iras_assoc_cats |
IRAS |
Catalog number |
tinyint |
1 |
|
|
ID_CATALOG |
cc_100 |
iras_psc |
IRAS |
point source correlation coefficient (100 micron). |
varchar |
1 |
|
|
REMARKS |
cc_12 |
iras_psc |
IRAS |
point source correlation coefficient (12 micron). |
varchar |
1 |
|
|
REMARKS |
cc_25 |
iras_psc |
IRAS |
point source correlation coefficient (25 micron). |
varchar |
1 |
|
|
REMARKS |
cc_60 |
iras_psc |
IRAS |
point source correlation coefficient (60 micron). |
varchar |
1 |
|
|
REMARKS |
cc_flags |
allwise_sc |
WISE |
Contamination and confusion flag. Four character string, one character per band [W1/W2/W3/W4], that indicates that the photometry and/or position measurements of a source may be contaminated or biased due to proximity to an image artifact. CAUTION: Non-zero cc_flags values in any band indicate the the measurement in that band may be contaminated and the photometry should be used with caution. |
varchar |
4 |
|
|
|
The type of artifact that may contaminate the measurements is denoted by the following codes. Lower-case letters correspond to instances in which the source detection in a band is believed to be real but the measurement may be contaminated by the artifact. Upper-case letters are instances in which the source detection in a band may be a spurious detection of an artifact. - D,d - Diffraction spike. Source may be a spurious detection of (D) or contaminated by (d) a diffraction spike from a nearby bright star on the same image, or
- P,p - Persistence. Source may be a spurious detection of (P) or contaminated by (p) a short-term latent image left by a bright source, or
- H,h - Halo. Source may be a spurious detection of (H) or contaminated by (h) the scattered light halo surrounding a nearby bright source, or
- O,o (letter "o") - Optical ghost. Source may be a spurious detection of (O) or contaminated by (o) an optical ghost image caused by a nearby bright source, or
- 0 (number zero) - Source is unaffected by known artifacts.
A source extraction may be affected by more than one type of artifact or condition. In this event, the cc_flags value in each band is set in the following priority order: D,P,H,O,d,p,h,o,0. The full tally of artifacts affecting a source in each band is given in the w?cc_map and w?cc_map_str columns. A source can appear in the AllWISE Source Catalog even if it is flagged as a spurious artifact detection in a band if there is a reliable detection in another band that is not flagged as a spurious artifact detection. Entries in the AllWISE Reject Table may be flagged as spurious detections of artifacts in all bands. |
cc_flags |
catwise_2020, catwise_prelim |
WISE |
worst case 4 character cc_flag from AllWISE |
varchar |
16 |
|
|
|
cc_flags |
wise_allskysc |
WISE |
Contamination and confusion flag. Four character strong, one character per band [W1/W2/W3/W4], that indicates that the photometry and/or position measurements of a source may be contaminated or biased due to proximity to an image artifact. CAUTION: Non-zero cc_flags values in any band indicate the the measurement in that band may be contaminated and the photometry should be used with caution. |
char |
4 |
|
|
|
cc_flags |
wise_prelimsc |
WISE |
Contamination and confusion flag Four character strong, one character per band [W1/W2/W3/W4], that indicates that the photometry and/or position measurements of a source may be contaminated or biased due to proximity to an image artifact |
char |
4 |
|
|
|
cc_flg |
twomass_psc |
2MASS |
Contamination and confusion flag. |
varchar |
3 |
|
|
CODE_MISC |
cc_flg |
twomass_sixx2_psc |
2MASS |
indicates JHK artifact contamination and/or confusion |
varchar |
3 |
|
|
|
cc_flg |
twomass_sixx2_xsc |
2MASS |
indicates artifact contamination and/or confusion |
varchar |
1 |
|
|
|
cc_flg |
twomass_xsc |
2MASS |
indicates artifact contamination and/or confusion. |
varchar |
1 |
|
|
CODE_MISC |
CCD |
mgcDetection |
MGC |
CCD number |
tinyint |
1 |
|
|
|
ccdHeaterLevel |
Multiframe |
WSA |
AG CCD heater level (in percent) {image primary HDU keyword: CCD_HTP} |
real |
4 |
|
-0.9999995e9 |
|
ccdHeaterLevel |
Multiframe |
WSACalib |
AG CCD heater level (in percent) {image primary HDU keyword: CCD_HTP} |
real |
4 |
|
-0.9999995e9 |
|
ccdHeaterLevel |
Multiframe |
WSATransit |
AG CCD heater level (in percent) {image primary HDU keyword: CCD_HTP} |
real |
4 |
|
-0.9999995e9 |
|
ccdHeaterLevel |
Multiframe |
WSAUHS |
AG CCD heater level (in percent) {image primary HDU keyword: CCD_HTP} |
real |
4 |
|
-0.9999995e9 |
|
ccdm |
tycho2 |
GAIADR1 |
CCDM component identifier for Hipparcos stars |
varchar |
4 |
|
|
meta.code.multip |
ccdTemp |
Multiframe |
WSA |
AG CCD temperature {image primary HDU keyword: CCD_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
ccdTemp |
Multiframe |
WSACalib |
AG CCD temperature {image primary HDU keyword: CCD_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
ccdTemp |
Multiframe |
WSATransit |
AG CCD temperature {image primary HDU keyword: CCD_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
ccdTemp |
Multiframe |
WSAUHS |
AG CCD temperature {image primary HDU keyword: CCD_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
ccdTempSetPt |
Multiframe |
WSA |
AG CCD temperature setpoint {image primary HDU keyword: CCDTEMPS} |
real |
4 |
|
-0.9999995e9 |
|
ccdTempSetPt |
Multiframe |
WSACalib |
AG CCD temperature setpoint {image primary HDU keyword: CCDTEMPS} |
real |
4 |
|
-0.9999995e9 |
|
ccdTempSetPt |
Multiframe |
WSATransit |
AG CCD temperature setpoint {image primary HDU keyword: CCDTEMPS} |
real |
4 |
|
-0.9999995e9 |
|
ccdTempSetPt |
Multiframe |
WSAUHS |
AG CCD temperature setpoint {image primary HDU keyword: CCDTEMPS} |
real |
4 |
|
-0.9999995e9 |
|
cd11 |
CurrentAstrometry |
WSACalib |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_1} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd11 |
CurrentAstrometry |
WSATransit |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_1} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd11 |
CurrentAstrometry |
WSAUHS |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_1} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd11 |
CurrentAstrometry, PreviousAstrometry |
WSA |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_1} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd12 |
CurrentAstrometry |
WSACalib |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_2} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd12 |
CurrentAstrometry |
WSATransit |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_2} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd12 |
CurrentAstrometry |
WSAUHS |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_2} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd12 |
CurrentAstrometry, PreviousAstrometry |
WSA |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_2} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd21 |
CurrentAstrometry |
WSACalib |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_1} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd21 |
CurrentAstrometry |
WSATransit |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_1} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd21 |
CurrentAstrometry |
WSAUHS |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_1} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd21 |
CurrentAstrometry, PreviousAstrometry |
WSA |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_1} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd22 |
CurrentAstrometry |
WSACalib |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_2} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd22 |
CurrentAstrometry |
WSATransit |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_2} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd22 |
CurrentAstrometry |
WSAUHS |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_2} |
float |
8 |
|
|
pos.wcs.cdmatrix |
cd22 |
CurrentAstrometry, PreviousAstrometry |
WSA |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_2} |
float |
8 |
|
|
pos.wcs.cdmatrix |
centralDec |
CurrentAstrometry |
WSACalib |
Dec (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
centralDec |
CurrentAstrometry |
WSATransit |
Dec (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
centralDec |
CurrentAstrometry |
WSAUHS |
Dec (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
centralDec |
CurrentAstrometry, PreviousAstrometry |
WSA |
Dec (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos.eq.dec;meta.main |
centralRa |
CurrentAstrometry |
WSACalib |
RA (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos.eq.ra;meta.main |
centralRa |
CurrentAstrometry |
WSATransit |
RA (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos.eq.ra;meta.main |
centralRa |
CurrentAstrometry |
WSAUHS |
RA (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos.eq.ra;meta.main |
centralRa |
CurrentAstrometry, PreviousAstrometry |
WSA |
RA (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
pos.eq.ra;meta.main |
CHI |
mgcGalaxyStruct |
MGC |
Chi^2 of GIM2D Fit |
real |
4 |
|
99.99 |
|
chi2 |
calVariability |
WSACalib |
Chi-squared value of astrometric solution |
real |
4 |
|
-0.9999995e9 |
FIT_CHI2 |
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. |
chi2 |
dxsVariability, gcsVariability, gpsVariability, lasVariability, udsVariability |
WSA |
Chi-squared value of astrometric solution |
real |
4 |
|
-0.9999995e9 |
FIT_CHI2 |
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. |
chi2 |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource |
WSA |
Chi-squared value of proper motion solution |
real |
4 |
|
-0.9999995e9 |
FIT_CHI2 |
chi2 |
uhsVariability |
WSAUHS |
Chi-squared value of astrometric solution |
real |
4 |
|
-0.9999995e9 |
FIT_CHI2 |
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. |
chi2pmdec |
catwise_2020, catwise_prelim |
WISE |
chi-square for PMRA difference (1 DF) |
real |
4 |
|
|
|
chi2pmra |
catwise_2020, catwise_prelim |
WISE |
chi-square for PMRA difference (1 DF) |
real |
4 |
|
|
|
chi2s |
dxsAstrometricInfo, gcsAstrometricInfo, gpsAstrometricInfo, lasAstrometricInfo, udsAstrometricInfo |
WSA |
Reduced chi-squared of fit |
float |
8 |
|
-0.9999995e9 |
?? |
chi2s |
uhsAstrometricInfo |
WSAUHS |
Reduced chi-squared of fit |
float |
8 |
|
-0.9999995e9 |
?? |
CIR_BVAR |
MultiframeDetector |
WSA |
Latest estimate of background variance {image extension keyword: CIR_BVAR} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIR_BVAR |
MultiframeDetector |
WSACalib |
Latest estimate of background variance {image extension keyword: CIR_BVAR} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIR_BVAR |
MultiframeDetector |
WSATransit |
Latest estimate of background variance {image extension keyword: CIR_BVAR} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIR_BVAR |
MultiframeDetector |
WSAUHS |
Latest estimate of background variance {image extension keyword: CIR_BVAR} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIR_SCAL |
MultiframeDetector |
WSA |
Background scale relative to group maximum {image extension keyword: CIR_SCAL} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIR_SCAL |
MultiframeDetector |
WSACalib |
Background scale relative to group maximum {image extension keyword: CIR_SCAL} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIR_SCAL |
MultiframeDetector |
WSATransit |
Background scale relative to group maximum {image extension keyword: CIR_SCAL} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIR_SCAL |
MultiframeDetector |
WSAUHS |
Background scale relative to group maximum {image extension keyword: CIR_SCAL} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIR_ZERO |
MultiframeDetector |
WSA |
Pedestal value relative to group average {image extension keyword: CIR_ZERO} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
CIR_ZERO |
MultiframeDetector |
WSACalib |
Pedestal value relative to group average {image extension keyword: CIR_ZERO} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
CIR_ZERO |
MultiframeDetector |
WSATransit |
Pedestal value relative to group average {image extension keyword: CIR_ZERO} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
CIR_ZERO |
MultiframeDetector |
WSAUHS |
Pedestal value relative to group average {image extension keyword: CIR_ZERO} |
real |
4 |
|
-0.9999995e9 |
stat.fit.param |
CIRMED |
MultiframeDetector |
WSA |
Latest estimate of background {image extension keyword: CIRMED} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIRMED |
MultiframeDetector |
WSACalib |
Latest estimate of background {image extension keyword: CIRMED} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIRMED |
MultiframeDetector |
WSATransit |
Latest estimate of background {image extension keyword: CIRMED} |
real |
4 |
|
-0.9999995e9 |
instr.background |
CIRMED |
MultiframeDetector |
WSAUHS |
Latest estimate of background {image extension keyword: CIRMED} |
real |
4 |
|
-0.9999995e9 |
instr.background |
cirr1 |
iras_psc |
IRAS |
Number of nearby 100 micron only WSDB sources |
tinyint |
1 |
|
|
NUMBER |
cirr2 |
iras_psc |
IRAS |
Spatially filtered 100 micron sky brightness ratio to flux density of point source |
tinyint |
1 |
|
|
PHOT_FLUX_RATIO |
cirr3 |
iras_psc |
IRAS |
Total 100 micron sky surface brightness |
smallint |
2 |
MJy/sr |
|
PHOT_SB_IR-100 |
CLASS |
mgcDetection |
MGC |
Classification parameter |
smallint |
2 |
|
|
|
class |
UKIDSSDetection |
WSA |
Flag indicating most probable morphological classification |
smallint |
2 |
|
|
CLASS_MISC |
class |
calDetection |
WSACalib |
Flag indicating most probable morphological classification {catalogue TType keyword: Classification} -1 stellar, +1 non--stellar, 0 noise, -2 borderline stellar, -3 borderline galaxy, -9 saturated |
smallint |
2 |
|
|
CLASS_MISC |
A discrete classification code for each detected image, based on various cuts on morphological parameters (see the Glossary entries for classStat and ell for further details). It is primarily based on cuts on the stellar profile statistic classStat and necessarily trades-off completeness against reliability between point-like (e.g. stellar) and extended (e.g. galaxy) images. The class assignments are as follows: Flag | Meaning | Generally satisfies | -2 | Probable star | +2.0≤classStat≤+3.0 | -1 | Star | -3.0≤classStat≤+2.0 | 0 | Noise | classStat≤-3.0 | +1 | Galaxy | classStat≥+3.0 | but these are also moderated by ellipticity overrides (e.g. ellipticity≥0.9 is flagged as class 0) and magnitude-dependent information (e.g. near or at saturation objects are preferentially flagged as class -1). Hence class is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely point-source samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point/extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). For much more information concerning the class attribute, see the CASU standard source extraction documentation. |
class |
dxsDetection, gcsDetection, gpsDetection, lasDetection |
WSA |
Flag indicating most probable morphological classification {catalogue TType keyword: Classification} -1 stellar, +1 non--stellar, 0 noise, -2 borderline stellar, -3 borderline galaxy, -9 saturated |
smallint |
2 |
|
|
CLASS_MISC |
A discrete classification code for each detected image, based on various cuts on morphological parameters (see the Glossary entries for classStat and ell for further details). It is primarily based on cuts on the stellar profile statistic classStat and necessarily trades-off completeness against reliability between point-like (e.g. stellar) and extended (e.g. galaxy) images. The class assignments are as follows: Flag | Meaning | Generally satisfies | -2 | Probable star | +2.0≤classStat≤+3.0 | -1 | Star | -3.0≤classStat≤+2.0 | 0 | Noise | classStat≤-3.0 | +1 | Galaxy | classStat≥+3.0 | but these are also moderated by ellipticity overrides (e.g. ellipticity≥0.9 is flagged as class 0) and magnitude-dependent information (e.g. near or at saturation objects are preferentially flagged as class -1). Hence class is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely point-source samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point/extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). For much more information concerning the class attribute, see the CASU standard source extraction documentation. |
class |
lasMapRemeasAver |
WSA |
Merged Flag indicating most probable morphological classification -1 stellar, +1 non--stellar, 0 noise, -2 borderline stellar, -3 borderline galaxy, -9 saturated |
smallint |
2 |
|
|
src.class |
A discrete classification code for each detected image, based on various cuts on morphological parameters (see the Glossary entries for classStat and ell for further details). It is primarily based on cuts on the stellar profile statistic classStat and necessarily trades-off completeness against reliability between point-like (e.g. stellar) and extended (e.g. galaxy) images. The class assignments are as follows: Flag | Meaning | Generally satisfies | -2 | Probable star | +2.0≤classStat≤+3.0 | -1 | Star | -3.0≤classStat≤+2.0 | 0 | Noise | classStat≤-3.0 | +1 | Galaxy | classStat≥+3.0 | but these are also moderated by ellipticity overrides (e.g. ellipticity≥0.9 is flagged as class 0) and magnitude-dependent information (e.g. near or at saturation objects are preferentially flagged as class -1). Hence class is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely point-source samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point/extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). For much more information concerning the class attribute, see the CASU standard source extraction documentation. |
class |
lasMapRemeasurement |
WSA |
Flag indicating most probable morphological classification {catalogue TType keyword: Classification} -1 stellar, +1 non--stellar, 0 noise, -2 borderline stellar, -3 borderline galaxy, -9 saturated |
smallint |
2 |
|
|
stat |
A discrete classification code for each detected image, based on various cuts on morphological parameters (see the Glossary entries for classStat and ell for further details). It is primarily based on cuts on the stellar profile statistic classStat and necessarily trades-off completeness against reliability between point-like (e.g. stellar) and extended (e.g. galaxy) images. The class assignments are as follows: Flag | Meaning | Generally satisfies | -2 | Probable star | +2.0≤classStat≤+3.0 | -1 | Star | -3.0≤classStat≤+2.0 | 0 | Noise | classStat≤-3.0 | +1 | Galaxy | classStat≥+3.0 | but these are also moderated by ellipticity overrides (e.g. ellipticity≥0.9 is flagged as class 0) and magnitude-dependent information (e.g. near or at saturation objects are preferentially flagged as class -1). Hence class is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely point-source samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point/extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). For much more information concerning the class attribute, see the CASU standard source extraction documentation. |
class |
ptsDetection |
WSATransit |
Flag indicating most probable morphological classification {catalogue TType keyword: Classification} -1 stellar, +1 non--stellar, 0 noise, -2 borderline stellar, -3 borderline galaxy, -9 saturated |
smallint |
2 |
|
|
CLASS_MISC |
A discrete classification code for each detected image, based on various cuts on morphological parameters (see the Glossary entries for classStat and ell for further details). It is primarily based on cuts on the stellar profile statistic classStat and necessarily trades-off completeness against reliability between point-like (e.g. stellar) and extended (e.g. galaxy) images. The class assignments are as follows: Flag | Meaning | Generally satisfies | -2 | Probable star | +2.0≤classStat≤+3.0 | -1 | Star | -3.0≤classStat≤+2.0 | 0 | Noise | classStat≤-3.0 | +1 | Galaxy | classStat≥+3.0 | but these are also moderated by ellipticity overrides (e.g. ellipticity≥0.9 is flagged as class 0) and magnitude-dependent information (e.g. near or at saturation objects are preferentially flagged as class -1). Hence class is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely point-source samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point/extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). For much more information concerning the class attribute, see the CASU standard source extraction documentation. |
class |
udsDetection |
WSA |
Flag indicating most probable morphological classification {catalogue TType keyword: Classification} -1 stellar, +1 non--stellar, 0 noise, -2 borderline stellar, -3 boderline galaxy, -9 saturated |
smallint |
2 |
|
|
CLASS_MISC |
Using the SE classification statistic (see the corresponding entry for classStat), a CASU-like discrete classification code is assigned for each detected object as follows: Flag | Meaning | | -9 | Saturated | | -3 | Probable galaxy | | -2 | Probable star | | -1 | Star | | +1 | Galaxy | | where rectangular regions in the magnitude-classStat plane are used to select each class. |
class |
uhsDetection, uhsDetectionAll |
WSAUHS |
Flag indicating most probable morphological classification {catalogue TType keyword: Classification} -1 stellar, +1 non--stellar, 0 noise, -2 borderline stellar, -3 borderline galaxy, -9 saturated |
smallint |
2 |
|
|
CLASS_MISC |
A discrete classification code for each detected image, based on various cuts on morphological parameters (see the Glossary entries for classStat and ell for further details). It is primarily based on cuts on the stellar profile statistic classStat and necessarily trades-off completeness against reliability between point-like (e.g. stellar) and extended (e.g. galaxy) images. The class assignments are as follows: Flag | Meaning | Generally satisfies | -2 | Probable star | +2.0≤classStat≤+3.0 | -1 | Star | -3.0≤classStat≤+2.0 | 0 | Noise | classStat≤-3.0 | +1 | Galaxy | classStat≥+3.0 | but these are also moderated by ellipticity overrides (e.g. ellipticity≥0.9 is flagged as class 0) and magnitude-dependent information (e.g. near or at saturation objects are preferentially flagged as class -1). Hence class is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely point-source samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point/extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). For much more information concerning the class attribute, see the CASU standard source extraction documentation. |
classification |
igsl_source |
GAIADR1 |
Classification, simply a 0=star and 1=nonstar taken from different sources as given in the souce_classification field |
bit |
1 |
|
|
meta.code.class |
classification |
variable_summary |
GAIADR1 |
Photometric variability classification "RRLYR" (for RR Lyrae) or "CEP" (for Cepheid) |
varchar |
8 |
|
|
meta.code.class;src.var |
classStat |
UKIDSSDetection |
WSA |
N(0,1) stellarness-of-profile statistic |
real |
4 |
|
|
STAT_PROP |
classStat |
calDetection |
WSACalib |
N(0,1) stellarness-of-profile statistic {catalogue TType keyword: Statistic} |
real |
4 |
|
|
STAT_PROP |
An equivalent N(0,1) measure of how point-like an image is, used in deriving the class attribute in a 'necessary but not sufficient' sense. Derived mainly from the curve-of-growth of flux using the well-defined stellar locus as a function of magnitude as a benchmark (see Irwin et al. 2004 SPIE 5493 411 for more details). Note that the assignment of the discrete classification flag class=-1 is based on a cut of -3.0≤classStat≤+2.0 cut on this statistic (along with ellipticity and magnitude information) and hence is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely stellar samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point or extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). |
classStat |
dxsDetection, gcsDetection, gpsDetection, lasDetection |
WSA |
N(0,1) stellarness-of-profile statistic {catalogue TType keyword: Statistic} |
real |
4 |
|
|
STAT_PROP |
An equivalent N(0,1) measure of how point-like an image is, used in deriving the class attribute in a 'necessary but not sufficient' sense. Derived mainly from the curve-of-growth of flux using the well-defined stellar locus as a function of magnitude as a benchmark (see Irwin et al. 2004 SPIE 5493 411 for more details). Note that the assignment of the discrete classification flag class=-1 is based on a cut of -3.0≤classStat≤+2.0 cut on this statistic (along with ellipticity and magnitude information) and hence is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely stellar samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point or extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). |
classStat |
lasMapRemeasAver |
WSA |
Averaged N(0,1) stellarness-of-profile statistic (SE: classification statistic CLASS_STAR; 0 - galaxy, 1 - star) |
real |
4 |
|
|
stat |
An equivalent N(0,1) measure of how point-like an image is, used in deriving the class attribute in a 'necessary but not sufficient' sense. Derived mainly from the curve-of-growth of flux using the well-defined stellar locus as a function of magnitude as a benchmark (see Irwin et al. 2004 SPIE 5493 411 for more details). Note that the assignment of the discrete classification flag class=-1 is based on a cut of -3.0≤classStat≤+2.0 cut on this statistic (along with ellipticity and magnitude information) and hence is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely stellar samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point or extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). |
classStat |
lasMapRemeasurement |
WSA |
N(0,1) stellarness-of-profile statistic (SE: classification statistic CLASS_STAR; 0 - galaxy, 1 - star) {catalogue TType keyword: Statistic} |
real |
4 |
|
|
stat |
An equivalent N(0,1) measure of how point-like an image is, used in deriving the class attribute in a 'necessary but not sufficient' sense. Derived mainly from the curve-of-growth of flux using the well-defined stellar locus as a function of magnitude as a benchmark (see Irwin et al. 2004 SPIE 5493 411 for more details). Note that the assignment of the discrete classification flag class=-1 is based on a cut of -3.0≤classStat≤+2.0 cut on this statistic (along with ellipticity and magnitude information) and hence is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely stellar samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point or extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). |
classStat |
ptsDetection |
WSATransit |
N(0,1) stellarness-of-profile statistic {catalogue TType keyword: Statistic} |
real |
4 |
|
|
STAT_PROP |
An equivalent N(0,1) measure of how point-like an image is, used in deriving the class attribute in a 'necessary but not sufficient' sense. Derived mainly from the curve-of-growth of flux using the well-defined stellar locus as a function of magnitude as a benchmark (see Irwin et al. 2004 SPIE 5493 411 for more details). Note that the assignment of the discrete classification flag class=-1 is based on a cut of -3.0≤classStat≤+2.0 cut on this statistic (along with ellipticity and magnitude information) and hence is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely stellar samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point or extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). |
classStat |
udsDetection |
WSA |
S-Extractor classification statistic CLASS_STAR (0 - galaxy, 1 - star) {catalogue TType keyword: Statistic} |
real |
4 |
|
|
STAT_PROP |
CLASS_STAR is SE's classification of objects on the basis of a Neural Network Output. There are several input parameters which are directly linked to the CLASS_STAR parameter: PIXEL_SCALE | Pixel size in arsec. | SEEING_FWHM | FWHM of stellar images in arcsec. | BACK_SIZE | Size, or Width, Height (in pixels) of a background mesh. | THRESH_TYPE | Meaning of the DETECT_THRESH and ANALYSIS_THRESH parameters: RELATIVE (scaling factor to the background rms) or ABSOLUTE (absolute level) | ANALYSIS_THRESH | Threshold (in surface brightness) at which CLASS_STAR and FWHM operate: 1argument (relative to background rms) or 2 arguments (mu[mag/arcsec²], zero-point [mag]) | A perfectly point-like (stellar) object has class=1.0. |
classStat |
uhsDetection, uhsDetectionAll |
WSAUHS |
N(0,1) stellarness-of-profile statistic {catalogue TType keyword: Statistic} |
real |
4 |
|
|
STAT_PROP |
An equivalent N(0,1) measure of how point-like an image is, used in deriving the class attribute in a 'necessary but not sufficient' sense. Derived mainly from the curve-of-growth of flux using the well-defined stellar locus as a function of magnitude as a benchmark (see Irwin et al. 2004 SPIE 5493 411 for more details). Note that the assignment of the discrete classification flag class=-1 is based on a cut of -3.0≤classStat≤+2.0 cut on this statistic (along with ellipticity and magnitude information) and hence is conservative in the sense that it defines galaxy samples optimised for completeness, and conversely stellar samples optimised for reliability. For examples of the use of the various classification attributes in sample selection, especially with respect to the trade-off between completeness and reliability for point or extended samples, see the Views predefined in the WSA schema (these can be examined using the schema browser). |
clat |
twomass_sixx2_psc, twomass_sixx2_scn |
2MASS |
The computed dec (J2000 EQ) of scan center in sexigesimal. |
varchar |
16 |
|
|
|
clat |
twomass_sixx2_xsc |
2MASS |
The computed dec (J2000 EQ) in sexigesimal. |
varchar |
16 |
|
|
|
cld |
twomass_scn |
2MASS |
Special flag indicating whether or not a cloud was found in the scan after comparison of its photometry to that of overlapping scans in the database. |
smallint |
2 |
|
|
CODE_MISC |
cld |
twomass_sixx2_scn |
2MASS |
downgrade from DB photom. overlap comparison (clouds) (0|1) |
smallint |
2 |
|
|
|
clon |
twomass_sixx2_psc, twomass_sixx2_scn |
2MASS |
The computed ra (J2000 EQ) of scan center in sexigesimal. |
varchar |
16 |
|
|
|
clon |
twomass_sixx2_xsc |
2MASS |
The computed ra (J2000 EQ) in sexigesimal. |
varchar |
16 |
|
|
|
cntr |
allwise_sc |
WISE |
Unique identification number for this object in the AllWISE Catalog/Reject Table. This number is formed from the source_id, which is in turn formed from the coadd_id and source number, src. |
bigint |
8 |
|
|
|
The cntr value is formed by making the source_id into an integer, in the format: RRRRsDDDtrevIIIIII, where For example, a source in the Tile 3041m137_ac51, with a source_id of '3041m137_ac51-012345', has a cntr value of 3041013701351012345. NOTE: AllWISE Catalog and Reject Table entries are cross-referenced with the Multiepoch Photometry (MEP) Database via the cntr identifier. The Catalog/Reject Table cntr value is referred to as cntr_mf in the MEP Database. |
cntr |
catwise_2020, catwise_prelim |
WISE |
Unique identifier |
int |
4 |
|
|
|
cntr |
twomass_sixx2_scn, twomass_sixx2_xsc |
2MASS |
entry counter (key) number (unique within table) |
int |
4 |
|
|
|
cntr |
wise_allskysc |
WISE |
Unique identification number for the Catalog source This number is formed entirely from the source_id, which is in turn formed from the coadd_id and source number src. On average, sources with cntr values close to each other are also close to each other on the sky, except at Tile boundaries. |
bigint |
8 |
|
|
ID_MAIN |
cntr |
wise_prelimsc |
WISE |
Unique identification number for the Catalog source This number is formed entirely from the source_id, which is in turn formed from the coadd_id and source number src. On average, sources with cntr values close to each other are also close to each other on the sky, except at Tile boundaries |
bigint |
8 |
|
|
ID_MAIN |
coadd |
twomass_psc |
2MASS |
Sequence number of the Atlas Image in which the position of this source falls. |
smallint |
2 |
|
|
NUMBER |
coadd |
twomass_xsc |
2MASS |
3-digit coadd number (unique within scan). |
smallint |
2 |
|
|
NUMBER |
coadd_id |
allwise_sc |
WISE |
Atlas Tile identifier from which source was extracted. |
varchar |
20 |
|
|
|
The identifier has the general form: RRRRsDDD_[trev], where |
coadd_id |
wise_allskysc |
WISE |
Atlas Tile identifier from which source was extracted. |
char |
20 |
|
|
|
coadd_id |
wise_prelimsc |
WISE |
Atlas Tile identifier from which source was extracted |
char |
20 |
|
|
|
coadd_key |
twomass_psc |
2MASS |
Unique identification number of the record in the Atlas Image Data Table (NOT YET AVAILABLE) that corresponds to Image in which the position of this source falls. |
int |
4 |
|
|
ID_NUMBER |
coadd_key |
twomass_xsc |
2MASS |
key to coadd data record in "scan DB". |
int |
4 |
|
|
ID_NUMBER |
combicatID |
MapProvenance |
WSA |
the UID of the combined frame (=combiframe) |
bigint |
8 |
|
|
obs.field |
combicatID |
MapProvenance |
WSAUHS |
the UID of the combined frame (=combiframe) |
bigint |
8 |
|
|
obs.field |
combicatID |
lasMapAverageWeights |
WSA |
Unique identifier for combined average catalogue |
bigint |
8 |
|
-99999999 |
meta_id;meta_main |
combiframeID |
Provenance |
WSA |
the UID of the combined frame (=combiframe) |
bigint |
8 |
|
|
obs.field |
combiframeID |
Provenance |
WSACalib |
the UID of the combined frame (=combiframe) |
bigint |
8 |
|
|
obs.field |
combiframeID |
Provenance |
WSATransit |
the UID of the combined frame (=combiframe) |
bigint |
8 |
|
|
obs.field |
combiframeID |
Provenance |
WSAUHS |
the UID of the combined frame (=combiframe) |
bigint |
8 |
|
|
obs.field |
combiProdType |
ProductLinks |
WSA |
Type (stack,tile,mosaic) of combination frame |
varchar |
8 |
|
|
?? |
combiProdType |
ProductLinks |
WSAUHS |
Type (stack,tile,mosaic) of combination frame |
varchar |
8 |
|
|
?? |
combiProductID |
ProductLinks |
WSA |
Product ID of combination frame |
int |
4 |
|
|
?? |
combiProductID |
ProductLinks |
WSAUHS |
Product ID of combination frame |
int |
4 |
|
|
?? |
comment |
ArchiveCurationHistory |
WSA |
Comment string supplied by the curator |
varchar |
256 |
|
|
?? |
comment |
ArchiveCurationHistory |
WSACalib |
Comment string supplied by the curator |
varchar |
256 |
|
|
?? |
comment |
ArchiveCurationHistory |
WSATransit |
Comment string supplied by the curator |
varchar |
256 |
|
|
?? |
comment |
ArchiveCurationHistory |
WSAUHS |
Comment string supplied by the curator |
varchar |
256 |
|
|
?? |
compFile |
MultiframeDetector |
WSA |
Filename of the compressed image of this image frame, eg. server:/path/filename.jpg |
varchar |
256 |
|
NONE |
meta.id;meta.file |
compFile |
MultiframeDetector |
WSACalib |
Filename of the compressed image of this image frame, eg. server:/path/filename.jpg |
varchar |
256 |
|
NONE |
meta.id;meta.file |
compFile |
MultiframeDetector |
WSATransit |
Filename of the compressed image of this image frame, eg. server:/path/filename.jpg |
varchar |
256 |
|
NONE |
meta.id;meta.file |
compFile |
MultiframeDetector |
WSAUHS |
Filename of the compressed image of this image frame, eg. server:/path/filename.jpg |
varchar |
256 |
|
NONE |
meta.id;meta.file |
conf |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca |
GLIMPSE |
Close source flag |
smallint |
2 |
|
-9 |
CODE_MISC |
conf |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Confusion flag |
smallint |
2 |
|
-9 |
CODE_MISC |
confID |
Multiframe |
WSA |
UID of library calibration confidence frame {image extension keyword: CIR_CPM} |
bigint |
8 |
|
-99999999 |
obs.field |
confID |
Multiframe |
WSACalib |
UID of library calibration confidence frame {image extension keyword: CIR_CPM} |
bigint |
8 |
|
-99999999 |
obs.field |
confID |
Multiframe |
WSATransit |
UID of library calibration confidence frame {image extension keyword: CIR_CPM} |
bigint |
8 |
|
-99999999 |
obs.field |
confID |
Multiframe |
WSAUHS |
UID of library calibration confidence frame {image extension keyword: CIR_CPM} |
bigint |
8 |
|
-99999999 |
obs.field |
configIndex |
MultiframeDetector |
WSA |
Configuration index {image extension keyword: CNFINDEX} |
int |
4 |
|
-99999999 |
spect.index |
configIndex |
MultiframeDetector |
WSACalib |
Configuration index {image extension keyword: CNFINDEX} |
int |
4 |
|
-99999999 |
spect.index |
configIndex |
MultiframeDetector |
WSATransit |
Configuration index {image extension keyword: CNFINDEX} |
int |
4 |
|
-99999999 |
spect.index |
configIndex |
MultiframeDetector |
WSAUHS |
Configuration index {image extension keyword: CNFINDEX} |
int |
4 |
|
-99999999 |
spect.index |
confuse_100 |
iras_psc |
IRAS |
Confusion flag (100 micron) |
tinyint |
1 |
|
|
REMARKS |
confuse_12 |
iras_psc |
IRAS |
Confusion flag (12 micron) |
tinyint |
1 |
|
|
REMARKS |
confuse_25 |
iras_psc |
IRAS |
Confusion flag (25 micron) |
tinyint |
1 |
|
|
REMARKS |
confuse_60 |
iras_psc |
IRAS |
Confusion flag (60 micron) |
tinyint |
1 |
|
|
REMARKS |
CONFUSED |
twoxmmi_dr3_v1_0 |
XMM |
This flag (True/False) signifies that the 3-sigma error circle of a detection within this unique source overlaps the 3-sigma error circle of a nearby unique source. As such, it is an indicator of possible confusion (uncertainty) about the assignment of detections between sources. |
varchar |
5 |
|
|
|
CONFUSED |
xmm3dr4 |
XMM |
Normally set 0 (= False), but set 1 (= True) when a given detection has a probability above zero of being associated with two or more distinct sources. The SRCID is that of the match with the highest probability, but there remains some uncertainty about which source is the correct match for the detection. |
bit |
1 |
|
|
|
contam_flg |
twomass_xsc |
2MASS |
contamination flag: 0=no stars, 1=stellar flux incl. in mag. |
smallint |
2 |
|
|
CODE_MISC |
convSegm |
RequiredMosaicTopLevel |
WSAUHS |
Convolution segmentation software |
varchar |
16 |
|
|
|
coord1 |
ExternalSurveyTable |
WSA |
The attribute name of the first (longitudinal) spherical co-ordinate, e.g. equatorial RA |
varchar |
32 |
|
|
?? |
coord1 |
ExternalSurveyTable |
WSACalib |
The attribute name of the first (longitudinal) spherical co-ordinate, e.g. equatorial RA |
varchar |
32 |
|
|
?? |
coord1 |
ExternalSurveyTable |
WSATransit |
The attribute name of the first (longitudinal) spherical co-ordinate, e.g. equatorial RA |
varchar |
32 |
|
|
?? |
coord1 |
ExternalSurveyTable |
WSAUHS |
The attribute name of the first (longitudinal) spherical co-ordinate, e.g. equatorial RA |
varchar |
32 |
|
|
?? |
coord2 |
ExternalSurveyTable |
WSA |
The attribute name of the second (latitudinal) spherical co-ordinate, e.g. equatorial Dec |
varchar |
32 |
|
|
?? |
coord2 |
ExternalSurveyTable |
WSACalib |
The attribute name of the second (latitudinal) spherical co-ordinate, e.g. equatorial Dec |
varchar |
32 |
|
|
?? |
coord2 |
ExternalSurveyTable |
WSATransit |
The attribute name of the second (latitudinal) spherical co-ordinate, e.g. equatorial Dec |
varchar |
32 |
|
|
?? |
coord2 |
ExternalSurveyTable |
WSAUHS |
The attribute name of the second (latitudinal) spherical co-ordinate, e.g. equatorial Dec |
varchar |
32 |
|
|
?? |
coreRadius |
MultiframeDetector |
WSA |
Core radius for default profile fit {catalogue extension keyword: RCORE} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
Tunable parameter, aperture flux designed to match median seeing of survey data. It is straightforward to show that if rcore = FWHM then for typical profiles encountered the rcore flux estimate has between 80-90% of the accuracy of an idealised perfectly known PSF model method. |
coreRadius |
MultiframeDetector |
WSACalib |
Core radius for default profile fit {catalogue extension keyword: RCORE} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
Tunable parameter, aperture flux designed to match median seeing of survey data. It is straightforward to show that if rcore = FWHM then for typical profiles encountered the rcore flux estimate has between 80-90% of the accuracy of an idealised perfectly known PSF model method. |
coreRadius |
MultiframeDetector |
WSATransit |
Core radius for default profile fit {catalogue extension keyword: RCORE} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
Tunable parameter, aperture flux designed to match median seeing of survey data. It is straightforward to show that if rcore = FWHM then for typical profiles encountered the rcore flux estimate has between 80-90% of the accuracy of an idealised perfectly known PSF model method. |
coreRadius |
MultiframeDetector |
WSAUHS |
Core radius for default profile fit {catalogue extension keyword: RCORE} |
real |
4 |
pixels |
-0.9999995e9 |
?? |
Tunable parameter, aperture flux designed to match median seeing of survey data. It is straightforward to show that if rcore = FWHM then for typical profiles encountered the rcore flux estimate has between 80-90% of the accuracy of an idealised perfectly known PSF model method. |
corPlateTemp |
Multiframe |
WSA |
Cor plate temperature {image primary HDU keyword: CP_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
corPlateTemp |
Multiframe |
WSACalib |
Cor plate temperature {image primary HDU keyword: CP_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
corPlateTemp |
Multiframe |
WSATransit |
Cor plate temperature {image primary HDU keyword: CP_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
corPlateTemp |
Multiframe |
WSAUHS |
Cor plate temperature {image primary HDU keyword: CP_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
corr |
tycho2 |
GAIADR1 |
Correlation (ra_deg,de_deg) |
float |
8 |
|
|
stat.correlation |
corrPointingDec |
ProblemFrames |
WSA |
Corrected pointing Declination |
float |
8 |
deg |
|
|
corrPointingDec |
ProblemFrames |
WSAUHS |
Corrected pointing Declination |
float |
8 |
deg |
|
|
corrPointingRa |
ProblemFrames |
WSA |
Corrected pointing Right Ascension |
float |
8 |
deg |
|
|
corrPointingRa |
ProblemFrames |
WSAUHS |
Corrected pointing Right Ascension |
float |
8 |
deg |
|
|
creationDate |
Multiframe |
WSA |
File creation date (YYYY-MM-DD HH:MM:SS) {image primary HDU keyword: DATE} |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
creationDate |
Multiframe |
WSACalib |
File creation date (YYYY-MM-DD HH:MM:SS) {image primary HDU keyword: DATE} |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
creationDate |
Multiframe |
WSATransit |
File creation date (YYYY-MM-DD HH:MM:SS) {image primary HDU keyword: DATE} |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
creationDate |
Multiframe |
WSAUHS |
File creation date (YYYY-MM-DD HH:MM:SS) {image primary HDU keyword: DATE} |
datetime |
8 |
MM-DD-YYYY |
12-31-9999 |
time.epoch |
creationDate |
MultiframeDetector |
WSA |
Creation date/time of file {image extension keyword: DATE} |
datetime |
8 |
MM-DD-YYYY:hh:mm:ss.sss |
12-31-9999 |
?? |
creationDate |
MultiframeDetector |
WSACalib |
Creation date/time of file {image extension keyword: DATE} |
datetime |
8 |
MM-DD-YYYY:hh:mm:ss.sss |
12-31-9999 |
?? |
creationDate |
MultiframeDetector |
WSATransit |
Creation date/time of file {image extension keyword: DATE} |
datetime |
8 |
MM-DD-YYYY:hh:mm:ss.sss |
12-31-9999 |
?? |
creationDate |
MultiframeDetector |
WSAUHS |
Creation date/time of file {image extension keyword: DATE} |
datetime |
8 |
MM-DD-YYYY:hh:mm:ss.sss |
12-31-9999 |
?? |
creator |
ExternalProduct |
WSA |
Name of the individual that created the product |
varchar |
32 |
|
|
?? |
creator |
ExternalProduct |
WSAUHS |
Name of the individual that created the product |
varchar |
32 |
|
|
?? |
crowdedFlag |
MultiframeDetector |
WSA |
Crowded field analysis flag (0 none, 1 active) {catalogue extension keyword: CROWDED} |
tinyint |
1 |
|
0 |
meta.code |
Tunable parameter, detection algorithm tried to disentangle overlapping images or images superposed on the "slowly" varying background of other large images (default) otherwise just straightforward isophotal detection. |
crowdedFlag |
MultiframeDetector |
WSACalib |
Crowded field analysis flag (0 none, 1 active) {catalogue extension keyword: CROWDED} |
tinyint |
1 |
|
0 |
meta.code |
Tunable parameter, detection algorithm tried to disentangle overlapping images or images superposed on the "slowly" varying background of other large images (default) otherwise just straightforward isophotal detection. |
crowdedFlag |
MultiframeDetector |
WSATransit |
Crowded field analysis flag (0 none, 1 active) {catalogue extension keyword: CROWDED} |
tinyint |
1 |
|
0 |
meta.code |
Tunable parameter, detection algorithm tried to disentangle overlapping images or images superposed on the "slowly" varying background of other large images (default) otherwise just straightforward isophotal detection. |
crowdedFlag |
MultiframeDetector |
WSAUHS |
Crowded field analysis flag (0 none, 1 active) {catalogue extension keyword: CROWDED} |
tinyint |
1 |
|
0 |
meta.code |
Tunable parameter, detection algorithm tried to disentangle overlapping images or images superposed on the "slowly" varying background of other large images (default) otherwise just straightforward isophotal detection. |
crPixX |
CurrentAstrometry |
WSACalib |
Pixel coordinate of the reference point on axis 1 {image extension keyword: CRPIX1} |
float |
8 |
pixels |
|
pos.cartesian.x;instr.det |
crPixX |
CurrentAstrometry |
WSATransit |
Pixel coordinate of the reference point on axis 1 {image extension keyword: CRPIX1} |
float |
8 |
pixels |
|
pos.cartesian.x;instr.det |
crPixX |
CurrentAstrometry |
WSAUHS |
Pixel coordinate of the reference point on axis 1 {image extension keyword: CRPIX1} |
float |
8 |
pixels |
|
pos.cartesian.x;instr.det |
crPixX |
CurrentAstrometry, PreviousAstrometry |
WSA |
Pixel coordinate of the reference point on axis 1 {image extension keyword: CRPIX1} |
float |
8 |
pixels |
|
pos.cartesian.x;instr.det |
crPixY |
CurrentAstrometry |
WSACalib |
Pixel coordinate of the reference point on axis 2 {image extension keyword: CRPIX2} |
float |
8 |
pixels |
|
pos.cartesian.y;instr.det |
crPixY |
CurrentAstrometry |
WSATransit |
Pixel coordinate of the reference point on axis 2 {image extension keyword: CRPIX2} |
float |
8 |
pixels |
|
pos.cartesian.y;instr.det |
crPixY |
CurrentAstrometry |
WSAUHS |
Pixel coordinate of the reference point on axis 2 {image extension keyword: CRPIX2} |
float |
8 |
pixels |
|
pos.cartesian.y;instr.det |
crPixY |
CurrentAstrometry, PreviousAstrometry |
WSA |
Pixel coordinate of the reference point on axis 2 {image extension keyword: CRPIX2} |
float |
8 |
pixels |
|
pos.cartesian.y;instr.det |
crUnit1 |
CurrentAstrometry |
WSACalib |
Unit of right ascension co-ordinates {image extension keyword: CRUNIT1} |
varchar |
8 |
|
NONE |
|
crUnit1 |
CurrentAstrometry |
WSATransit |
Unit of right ascension co-ordinates {image extension keyword: CRUNIT1} |
varchar |
8 |
|
NONE |
|
crUnit1 |
CurrentAstrometry |
WSAUHS |
Unit of right ascension co-ordinates {image extension keyword: CRUNIT1} |
varchar |
8 |
|
NONE |
|
crUnit1 |
CurrentAstrometry, PreviousAstrometry |
WSA |
Unit of right ascension co-ordinates {image extension keyword: CRUNIT1} |
varchar |
8 |
|
NONE |
|
crUnit2 |
CurrentAstrometry |
WSACalib |
Unit of declination co-ordinates {image extension keyword: CRUNIT2} |
varchar |
8 |
|
NONE |
|
crUnit2 |
CurrentAstrometry |
WSATransit |
Unit of declination co-ordinates {image extension keyword: CRUNIT2} |
varchar |
8 |
|
NONE |
|
crUnit2 |
CurrentAstrometry |
WSAUHS |
Unit of declination co-ordinates {image extension keyword: CRUNIT2} |
varchar |
8 |
|
NONE |
|
crUnit2 |
CurrentAstrometry, PreviousAstrometry |
WSA |
Unit of declination co-ordinates {image extension keyword: CRUNIT2} |
varchar |
8 |
|
NONE |
|
crValX |
CurrentAstrometry |
WSACalib |
Coordinate value at reference point on axis 1 {image extension keyword: CRVAL1} |
float |
8 |
|
-0.9999995e9 |
pos.cartesian.x;instr.det |
crValX |
CurrentAstrometry |
WSATransit |
Coordinate value at reference point on axis 1 {image extension keyword: CRVAL1} |
float |
8 |
|
-0.9999995e9 |
pos.cartesian.x;instr.det |
crValX |
CurrentAstrometry |
WSAUHS |
Coordinate value at reference point on axis 1 {image extension keyword: CRVAL1} |
float |
8 |
|
-0.9999995e9 |
pos.cartesian.x;instr.det |
crValX |
CurrentAstrometry, PreviousAstrometry |
WSA |
Coordinate value at reference point on axis 1 {image extension keyword: CRVAL1} |
float |
8 |
|
-0.9999995e9 |
pos.cartesian.x;instr.det |
crValY |
CurrentAstrometry |
WSACalib |
Coordinate value at reference point on axis 2 {image extension keyword: CRVAL2} |
float |
8 |
|
-0.9999995e9 |
pos.cartesian.y;instr.det |
crValY |
CurrentAstrometry |
WSATransit |
Coordinate value at reference point on axis 2 {image extension keyword: CRVAL2} |
float |
8 |
|
-0.9999995e9 |
pos.cartesian.y;instr.det |
crValY |
CurrentAstrometry |
WSAUHS |
Coordinate value at reference point on axis 2 {image extension keyword: CRVAL2} |
float |
8 |
|
-0.9999995e9 |
pos.cartesian.y;instr.det |
crValY |
CurrentAstrometry, PreviousAstrometry |
WSA |
Coordinate value at reference point on axis 2 {image extension keyword: CRVAL2} |
float |
8 |
|
-0.9999995e9 |
pos.cartesian.y;instr.det |
cryostPres |
Multiframe |
WSA |
Cryostat Pressure {image primary HDU keyword: CC_PRES} |
float |
8 |
millibar |
-0.9999995e9 |
|
cryostPres |
Multiframe |
WSACalib |
Cryostat Pressure {image primary HDU keyword: CC_PRES} |
float |
8 |
millibar |
-0.9999995e9 |
|
cryostPres |
Multiframe |
WSATransit |
Cryostat Pressure {image primary HDU keyword: CC_PRES} |
float |
8 |
millibar |
-0.9999995e9 |
|
cryostPres |
Multiframe |
WSAUHS |
Cryostat Pressure {image primary HDU keyword: CC_PRES} |
float |
8 |
millibar |
-0.9999995e9 |
|
cTypeX |
CurrentAstrometry |
WSACalib |
G&C WCS type, eg 'RA---ZPN' {image extension keyword: CTYPE1} |
varchar |
8 |
|
|
pos.eq.ra;meta.main |
cTypeX |
CurrentAstrometry |
WSATransit |
G&C WCS type, eg 'RA---ZPN' {image extension keyword: CTYPE1} |
varchar |
8 |
|
|
pos.eq.ra;meta.main |
cTypeX |
CurrentAstrometry |
WSAUHS |
G&C WCS type, eg 'RA---ZPN' {image extension keyword: CTYPE1} |
varchar |
8 |
|
|
pos.eq.ra;meta.main |
cTypeX |
CurrentAstrometry, PreviousAstrometry |
WSA |
G&C WCS type, eg 'RA---ZPN' {image extension keyword: CTYPE1} |
varchar |
8 |
|
|
pos.eq.ra;meta.main |
cTypeY |
CurrentAstrometry |
WSACalib |
G&C WCS type, eg 'DEC--ZPN' {image extension keyword: CTYPE2} |
varchar |
8 |
|
|
pos.eq.dec;meta.main |
cTypeY |
CurrentAstrometry |
WSATransit |
G&C WCS type, eg 'DEC--ZPN' {image extension keyword: CTYPE2} |
varchar |
8 |
|
|
pos.eq.dec;meta.main |
cTypeY |
CurrentAstrometry |
WSAUHS |
G&C WCS type, eg 'DEC--ZPN' {image extension keyword: CTYPE2} |
varchar |
8 |
|
|
pos.eq.dec;meta.main |
cTypeY |
CurrentAstrometry, PreviousAstrometry |
WSA |
G&C WCS type, eg 'DEC--ZPN' {image extension keyword: CTYPE2} |
varchar |
8 |
|
|
pos.eq.dec;meta.main |
cuEventID |
ArchiveCurationHistory |
WSACalib |
UID of curation event giving rise to this record |
int |
4 |
|
|
meta.bib |
cuEventID |
ArchiveCurationHistory |
WSATransit |
UID of curation event giving rise to this record |
int |
4 |
|
|
meta.bib |
cuEventID |
ArchiveCurationHistory |
WSAUHS |
UID of curation event giving rise to this record |
int |
4 |
|
|
meta.bib |
cuEventID |
ArchiveCurationHistory, AstrCalVers, CurrentAstrometry, EpochFrameStatus, lasMapRemeasAver, lasMapRemeasurement, lasYselJRemeasMergeLog, lasYselJSourceRemeasurement, MapApertureIDslasYselJ, MapProvenance, Multiframe, MultiframeDetector, PhotCalVers, PreviousAstrometry, ProgrammeCurationHistory, ProgrammeFrame, Provenance |
WSA |
UID of curation event giving rise to this record |
int |
4 |
|
|
meta.bib |
cuEventID |
MapFrameStatus |
WSA |
UID of curation event giving rise to this record |
int |
4 |
|
-99999999 |
REFER_CODE |
cuEventID |
MapFrameStatus |
WSAUHS |
UID of curation event giving rise to this record |
int |
4 |
|
-99999999 |
REFER_CODE |
cuEventID |
dxsAstrometricInfo, dxsDetection, dxsJKmergeLog, dxsJKsource, dxsMergeLog, dxsOrphan, dxsSource, dxsSourceXDetectionBestMatch, dxsVarFrameSetInfo, dxsVariability, gcsAstrometricInfo, gcsDetection, gcsMergeLog, gcsOrphan, gcsPointSource, gcsSource, gcsSourceXDetectionBestMatch, gcsVarFrameSetInfo, gcsVariability, gcsZYJHKmergeLog, gcsZYJHKsource, gpsAstrometricInfo, gpsDetection, gpsJHKmergeLog, gpsJHKsource, gpsMergeLog, gpsOrphan, gpsPointSource, gpsSource, gpsSourceXDetectionBestMatch, gpsVarFrameSetInfo, gpsVariability, lasAstrometricInfo, lasDetection, lasExtendedSource, lasMergeLog, lasOrphan, lasPointSource, lasSource, lasSourceXDetectionBestMatch, lasVarFrameSetInfo, lasVariability, lasYJHKmergeLog, lasYJHKsource, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, UKIDSSDetection, udsAstrometricInfo, udsDetection, udsMergeLog, udsOrphan, udsSource, udsSourceXDetectionBestMatch, udsVarFrameSetInfo, udsVariability |
WSA |
UID of curation event giving rise to this record |
int |
4 |
|
|
REFER_CODE |
cuEventID |
calDetection, calMergeLog, calSource, calSourceXSynopticSourceBestMatch, calSynopticMergeLog, calSynopticSource, calVarFrameSetInfo, calVariability |
WSACalib |
UID of curation event giving rise to this record |
int |
4 |
|
|
REFER_CODE |
cuEventID |
ptsDetection |
WSATransit |
UID of curation event giving rise to this record |
int |
4 |
|
|
REFER_CODE |
cuEventID |
uhsAstrometricInfo, uhsDetection, uhsDetectionAll, uhsMergeLog, uhsOrphan, uhsSource, uhsSourceAll, uhsSourceXDetectionBestMatch, uhsVarFrameSetInfo, uhsVariability |
WSAUHS |
UID of curation event giving rise to this record |
int |
4 |
|
|
REFER_CODE |
cuID |
ArchiveCurationHistory |
WSACalib |
the unique curation task ID |
smallint |
2 |
|
|
meta.bib |
cuID |
ArchiveCurationHistory |
WSATransit |
the unique curation task ID |
smallint |
2 |
|
|
meta.bib |
cuID |
ArchiveCurationHistory |
WSAUHS |
the unique curation task ID |
smallint |
2 |
|
|
meta.bib |
cuID |
ArchiveCurationHistory, CurationTask |
WSA |
the unique curation task ID |
smallint |
2 |
|
|
meta.bib |
curator |
ArchiveCurationHistory |
WSA |
The archive curation scientist responsible for this event |
varchar |
16 |
|
|
?? |
curator |
ArchiveCurationHistory |
WSACalib |
The archive curation scientist responsible for this event |
varchar |
16 |
|
|
?? |
curator |
ArchiveCurationHistory |
WSATransit |
The archive curation scientist responsible for this event |
varchar |
16 |
|
|
?? |
curator |
ArchiveCurationHistory |
WSAUHS |
The archive curation scientist responsible for this event |
varchar |
16 |
|
|
?? |
cutOff |
Filter |
WSA |
The 50% cut-off wavelength of the filter |
real |
4 |
microns |
|
?? |
cutOff |
Filter |
WSACalib |
The 50% cut-off wavelength of the filter |
real |
4 |
microns |
|
?? |
cutOff |
Filter |
WSATransit |
The 50% cut-off wavelength of the filter |
real |
4 |
microns |
|
?? |
cutOff |
Filter |
WSAUHS |
The 50% cut-off wavelength of the filter |
real |
4 |
microns |
|
?? |
cutOn |
Filter |
WSA |
The 50% cut-on wavelength of the filter |
real |
4 |
microns |
|
?? |
cutOn |
Filter |
WSACalib |
The 50% cut-on wavelength of the filter |
real |
4 |
microns |
|
?? |
cutOn |
Filter |
WSATransit |
The 50% cut-on wavelength of the filter |
real |
4 |
microns |
|
?? |
cutOn |
Filter |
WSAUHS |
The 50% cut-on wavelength of the filter |
real |
4 |
microns |
|
?? |
CX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
CurrentAstrometry |
WSACalib |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
cx |
CurrentAstrometry |
WSATransit |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
cx |
CurrentAstrometry |
WSAUHS |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
cx |
CurrentAstrometry, PreviousAstrometry |
WSA |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
cx |
ObjectThin |
PS1DR2 |
Cartesian x on a unit sphere. |
float |
8 |
|
|
pos.cartesian.x;pos.eq |
cx |
dxsDetection, dxsJKmergeLog, dxsJKsource, dxsMergeLog, dxsSource, gcsDetection, gcsMergeLog, gcsPointSource, gcsSource, gcsZYJHKmergeLog, gcsZYJHKsource, gpsDetection, gpsJHKmergeLog, gpsJHKsource, gpsMergeLog, gpsPointSource, gpsSource, lasDetection, lasExtendedSource, lasMergeLog, lasPointSource, lasSource, lasYJHKmergeLog, lasYJHKsource, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, UKIDSSDetection, udsDetection, udsMergeLog, udsSource |
WSA |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
calDetection, calMergeLog, calSource, calSynopticMergeLog, calSynopticSource |
WSACalib |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
catwise_2020, catwise_prelim |
WISE |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
gaia_source |
GAIADR2 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
cx |
gaia_source |
GAIAEDR3 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
cx |
gaia_source, hipparcos_new_reduction, igsl_source, tgas_source, tycho2 |
GAIADR1 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
cx |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca, glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
iras_psc |
IRAS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
lasMapRemeasAver, lasMapRemeasurement, lasYselJRemeasMergeLog |
WSA |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.x |
cx |
lasYselJSourceRemeasurement |
WSA |
unit vector of spherical co-ordinates of aperture |
float |
8 |
|
|
pos.cartesian.x;pos.eq |
cx |
mgcDetection |
MGC |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
nvssSource |
NVSS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
ptsDetection |
WSATransit |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
rosat_bsc, rosat_fsc |
ROSAT |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
twomass_psc, twomass_scn, twomass_sixx2_psc, twomass_sixx2_scn, twomass_sixx2_xsc, twomass_xsc |
2MASS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
twompzPhotoz |
TWOMPZ |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.x;pos.eq |
cx |
uhsDetection, uhsDetectionAll, uhsMergeLog, uhsSource, uhsSourceAll |
WSAUHS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
wiseScosPhotoz, wiseScosPhotozRejects, wiseScosSvm |
WISExSCOSPZ |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.x;pos.eq |
cx |
wise_allskysc, wise_prelimsc |
WISE |
unit vector of spherical co-ordinates (similar to x in IPAC IRSA schema, but recomputed) |
float |
8 |
|
|
POS_EQ_X |
CY |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
CurrentAstrometry |
WSACalib |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
cy |
CurrentAstrometry |
WSATransit |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
cy |
CurrentAstrometry |
WSAUHS |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
cy |
CurrentAstrometry, PreviousAstrometry |
WSA |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
cy |
ObjectThin |
PS1DR2 |
Cartesian y on a unit sphere. |
float |
8 |
|
|
pos.cartesian.y;pos.eq |
cy |
dxsDetection, dxsJKmergeLog, dxsJKsource, dxsMergeLog, dxsSource, gcsDetection, gcsMergeLog, gcsPointSource, gcsSource, gcsZYJHKmergeLog, gcsZYJHKsource, gpsDetection, gpsJHKmergeLog, gpsJHKsource, gpsMergeLog, gpsPointSource, gpsSource, lasDetection, lasExtendedSource, lasMergeLog, lasPointSource, lasSource, lasYJHKmergeLog, lasYJHKsource, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, UKIDSSDetection, udsDetection, udsMergeLog, udsSource |
WSA |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
calDetection, calMergeLog, calSource, calSynopticMergeLog, calSynopticSource |
WSACalib |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
catwise_2020, catwise_prelim |
WISE |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
gaia_source |
GAIADR2 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
cy |
gaia_source |
GAIAEDR3 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
cy |
gaia_source, hipparcos_new_reduction, igsl_source, tgas_source, tycho2 |
GAIADR1 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
cy |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca, glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
iras_psc |
IRAS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
lasMapRemeasAver, lasMapRemeasurement, lasYselJRemeasMergeLog |
WSA |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.y |
cy |
lasYselJSourceRemeasurement |
WSA |
unit vector of spherical co-ordinates of aperture |
float |
8 |
|
|
pos.cartesian.y;pos.eq |
cy |
mgcDetection |
MGC |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
nvssSource |
NVSS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
ptsDetection |
WSATransit |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
rosat_bsc, rosat_fsc |
ROSAT |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
twomass_psc, twomass_scn, twomass_sixx2_psc, twomass_sixx2_scn, twomass_sixx2_xsc, twomass_xsc |
2MASS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
twompzPhotoz |
TWOMPZ |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.y;pos.eq |
cy |
uhsDetection, uhsDetectionAll, uhsMergeLog, uhsSource, uhsSourceAll |
WSAUHS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
wiseScosPhotoz, wiseScosPhotozRejects, wiseScosSvm |
WISExSCOSPZ |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.y;pos.eq |
cy |
wise_allskysc, wise_prelimsc |
WISE |
unit vector of spherical co-ordinates (similar to y in IPAC IRSA schema, but recomputed) |
float |
8 |
|
|
POS_EQ_Y |
CZ |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0, xmm3dr4 |
XMM |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
CurrentAstrometry |
WSACalib |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.z |
cz |
CurrentAstrometry |
WSATransit |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.z |
cz |
CurrentAstrometry |
WSAUHS |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.z |
cz |
CurrentAstrometry, PreviousAstrometry |
WSA |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
pos.distance;pos.cartesian.z |
cz |
ObjectThin |
PS1DR2 |
Cartesian z on a unit sphere. |
float |
8 |
|
|
pos.cartesian.y;pos.eq |
cz |
dxsDetection, dxsJKmergeLog, dxsJKsource, dxsMergeLog, dxsSource, gcsDetection, gcsMergeLog, gcsPointSource, gcsSource, gcsZYJHKmergeLog, gcsZYJHKsource, gpsDetection, gpsJHKmergeLog, gpsJHKsource, gpsMergeLog, gpsPointSource, gpsSource, lasDetection, lasExtendedSource, lasMergeLog, lasPointSource, lasSource, lasYJHKmergeLog, lasYJHKsource, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, UKIDSSDetection, udsDetection, udsMergeLog, udsSource |
WSA |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
calDetection, calMergeLog, calSource, calSynopticMergeLog, calSynopticSource |
WSACalib |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
catwise_2020, catwise_prelim |
WISE |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
first08Jul16Source, firstSource, firstSource12Feb16 |
FIRST |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
gaia_source |
GAIADR2 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.z |
cz |
gaia_source |
GAIAEDR3 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.z |
cz |
gaia_source, hipparcos_new_reduction, igsl_source, tgas_source, tycho2 |
GAIADR1 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.z |
cz |
glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca, glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
iras_psc |
IRAS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
lasMapRemeasAver, lasMapRemeasurement, lasYselJRemeasMergeLog |
WSA |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.z |
cz |
lasYselJSourceRemeasurement |
WSA |
unit vector of spherical co-ordinates of aperture |
float |
8 |
|
|
pos.cartesian.z;pos.eq |
cz |
mgcDetection |
MGC |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
nvssSource |
NVSS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
ptsDetection |
WSATransit |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
rosat_bsc, rosat_fsc |
ROSAT |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
twomass_psc, twomass_scn, twomass_sixx2_psc, twomass_sixx2_scn, twomass_sixx2_xsc, twomass_xsc |
2MASS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
twompzPhotoz |
TWOMPZ |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.z;pos.eq |
cz |
uhsDetection, uhsDetectionAll, uhsMergeLog, uhsSource, uhsSourceAll |
WSAUHS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
wiseScosPhotoz, wiseScosPhotozRejects, wiseScosSvm |
WISExSCOSPZ |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.z;pos.eq |
cz |
wise_allskysc, wise_prelimsc |
WISE |
unit vector of spherical co-ordinates (similar to z in IPAC IRSA schema, but recomputed) |
float |
8 |
|
|
POS_EQ_Z |