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 |
|
|
ID_PLATE |
camNum |
MultiframeDetector |
WSACalib |
Number of WFCAM camera (1, 2, 3 or 4) {image extension keyword: CAMNUM} |
int |
4 |
|
|
ID_PLATE |
camNum |
MultiframeDetector |
WSATransit |
Number of WFCAM camera (1, 2, 3 or 4) {image extension keyword: CAMNUM} |
int |
4 |
|
|
ID_PLATE |
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 |
|
--- |
?? |
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 |
|
--- |
?? |
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 |
?? |
cat |
twomass_sixx2_psc, twomass_sixx2_scn, twomass_sixx2_xsc |
2MASS |
Catalog indicator 1=catalog, 0=not catalog |
smallint |
2 |
|
|
|
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 |
|
|
?? |
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 |
?? |
catName |
Multiframe |
WSA |
the filename of the associated catalogue MEF, eg. server:/path/filename.fits |
varchar |
256 |
|
|
ID_CATALOG |
catName |
Multiframe |
WSACalib |
the filename of the associated catalogue MEF, eg. server:/path/filename.fits |
varchar |
256 |
|
|
ID_CATALOG |
catName |
Multiframe |
WSATransit |
the filename of the associated catalogue MEF, eg. server:/path/filename.fits |
varchar |
256 |
|
|
ID_CATALOG |
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_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 |
|
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 |
|
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 |
|
cd11 |
CurrentAstrometry |
WSACalib |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_1} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd11 |
CurrentAstrometry |
WSATransit |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_1} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd11 |
CurrentAstrometry, PreviousAstrometry |
WSA |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_1} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd12 |
CurrentAstrometry |
WSACalib |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_2} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd12 |
CurrentAstrometry |
WSATransit |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_2} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd12 |
CurrentAstrometry, PreviousAstrometry |
WSA |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_2} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd21 |
CurrentAstrometry |
WSACalib |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_1} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd21 |
CurrentAstrometry |
WSATransit |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_1} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd21 |
CurrentAstrometry, PreviousAstrometry |
WSA |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_1} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd22 |
CurrentAstrometry |
WSACalib |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_2} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd22 |
CurrentAstrometry |
WSATransit |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_2} |
float |
8 |
|
|
POS_TRANSF_PARAM |
cd22 |
CurrentAstrometry, PreviousAstrometry |
WSA |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_2} |
float |
8 |
|
|
POS_TRANSF_PARAM |
centralDec |
CurrentAstrometry |
WSACalib |
Dec (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
centralDec |
CurrentAstrometry |
WSATransit |
Dec (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
centralDec |
CurrentAstrometry, PreviousAstrometry |
WSA |
Dec (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
centralRa |
CurrentAstrometry |
WSACalib |
RA (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_RA_MAIN |
centralRa |
CurrentAstrometry |
WSATransit |
RA (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_RA_MAIN |
centralRa |
CurrentAstrometry, PreviousAstrometry |
WSA |
RA (J2000) at device centre |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_RA_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, 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 |
chi2s |
dxsAstrometricInfo, udsAstrometricInfo |
WSA |
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 |
INST_BACKGROUND |
CIR_BVAR |
MultiframeDetector |
WSACalib |
Latest estimate of background variance {image extension keyword: CIR_BVAR} |
real |
4 |
|
-0.9999995e9 |
INST_BACKGROUND |
CIR_BVAR |
MultiframeDetector |
WSATransit |
Latest estimate of background variance {image extension keyword: CIR_BVAR} |
real |
4 |
|
-0.9999995e9 |
INST_BACKGROUND |
CIR_SCAL |
MultiframeDetector |
WSA |
Background scale relative to group maximum {image extension keyword: CIR_SCAL} |
real |
4 |
|
-0.9999995e9 |
INST_BACKGROUND |
CIR_SCAL |
MultiframeDetector |
WSACalib |
Background scale relative to group maximum {image extension keyword: CIR_SCAL} |
real |
4 |
|
-0.9999995e9 |
INST_BACKGROUND |
CIR_SCAL |
MultiframeDetector |
WSATransit |
Background scale relative to group maximum {image extension keyword: CIR_SCAL} |
real |
4 |
|
-0.9999995e9 |
INST_BACKGROUND |
CIR_ZERO |
MultiframeDetector |
WSA |
Pedestal value relative to group average {image extension keyword: CIR_ZERO} |
real |
4 |
|
-0.9999995e9 |
FIT_PARAM_VALUE |
CIR_ZERO |
MultiframeDetector |
WSACalib |
Pedestal value relative to group average {image extension keyword: CIR_ZERO} |
real |
4 |
|
-0.9999995e9 |
FIT_PARAM_VALUE |
CIR_ZERO |
MultiframeDetector |
WSATransit |
Pedestal value relative to group average {image extension keyword: CIR_ZERO} |
real |
4 |
|
-0.9999995e9 |
FIT_PARAM_VALUE |
CIRMED |
MultiframeDetector |
WSA |
Latest estimate of background {image extension keyword: CIRMED} |
real |
4 |
|
-0.9999995e9 |
INST_BACKGROUND |
CIRMED |
MultiframeDetector |
WSACalib |
Latest estimate of background {image extension keyword: CIRMED} |
real |
4 |
|
-0.9999995e9 |
INST_BACKGROUND |
CIRMED |
MultiframeDetector |
WSATransit |
Latest estimate of background {image extension keyword: CIRMED} |
real |
4 |
|
-0.9999995e9 |
INST_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, calListRemeasurement |
WSACalib |
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 |
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 |
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 |
dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement |
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 |
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 boderline 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. |
classStat |
UKIDSSDetection |
WSA |
N(0,1) stellarness-of-profile statistic |
real |
4 |
|
|
STAT_PROP |
classStat |
calDetection, calListRemeasurement |
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, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement |
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 |
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. |
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 |
twomass_sixx2_scn, twomass_sixx2_xsc |
2MASS |
entry counter (key) number (unique within table) |
int |
4 |
|
|
|
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_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 |
combiframeID |
Provenance |
WSA |
the UID of the combined frame (=combiframe) |
bigint |
8 |
|
|
ID_FRAME |
combiframeID |
Provenance |
WSACalib |
the UID of the combined frame (=combiframe) |
bigint |
8 |
|
|
ID_FRAME |
combiframeID |
Provenance |
WSATransit |
the UID of the combined frame (=combiframe) |
bigint |
8 |
|
|
ID_FRAME |
combiProdType |
ProductLinks |
WSA |
Type (stack,tile,mosaic) of combination frame |
varchar |
8 |
|
|
?? |
combiProductID |
ProductLinks |
WSA |
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 |
|
|
?? |
compFile |
MultiframeDetector |
WSA |
Filename of the compressed image of this image frame, eg. server:/path/filename.jpg |
varchar |
256 |
|
NONE |
ID_FILE |
compFile |
MultiframeDetector |
WSACalib |
Filename of the compressed image of this image frame, eg. server:/path/filename.jpg |
varchar |
256 |
|
NONE |
ID_FILE |
compFile |
MultiframeDetector |
WSATransit |
Filename of the compressed image of this image frame, eg. server:/path/filename.jpg |
varchar |
256 |
|
NONE |
ID_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 |
ID_FRAME |
confID |
Multiframe |
WSACalib |
UID of library calibration confidence frame {image extension keyword: CIR_CPM} |
bigint |
8 |
|
-99999999 |
ID_FRAME |
confID |
Multiframe |
WSATransit |
UID of library calibration confidence frame {image extension keyword: CIR_CPM} |
bigint |
8 |
|
-99999999 |
ID_FRAME |
configIndex |
MultiframeDetector |
WSA |
Configuration index {image extension keyword: CNFINDEX} |
int |
4 |
|
-99999999 |
SPECT_INDEX_MISC |
configIndex |
MultiframeDetector |
WSACalib |
Configuration index {image extension keyword: CNFINDEX} |
int |
4 |
|
-99999999 |
SPECT_INDEX_MISC |
configIndex |
MultiframeDetector |
WSATransit |
Configuration index {image extension keyword: CNFINDEX} |
int |
4 |
|
-99999999 |
SPECT_INDEX_MISC |
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 |
|
|
|
contam_flg |
twomass_xsc |
2MASS |
contamination flag: 0=no stars, 1=stellar flux incl. in mag. |
smallint |
2 |
|
|
CODE_MISC |
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 |
|
|
?? |
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 |
|
|
?? |
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. |
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 |
|
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_DATE |
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_DATE |
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_DATE |
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 |
?? |
crowdedFlag |
MultiframeDetector |
WSA |
Crowded field analysis flag (0 none, 1 active) {catalogue extension keyword: CROWDED} |
tinyint |
1 |
|
0 |
CODE_MISC |
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 |
CODE_MISC |
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 |
CODE_MISC |
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_CCD_X |
crPixX |
CurrentAstrometry |
WSATransit |
Pixel coordinate of the reference point on axis 1 {image extension keyword: CRPIX1} |
float |
8 |
pixels |
|
POS_CCD_X |
crPixX |
CurrentAstrometry, PreviousAstrometry |
WSA |
Pixel coordinate of the reference point on axis 1 {image extension keyword: CRPIX1} |
float |
8 |
pixels |
|
POS_CCD_X |
crPixY |
CurrentAstrometry |
WSACalib |
Pixel coordinate of the reference point on axis 2 {image extension keyword: CRPIX2} |
float |
8 |
pixels |
|
POS_CCD_Y |
crPixY |
CurrentAstrometry |
WSATransit |
Pixel coordinate of the reference point on axis 2 {image extension keyword: CRPIX2} |
float |
8 |
pixels |
|
POS_CCD_Y |
crPixY |
CurrentAstrometry, PreviousAstrometry |
WSA |
Pixel coordinate of the reference point on axis 2 {image extension keyword: CRPIX2} |
float |
8 |
pixels |
|
POS_CCD_Y |
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, 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, 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_CCD_X |
crValX |
CurrentAstrometry |
WSATransit |
Coordinate value at reference point on axis 1 {image extension keyword: CRVAL1} |
float |
8 |
|
-0.9999995e9 |
POS_CCD_X |
crValX |
CurrentAstrometry, PreviousAstrometry |
WSA |
Coordinate value at reference point on axis 1 {image extension keyword: CRVAL1} |
float |
8 |
|
-0.9999995e9 |
POS_CCD_X |
crValY |
CurrentAstrometry |
WSACalib |
Coordinate value at reference point on axis 2 {image extension keyword: CRVAL2} |
float |
8 |
|
-0.9999995e9 |
POS_CCD_Y |
crValY |
CurrentAstrometry |
WSATransit |
Coordinate value at reference point on axis 2 {image extension keyword: CRVAL2} |
float |
8 |
|
-0.9999995e9 |
POS_CCD_Y |
crValY |
CurrentAstrometry, PreviousAstrometry |
WSA |
Coordinate value at reference point on axis 2 {image extension keyword: CRVAL2} |
float |
8 |
|
-0.9999995e9 |
POS_CCD_Y |
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 |
|
cTypeX |
CurrentAstrometry |
WSACalib |
G&C WCS type, eg 'RA---ZPN' {image extension keyword: CTYPE1} |
varchar |
8 |
|
|
POS_EQ_RA_MAIN |
cTypeX |
CurrentAstrometry |
WSATransit |
G&C WCS type, eg 'RA---ZPN' {image extension keyword: CTYPE1} |
varchar |
8 |
|
|
POS_EQ_RA_MAIN |
cTypeX |
CurrentAstrometry, PreviousAstrometry |
WSA |
G&C WCS type, eg 'RA---ZPN' {image extension keyword: CTYPE1} |
varchar |
8 |
|
|
POS_EQ_RA_MAIN |
cTypeY |
CurrentAstrometry |
WSACalib |
G&C WCS type, eg 'DEC--ZPN' {image extension keyword: CTYPE2} |
varchar |
8 |
|
|
POS_EQ_DEC_MAIN |
cTypeY |
CurrentAstrometry |
WSATransit |
G&C WCS type, eg 'DEC--ZPN' {image extension keyword: CTYPE2} |
varchar |
8 |
|
|
POS_EQ_DEC_MAIN |
cTypeY |
CurrentAstrometry, PreviousAstrometry |
WSA |
G&C WCS type, eg 'DEC--ZPN' {image extension keyword: CTYPE2} |
varchar |
8 |
|
|
POS_EQ_DEC_MAIN |
cuEventID |
ArchiveCurationHistory, AstrCalVers, CurrentAstrometry, dxsAstrometricInfo, dxsDetection, dxsJKmergeLog, dxsJKsource, dxsListRemeasurement, dxsMergeLog, dxsSource, dxsSourceRemeasurement, dxsSourceXDetectionBestMatch, dxsVarFrameSetInfo, dxsVariability, gcsDetection, gcsListRemeasurement, gcsMergeLog, gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKmergeLog, gcsZYJHKsource, gpsDetection, gpsJHKmergeLog, gpsJHKsource, gpsListRemeasurement, gpsMergeLog, gpsPointSource, gpsSource, gpsSourceRemeasurement, lasDetection, lasExtendedSource, lasListRemeasurement, lasMergeLog, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKmergeLog, lasYJHKsource, Multiframe, MultiframeDetector, PhotCalVers, PreviousAstrometry, ProgrammeCurationHistory, ProgrammeFrame, Provenance, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, UKIDSSDetection, udsAstrometricInfo, udsDetection, udsListRemeasurement, udsMergeLog, udsSource, udsSourceRemeasurement, udsSourceXDetectionBestMatch, udsVarFrameSetInfo, udsVariability |
WSA |
UID of curation event giving rise to this record |
int |
4 |
|
|
REFER_CODE |
cuEventID |
ArchiveCurationHistory, calDetection, calListRemeasurement, calMergeLog, calSource, calSourceRemeasurement, calSourceXSynopticSourceBestMatch, calSynopticMergeLog, calSynopticSource, calVarFrameSetInfo, calVariability |
WSACalib |
UID of curation event giving rise to this record |
int |
4 |
|
|
REFER_CODE |
cuEventID |
ArchiveCurationHistory, ptsDetection |
WSATransit |
UID of curation event giving rise to this record |
int |
4 |
|
|
REFER_CODE |
cuID |
ArchiveCurationHistory |
WSACalib |
the unique curation task ID |
smallint |
2 |
|
|
REFER_CODE |
cuID |
ArchiveCurationHistory |
WSATransit |
the unique curation task ID |
smallint |
2 |
|
|
REFER_CODE |
cuID |
ArchiveCurationHistory, CurationTask |
WSA |
the unique curation task ID |
smallint |
2 |
|
|
REFER_CODE |
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 |
|
|
?? |
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 |
|
?? |
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 |
|
?? |
CX |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
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_EQ_X |
cx |
CurrentAstrometry |
WSATransit |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
POS_EQ_X |
cx |
CurrentAstrometry, PreviousAstrometry |
WSA |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
POS_EQ_X |
cx |
dxsDetection, dxsJKmergeLog, dxsJKsource, dxsListRemeasurement, dxsMergeLog, dxsSource, dxsSourceRemeasurement, gcsDetection, gcsListRemeasurement, gcsMergeLog, gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKmergeLog, gcsZYJHKsource, gpsDetection, gpsJHKmergeLog, gpsJHKsource, gpsListRemeasurement, gpsMergeLog, gpsPointSource, gpsSource, gpsSourceRemeasurement, lasDetection, lasExtendedSource, lasListRemeasurement, lasMergeLog, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKmergeLog, lasYJHKsource, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, UKIDSSDetection, udsDetection, udsListRemeasurement, udsMergeLog, udsSource, udsSourceRemeasurement |
WSA |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
calDetection, calListRemeasurement, calMergeLog, calSource, calSourceRemeasurement, calSynopticMergeLog, calSynopticSource |
WSACalib |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_X |
cx |
first08Jul16Source, firstSource |
FIRST |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_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 |
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 |
CY |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
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_EQ_Y |
cy |
CurrentAstrometry |
WSATransit |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
POS_EQ_Y |
cy |
CurrentAstrometry, PreviousAstrometry |
WSA |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
POS_EQ_Y |
cy |
dxsDetection, dxsJKmergeLog, dxsJKsource, dxsListRemeasurement, dxsMergeLog, dxsSource, dxsSourceRemeasurement, gcsDetection, gcsListRemeasurement, gcsMergeLog, gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKmergeLog, gcsZYJHKsource, gpsDetection, gpsJHKmergeLog, gpsJHKsource, gpsListRemeasurement, gpsMergeLog, gpsPointSource, gpsSource, gpsSourceRemeasurement, lasDetection, lasExtendedSource, lasListRemeasurement, lasMergeLog, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKmergeLog, lasYJHKsource, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, UKIDSSDetection, udsDetection, udsListRemeasurement, udsMergeLog, udsSource, udsSourceRemeasurement |
WSA |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
calDetection, calListRemeasurement, calMergeLog, calSource, calSourceRemeasurement, calSynopticMergeLog, calSynopticSource |
WSACalib |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Y |
cy |
first08Jul16Source, firstSource |
FIRST |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_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 |
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 |
CZ |
twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 |
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_EQ_Z |
cz |
CurrentAstrometry |
WSATransit |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
POS_EQ_Z |
cz |
CurrentAstrometry, PreviousAstrometry |
WSA |
unit vector of spherical co-ordinates of device centre |
float |
8 |
|
|
POS_EQ_Z |
cz |
dxsDetection, dxsJKmergeLog, dxsJKsource, dxsListRemeasurement, dxsMergeLog, dxsSource, dxsSourceRemeasurement, gcsDetection, gcsListRemeasurement, gcsMergeLog, gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKmergeLog, gcsZYJHKsource, gpsDetection, gpsJHKmergeLog, gpsJHKsource, gpsListRemeasurement, gpsMergeLog, gpsPointSource, gpsSource, gpsSourceRemeasurement, lasDetection, lasExtendedSource, lasListRemeasurement, lasMergeLog, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKmergeLog, lasYJHKsource, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, UKIDSSDetection, udsDetection, udsListRemeasurement, udsMergeLog, udsSource, udsSourceRemeasurement |
WSA |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
calDetection, calListRemeasurement, calMergeLog, calSource, calSourceRemeasurement, calSynopticMergeLog, calSynopticSource |
WSACalib |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_Z |
cz |
first08Jul16Source, firstSource |
FIRST |
unit vector of spherical co-ordinates |
float |
8 |
|
|
POS_EQ_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 |
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 |