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Glossary of WSA attributes

This Glossary alphabetically lists all attributes used in the UKIDSSDR7 database(s) held in the WSA. If you would like to have more information about the schema tables please use the UKIDSSDR7 Schema Browser (other Browser versions).
A B C D E F G H I J K L M
N O P Q R S T U V W X Y Z

S

NameSchema TableDatabaseDescriptionTypeLengthUnitDefault ValueUnified Content Descriptor
S14 nvssSource NVSS Integrated 1.4GHz flux density of radio source real 4 mJy   PHOT_FLUX_RADIO_1.4G
SC_CHI2PROB twoxmm XMM The Chi² probability (based on the null hypothesis) that the unique source SRCID as detected by any of the observations is constant, that is, the minimum value of the EPIC probabilities in each detection, EP_CHI2PROB, is given. real 4      
SC_DEC twoxmm XMM The mean Declination in degrees (J2000) of all the detections of the source SRCID (see DEC) weighted by the positional errors POSERR. float 8 degrees    
SC_DET_ML twoxmm XMM The total band detection likelihood of the source SRCID is the maximum of the likelihoods of all detections of this source (EP_8_DET_ML). real 4      
SC_EP_1_FLUX twoxmm XMM The mean band 1 flux (0.2 - 0.5 keV) of all the detections of the source SRCID (see EP_1_FLUX) weighted by the errors (EP_1_FLUX_ERR), in erg/cm2/s. real 4 erg/cm**2/s    
SC_EP_1_FLUX_ERR twoxmm XMM Error on the weighted mean band 1 flux in SC_EP_1_FLUX. real 4 erg/cm**2/s    
SC_EP_2_FLUX twoxmm XMM The mean band 2 flux (0.5 - 1.0 keV) of all the detections of the source SRCID (see EP_2_FLUX) weighted by the errors (EP_2_FLUX_ERR), in erg/cm2/s. real 4 erg/cm**2/s    
SC_EP_2_FLUX_ERR twoxmm XMM Error on the weighted mean band 2 flux in SC_EP_2_FLUX. real 4 erg/cm**2/s    
SC_EP_3_FLUX twoxmm XMM The mean band 3 flux (1.0 - 2.0 keV) of all the detections of the source SRCID (see EP_3_FLUX) weighted by the errors (EP_3_FLUX_ERR), in erg/cm2/s. real 4 erg/cm**2/s    
SC_EP_3_FLUX_ERR twoxmm XMM Error on the weighted mean band 3 flux in SC_EP_3_FLUX. real 4 erg/cm**2/s    
SC_EP_4_FLUX twoxmm XMM The mean band 4 flux (2.0 - 4.5 keV) of all the detections of the source SRCID (see EP_4_FLUX) weighted by the errors (EP_4_FLUX_ERR), in erg/cm2/s. real 4 erg/cm**2/s    
SC_EP_4_FLUX_ERR twoxmm XMM Error on the weighted mean band 4 flux in SC_EP_4_FLUX. real 4 erg/cm**2/s    
SC_EP_5_FLUX twoxmm XMM The mean band 5 flux (4.5 - 12 keV) of all the detections of the source SRCID (see EP_5_FLUX) weighted by the errors (EP_5_FLUX_ERR), in erg/cm2/s. real 4 erg/cm**2/s    
SC_EP_5_FLUX_ERR twoxmm XMM Error on the weighted mean band 5 flux in SC_EP_5_FLUX. real 4 erg/cm**2/s    
SC_EP_8_FLUX twoxmm XMM The mean total band flux (0.2 - 12 keV) of all the detections of the source SRCID (see EP_8_FLUX) weighted by the errors (EP_8_FLUX_ERR), in erg/cm2/s. real 4 erg/cm**2/s    
SC_EP_8_FLUX_ERR twoxmm XMM Error on the weighted mean total band flux in SC_EP_8_FLUX. real 4 erg/cm**2/s    
SC_EP_9_FLUX twoxmm XMM The mean band 9 flux (0.5 - 4.5 keV) of all the detections of the source SRCID (see EP_9_FLUX) weighted by the errors (EP_9_FLUX_ERR), in erg/cm2/s. real 4 erg/cm**2/s    
SC_EP_9_FLUX_ERR twoxmm XMM Error on the weighted mean band 9 flux in SC_EP_9_FLUX. real 4 erg/cm**2/s    
SC_EXT_ML twoxmm XMM The total band detection likelihood of the extended source SRCID is the average of the extent likelihoods of all detections of this source (EP_EXTENT_ML). real 4      
SC_HR1 twoxmm XMM The mean hardness ratio of the bands 1 and 2 of all the detections of the source SRCID (EP_HR1) weighted by the errors(EP_HR1_ERR). real 4      
SC_HR1_ERR twoxmm XMM Error on the weighted mean hardness ratio in SC_HR1. real 4      
SC_HR2 twoxmm XMM The mean hardness ratio of the bands 2 and 3 of all the detections of the source SRCID (EP_HR2) weighted by the errors(EP_HR2_ERR). real 4      
SC_HR2_ERR twoxmm XMM Error on the weighted mean hardness ratio in SC_HR2. real 4      
SC_HR3 twoxmm XMM The mean hardness ratio of the bands 3 and 4 of all the detections of the source SRCID (EP_HR3) weighted by the errors(EP_HR3_ERR). real 4      
SC_HR3_ERR twoxmm XMM Error on the weighted mean hardness ratio in SC_HR3. real 4      
SC_HR4 twoxmm XMM The mean hardness ratio of the bands 4 and 5 of all the detections of the source SRCID (EP_HR4) weighted by the errors(EP_HR4_ERR). real 4      
SC_HR4_ERR twoxmm XMM Error on the weighted mean hardness ratio in SC_HR4. real 4      
SC_POSERR twoxmm XMM The error of the weighted mean position given in SC_RA and SC_DEC in arcseconds. real 4 arcsec    
SC_RA twoxmm XMM The mean Right Ascension in degrees (J2000) of all the detections of the source SRCID (see RA) weighted by the positional errors POSERR. float 8 degrees    
SC_SUM_FLAG twoxmm XMM The summary flag for the unique source SRCID is taken to be the worst flag of all detections of this source (SUM_FLAG). int 4      
SC_VAR_FLAG twoxmm XMM The variability flag for the unique source SRCID is set to VAR_FLAG of the most variable detection of this source. varchar 5      
scan twomass_psc 2MASS The nightly scan number in which the source was detected. smallint 2     NUMBER
scan twomass_scn 2MASS Scan number (unique within date). smallint 2     NUMBER
scan twomass_xsc 2MASS scan number (unique within date). smallint 2     NUMBER
scan_key twomass_psc 2MASS Unique identification number of the record in the Scan Information Table that corresponds to the survey scan in which this source was detected. int 4     ID_NUMBER
scan_key twomass_scn 2MASS the unique identification number for this scan. int 4     ID_NUMBER
scan_key twomass_xsc 2MASS key to scan data record in "scan DB". int 4     ID_NUMBER
scrunch RequiredMosaic WSA CASU mosaic tool mandatory parameter to specifying the no. of pixels to rebin into one pixel in the output image (1=no rebinning) smallint 2 pixels   ??
scrunch RequiredMosaic WSACalib CASU mosaic tool mandatory parameter to specifying the no. of pixels to rebin into one pixel in the output image (1=no rebinning) smallint 2 pixels   ??
scrunch RequiredMosaic WSATransit CASU mosaic tool mandatory parameter to specifying the no. of pixels to rebin into one pixel in the output image (1=no rebinning) smallint 2 pixels   ??
scTemp Multiframe WSA SCSU cab temperature {image primary HDU keyword: SC_TEMP} real 4 degrees_Kelvin -0.9999995e9  
scTemp Multiframe WSACalib SCSU cab temperature {image primary HDU keyword: SC_TEMP} real 4 degrees_Kelvin -0.9999995e9  
scTemp Multiframe WSATransit SCSU cab temperature {image primary HDU keyword: SC_TEMP} real 4 degrees_Kelvin -0.9999995e9  
sd twomass_scn 2MASS Scanning direction: "n" = north-going, "s" = south-going. varchar 1     POS_POS-ANG
SDSS_CAMCOL mgcBrightSpec MGC SDSS camera column int 4      
SDSS_CLASS mgcBrightSpec MGC MGC translation of SDSS_TYPE smallint 2      
SDSS_DEC mgcBrightSpec MGC SDSS object declination in deg (J2000) float 8      
SDSS_EXTINC_G mgcBrightSpec MGC SDSS Galactic extinction correction in mag real 4      
SDSS_EXTINC_I mgcBrightSpec MGC SDSS Galactic extinction correction in mag real 4      
SDSS_EXTINC_R mgcBrightSpec MGC SDSS Galactic extinction correction in mag real 4      
SDSS_EXTINC_U mgcBrightSpec MGC SDSS Galactic extinction correction in mag real 4      
SDSS_EXTINC_Z mgcBrightSpec MGC SDSS Galactic extinction correction in mag real 4      
SDSS_FIELD mgcBrightSpec MGC SDSS field number int 4      
SDSS_MODMAG_G mgcBrightSpec MGC SDSS extinction corrected model magnitude real 4      
SDSS_MODMAG_I mgcBrightSpec MGC SDSS extinction corrected model magnitude real 4      
SDSS_MODMAG_R mgcBrightSpec MGC SDSS extinction corrected model magnitude real 4      
SDSS_MODMAG_U mgcBrightSpec MGC SDSS extinction corrected model magnitude real 4      
SDSS_MODMAG_Z mgcBrightSpec MGC SDSS extinction corrected model magnitude real 4      
SDSS_N mgcBrightSpec MGC Number of SDSS objects matched to MGC object int 4      
SDSS_OBJID mgcBrightSpec MGC SDSS PhotoObject ID bigint 8      
SDSS_PETMAG_G mgcBrightSpec MGC SDSS extinction corrected Petrosian magnitude real 4      
SDSS_PETMAG_I mgcBrightSpec MGC SDSS extinction corrected Petrosian magnitude real 4      
SDSS_PETMAG_R mgcBrightSpec MGC SDSS extinction corrected Petrosian magnitude real 4      
SDSS_PETMAG_U mgcBrightSpec MGC SDSS extinction corrected Petrosian magnitude real 4      
SDSS_PETMAG_Z mgcBrightSpec MGC SDSS extinction corrected Petrosian magnitude real 4      
SDSS_PETR50_G mgcBrightSpec MGC SDSS radius containing 50% Petrosian flux in arcsec real 4      
SDSS_PETR50_I mgcBrightSpec MGC SDSS radius containing 50% Petrosian flux in arcsec real 4      
SDSS_PETR50_R mgcBrightSpec MGC SDSS radius containing 50% Petrosian flux in arcsec real 4      
SDSS_PETR50_U mgcBrightSpec MGC SDSS radius containing 50% Petrosian flux in arcsec real 4      
SDSS_PETR50_Z mgcBrightSpec MGC SDSS radius containing 50% Petrosian flux in arcsec real 4      
SDSS_PSFMAG_G mgcBrightSpec MGC SDSS extinction corrected PSF magnitude real 4      
SDSS_PSFMAG_I mgcBrightSpec MGC SDSS extinction corrected PSF magnitude real 4      
SDSS_PSFMAG_R mgcBrightSpec MGC SDSS extinction corrected PSF magnitude real 4      
SDSS_PSFMAG_U mgcBrightSpec MGC SDSS extinction corrected PSF magnitude real 4      
SDSS_PSFMAG_Z mgcBrightSpec MGC SDSS extinction corrected PSF magnitude real 4      
SDSS_RA mgcBrightSpec MGC SDSS object right ascension in deg (J2000) float 8      
SDSS_RERUN mgcBrightSpec MGC SDSS rerun number int 4      
SDSS_RUN mgcBrightSpec MGC SDSS run number int 4      
SDSS_SPCLASS mgcBrightSpec MGC MGC translation of SDSS_SPECCLASS smallint 2      
SDSS_SPECCLASS mgcBrightSpec MGC SDSS spectroscopic classification smallint 2      
SDSS_TYPE mgcBrightSpec MGC SDSS morphological classification smallint 2      
SDSS_Z mgcBrightSpec MGC SDSS redshift real 4      
SDSS_ZQUAL mgcBrightSpec MGC SDSS redshift quality tinyint 1      
sdssPrimary dxsSourceXDR7PhotoObj, dxsSourceXStripe82PhotoObjAll, gcsSourceXDR5PhotoObj, gcsSourceXDR7PhotoObj, lasSourceXDR2PhotoObj, lasSourceXDR3PhotoObj, lasSourceXDR5PhotoObj, lasSourceXDR5PhotoObjAll, lasSourceXDR7PhotoObj, lasSourceXDR7PhotoObjAll, lasSourceXSegueDR6PhotoObj, lasSourceXSegueDR6PhotoObjAll, lasSourceXStripe82PhotoObjAll WSA SDSS flag for neighbour being primary (1) or secondary (0) tinyint 1     CODE_MISC
sdssType dxsSourceXDR7PhotoObj, dxsSourceXStripe82PhotoObjAll, gcsSourceXDR5PhotoObj, gcsSourceXDR7PhotoObj, lasSourceXDR2PhotoObj, lasSourceXDR3PhotoObj, lasSourceXDR5PhotoObj, lasSourceXDR5PhotoObjAll, lasSourceXDR7PhotoObj, lasSourceXDR7PhotoObjAll, lasSourceXSegueDR6PhotoObj, lasSourceXSegueDR6PhotoObjAll, lasSourceXStripe82PhotoObjAll WSA SDSS type of neighbour: 3=galaxy; 6=star tinyint 1     CLASS_OBJECT
sdsuNum MultiframeDetector WSA Serial number of SDSU controller {image extension keyword: SDSUID} varchar 32   NONE ??
sdsuNum MultiframeDetector WSACalib Serial number of SDSU controller {image extension keyword: SDSUID} varchar 32   NONE ??
sdsuNum MultiframeDetector WSATransit Serial number of SDSU controller {image extension keyword: SDSUID} varchar 32   NONE ??
secondaryTemp Multiframe WSA Temperature of secondary {image primary HDU keyword: SECONDAR} real 4 degrees_Celsius -0.9999995e9 PHYS_TEMP_MISC
secondaryTemp Multiframe WSACalib Temperature of secondary {image primary HDU keyword: SECONDAR} real 4 degrees_Celsius -0.9999995e9 PHYS_TEMP_MISC
secondaryTemp Multiframe WSATransit Temperature of secondary {image primary HDU keyword: SECONDAR} real 4 degrees_Celsius -0.9999995e9 PHYS_TEMP_MISC
seeing MultiframeDetector WSA Average FWHM {catalogue extension keyword:  SEEING} real 4 pixels -0.9999995e9 ??
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC).
seeing MultiframeDetector WSACalib Average FWHM {catalogue extension keyword:  SEEING} real 4 pixels -0.9999995e9 ??
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC).
seeing MultiframeDetector WSATransit Average FWHM {catalogue extension keyword:  SEEING} real 4 pixels -0.9999995e9 ??
An average realistic FWHM estimated directly from the stellar images on the frame. Multiply by pixel scale size to convert to arcsec (eg. ×0.400 WFCAM; ×0.333 INT WFC).
SEP_1XMM twoxmm XMM The distance between this source and the matched 1XMM source (MATCH_1XMM) in arcseconds. real 4 arcsec    
SEP_2XMMP twoxmm XMM The distance between this source and the matched 2XMMp source (MATCH_2XMMp) in arcseconds. real 4 arcsec    
seqNo firstSource FIRST sequential object number int 4     ID_NUMBER
seqNo glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca, glimpse_hrc_inter GLIMPSE sequential object number in the HRC int 4     ID_NUMBER
seqNo glimpse_mca_inter GLIMPSE sequential object number in the MCA int 4     ID_NUMBER
seqNo iras_psc IRAS sequential object number int 4     ID_NUMBER
seqNo nvssSource NVSS sequential object number int 4     ID_NUMBER
seqNo rosat_bsc ROSAT sequential object number in the BSC int 4     ID_NUMBER
seqNo rosat_fsc ROSAT sequential object number in the FSC int 4     ID_NUMBER
seqNum UKIDSSDetection WSA the running number of this detection int 4     ID_NUMBER
seqNum calDetection, calListRemeasurement WSACalib the running number of this detection {catalogue TType keyword: Sequence_number}
The running number for ease of reference, in strict order of image detections.
int 4     ID_NUMBER
seqNum dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsDetection, udsListRemeasurement WSA the running number of this detection {catalogue TType keyword: Sequence_number}
The running number for ease of reference, in strict order of image detections.
int 4     ID_NUMBER
seqNum dxsSourceXDetectionBestMatch, udsSourceXDetectionBestMatch WSA the running number of this detection {catalogue TType keyword: Sequence_number}
The running number for ease of reference, in strict order of image detections.
int 4   -99999999 ID_NUMBER
seqNum ptsDetection WSATransit the running number of this detection {catalogue TType keyword: Sequence_number}
The running number for ease of reference, in strict order of image detections.
int 4     ID_NUMBER
SerFit1DChi2 UKIDSSDetection WSA Error in 1D fit real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerFit1DChi2 calDetection, calListRemeasurement WSACalib Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2}
standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerFit1DChi2 dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2}
standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerFit1DChi2 ptsDetection WSATransit Error in 1D fit {catalogue TType keyword: 1D_Sersic_fit_chi2}
standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerFit1DChi2 udsDetection WSA Not available in SE output {catalogue TType keyword: 1D_Sersic_fit_chi2} real 4   -0.9999995e9  
SerFit2DChi2 UKIDSSDetection WSA Error in 2D fit real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerFit2DChi2 calDetection, calListRemeasurement WSACalib Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2}
standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerFit2DChi2 dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2}
standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerFit2DChi2 ptsDetection WSATransit Error in 2D fit {catalogue TType keyword: 2D_Sersic_fit_chi2}
standard normalised variance of fit [For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerFit2DChi2 udsDetection WSA Not available in SE output {catalogue TType keyword: 2D_Sersic_fit_chi2} real 4   -0.9999995e9  
SerFitNu1D UKIDSSDetection WSA No. of degrees of freedom for 1D Sersic fit real 4   -0.9999995e9 STAT_N-DOF
SerFitNu1D calDetection, calListRemeasurement WSACalib No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 STAT_N-DOF
SerFitNu1D dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 STAT_N-DOF
SerFitNu1D ptsDetection WSATransit No. of degrees of freedom for 1D Sersic fit {catalogue TType keyword: 1D_Sersic_fit_nu}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 STAT_N-DOF
SerFitNu1D udsDetection WSA Not available in SE output {catalogue TType keyword: 1D_Sersic_fit_nu} real 4   -0.9999995e9  
SerFitNu2D UKIDSSDetection WSA No. of degrees of freedom for 2D Sersic fit real 4   -0.9999995e9 STAT_N-DOF
SerFitNu2D calDetection, calListRemeasurement WSACalib No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 STAT_N-DOF
SerFitNu2D dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 STAT_N-DOF
SerFitNu2D ptsDetection WSATransit No. of degrees of freedom for 2D Sersic fit {catalogue TType keyword: 2D_Sersic_fit_nu}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 STAT_N-DOF
SerFitNu2D udsDetection WSA Not available in SE output {catalogue TType keyword: 2D_Sersic_fit_nu} real 4   -0.9999995e9  
SerFlux1D UKIDSSDetection WSA 1D Sersic flux real 4 ADU -0.9999995e9 PHOT_INTENSITY_ADU
SerFlux1D calDetection, calListRemeasurement WSACalib 1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 ADU -0.9999995e9 PHOT_INTENSITY_ADU
SerFlux1D dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA 1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 ADU -0.9999995e9 PHOT_INTENSITY_ADU
SerFlux1D ptsDetection WSATransit 1D Sersic flux {catalogue TType keyword: 1D_Sersic_flux}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 ADU -0.9999995e9 PHOT_INTENSITY_ADU
SerFlux1D udsDetection WSA Not available in SE output {catalogue TType keyword: 1D_Sersic_flux} real 4   -0.9999995e9  
SerFlux2D UKIDSSDetection WSA 2D Sersic flux real 4 ADU -0.9999995e9 PHOT_INTENSITY_ADU
SerFlux2D calDetection, calListRemeasurement WSACalib 2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 ADU -0.9999995e9 PHOT_INTENSITY_ADU
SerFlux2D dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA 2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 ADU -0.9999995e9 PHOT_INTENSITY_ADU
SerFlux2D ptsDetection WSATransit 2D Sersic flux {catalogue TType keyword: 2D_Sersic_flux}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 ADU -0.9999995e9 PHOT_INTENSITY_ADU
SerFlux2D udsDetection WSA Not available in SE output {catalogue TType keyword: 2D_Sersic_flux} real 4   -0.9999995e9  
SerIdx1D UKIDSSDetection WSA Power law index real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerIdx1D calDetection, calListRemeasurement WSACalib Power law index {catalogue TType keyword: 1D_Sersic_index}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerIdx1D dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA Power law index {catalogue TType keyword: 1D_Sersic_index}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerIdx1D ptsDetection WSATransit Power law index {catalogue TType keyword: 1D_Sersic_index}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerIdx1D udsDetection WSA Not available in SE output {catalogue TType keyword: 1D_Sersic_index} real 4   -0.9999995e9  
SerIdx2D UKIDSSDetection WSA Power law index real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerIdx2D calDetection, calListRemeasurement WSACalib Power law index {catalogue TType keyword: 2D_Sersic_index}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerIdx2D dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA Power law index {catalogue TType keyword: 2D_Sersic_index}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerIdx2D ptsDetection WSATransit Power law index {catalogue TType keyword: 2D_Sersic_index}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerIdx2D udsDetection WSA Not available in SE output {catalogue TType keyword: 2D_Sersic_index} real 4   -0.9999995e9  
SerMag1D UKIDSSDetection WSA Calibrated 1D Sersic flux real 4 mag -0.9999995e9 PHOT_PROFILE
SerMag1D calDetection, calListRemeasurement WSACalib Calibrated 1D Sersic flux
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 mag -0.9999995e9 PHOT_PROFILE
SerMag1D dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA Calibrated 1D Sersic flux
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 mag -0.9999995e9 PHOT_PROFILE
SerMag1D ptsDetection WSATransit Calibrated 1D Sersic flux
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 mag -0.9999995e9 PHOT_PROFILE
SerMag1D udsDetection WSA Not available in SE output real 4   -0.9999995e9  
SerMag2D UKIDSSDetection WSA Calibrated 2D Sersic flux real 4 mag -0.9999995e9 PHOT_PROFILE
SerMag2D calDetection, calListRemeasurement WSACalib Calibrated 2D Sersic flux
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 mag -0.9999995e9 PHOT_PROFILE
SerMag2D dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA Calibrated 2D Sersic flux
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 mag -0.9999995e9 PHOT_PROFILE
SerMag2D ptsDetection WSATransit Calibrated 2D Sersic flux
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4 mag -0.9999995e9 PHOT_PROFILE
SerMag2D udsDetection WSA Not available in SE output real 4   -0.9999995e9  
SerScaleLen1D UKIDSSDetection WSA Scale length real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerScaleLen1D calDetection, calListRemeasurement WSACalib Scale length {catalogue TType keyword: 1D_Sersic_scale_len}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerScaleLen1D dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA Scale length {catalogue TType keyword: 1D_Sersic_scale_len}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerScaleLen1D ptsDetection WSATransit Scale length {catalogue TType keyword: 1D_Sersic_scale_len}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerScaleLen1D udsDetection WSA Not available in SE output {catalogue TType keyword: 1D_Sersic_scale_len} real 4   -0.9999995e9  
SerScaleLen2D UKIDSSDetection WSA Scale length real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerScaleLen2D calDetection, calListRemeasurement WSACalib Scale length {catalogue TType keyword: 2D_Sersic_scale_len}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerScaleLen2D dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA Scale length {catalogue TType keyword: 2D_Sersic_scale_len}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerScaleLen2D ptsDetection WSATransit Scale length {catalogue TType keyword: 2D_Sersic_scale_len}
[For numerical stability the Sersic fits will use the previously derived x-y coordinates]
real 4   -0.9999995e9 PHOT_PROFILE_PAR
SerScaleLen2D udsDetection WSA Not available in SE output {catalogue TType keyword: 2D_Sersic_scale_len} real 4   -0.9999995e9  
SERSIC mgcGalaxyStruct MGC Sersic Index (=4 for de Vaucouleurs profile) real 4   99.99  
SERSIC_KAPPA mgcGalaxyStruct MGC Sersic profile coefficient real 4      
SERSICm mgcGalaxyStruct MGC Sersic Index error (-) real 4   99.99  
SERSICp mgcGalaxyStruct MGC Sersic Index error (+) real 4   99.99  
server ExternalSurvey WSA The location of the database: load or public server varchar 16     ??
server ExternalSurvey WSACalib The location of the database: load or public server varchar 16     ??
server ExternalSurvey WSATransit The location of the database: load or public server varchar 16     ??
ses1_100 iras_psc IRAS Number of seconds-confirmed nearby small extended sources (100 micron). tinyint 1     INST_PARAM
ses1_12 iras_psc IRAS Number of seconds-confirmed nearby small extended sources (12 micron). tinyint 1     INST_PARAM
ses1_25 iras_psc IRAS Number of seconds-confirmed nearby small extended sources (25 micron). tinyint 1     INST_PARAM
ses1_60 iras_psc IRAS Number of seconds-confirmed nearby small extended sources (60 micron). tinyint 1     INST_PARAM
ses2_100 iras_psc IRAS Number of nearby weeks-confirmed small extended sources (100 micron). tinyint 1     CODE_MISC
ses2_12 iras_psc IRAS Number of nearby weeks-confirmed small extended sources (12 micron). tinyint 1     CODE_MISC
ses2_25 iras_psc IRAS Number of nearby weeks-confirmed small extended sources (25 micron). tinyint 1     CODE_MISC
ses2_60 iras_psc IRAS Number of nearby weeks-confirmed small extended sources (60 micron). tinyint 1     CODE_MISC
SEX_FLAG mgcGalaxyStruct MGC SExtractor Flag int 4 Integer    
shortName Filter WSA Short identification name for the filter varchar 4     ??
shortName Filter WSACalib Short identification name for the filter varchar 4     ??
shortName Filter WSATransit Short identification name for the filter varchar 4     ??
sigDec calSourceRemeasurement WSACalib Uncertainty in Dec real 4 Degrees -0.9999995e9 ERROR
sigDec calVariability WSACalib Uncertainty in mean Dec real 4 Arcseconds -0.9999995e9 ERROR
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.
sigDec dxsSourceRemeasurement, gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, lasExtendedSource, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKsource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, udsSourceRemeasurement WSA Uncertainty in Dec real 4 Degrees -0.9999995e9 ERROR
sigDec dxsVariability, udsVariability WSA Uncertainty in mean Dec real 4 Arcseconds -0.9999995e9 ERROR
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.
sigMuDec calVariability WSACalib Error on proper motion in Dec real 4 mas/yr -0.9999995e9 ERROR
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.
sigMuDec dxsVariability, udsVariability WSA Error on proper motion in Dec real 4 mas/yr -0.9999995e9 ERROR
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.
sigMuDec gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource WSA Error on proper motion in Dec direction real 4 mas/yr -0.9999995e9 ERROR
sigMuRa calVariability WSACalib Error on proper motion in RA real 4 mas/yr -0.9999995e9 ERROR
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.
sigMuRa dxsVariability, udsVariability WSA Error on proper motion in RA real 4 mas/yr -0.9999995e9 ERROR
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.
sigMuRa gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource WSA Error on proper motion in RA direction real 4 mas/yr -0.9999995e9 ERROR
sigRa calSourceRemeasurement WSACalib Uncertainty in RA real 4 Degrees -0.9999995e9 ERROR
sigRa calVariability WSACalib Uncertainty in mean RA real 4 Arcseconds -0.9999995e9 ERROR
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.
sigRa dxsSourceRemeasurement, gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, lasExtendedSource, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKsource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, udsSourceRemeasurement WSA Uncertainty in RA real 4 Degrees -0.9999995e9 ERROR
sigRa dxsVariability, udsVariability WSA Uncertainty in mean RA real 4 Arcseconds -0.9999995e9 ERROR
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.
sky UKIDSSDetection WSA local interpolated sky level from background tracker real 4 ADU   INST_SKY_LEVEL
sky calDetection, calListRemeasurement WSACalib local interpolated sky level from background tracker {catalogue TType keyword: Sky_level} real 4 ADU   INST_SKY_LEVEL
sky dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA local interpolated sky level from background tracker {catalogue TType keyword: Sky_level} real 4 ADU   INST_SKY_LEVEL
sky ptsDetection WSATransit local interpolated sky level from background tracker {catalogue TType keyword: Sky_level} real 4 ADU   INST_SKY_LEVEL
sky udsDetection WSA local interpolated sky level from background tracker (SE: BACKGROUND) {catalogue TType keyword: Sky_level} real 4 ADU   INST_SKY_LEVEL
sky1 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Local sky bkg. for band 1 flux real 4 MJy/sr -999.9  
sky2 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Local sky bkg. for band 2 flux real 4 MJy/sr -999.9  
sky3 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Local sky bkg. for band 3 flux real 4 MJy/sr -999.9  
sky3_6 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Local sky background for 3.6um IRAC (Band 1) real 4 MJy/sr -999.9  
sky4 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Local sky bkg. for band 4 flux real 4 MJy/sr -999.9  
sky4_5 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Local sky background for 4.5um IRAC (Band 2) real 4 MJy/sr -999.9  
sky5_8 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Local sky background for 5.8um IRAC (Band 3) real 4 MJy/sr -999.9  
sky8_0 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Local sky background for 8.0um IRAC (Band 4) real 4 MJy/sr -999.9  
skyAlgorithm Multiframe WSA Sky estimation algorithm {image primary HDU keyword: SKYALGO} varchar 64   NONE  
skyAlgorithm Multiframe WSACalib Sky estimation algorithm {image primary HDU keyword: SKYALGO} varchar 64   NONE  
skyAlgorithm Multiframe WSATransit Sky estimation algorithm {image primary HDU keyword: SKYALGO} varchar 64   NONE  
skyCorrCat MultiframeDetector WSA Percentage sky correction for the catalogue data {catalogue extension keyword:  PERCORR}
corrected photometry = 2.5×log10(flux) + aperCor + skyCorr
real 4   -0.9999995e9 ??
This is a correction based on the median dark sky recorded in science frames compared to the median for all the detectors and as such is an ancillary correction to the gain correction derived from the flatfield (usually twilight flats) data.
skyCorrCat MultiframeDetector WSACalib Percentage sky correction for the catalogue data {catalogue extension keyword:  PERCORR}
corrected photometry = 2.5×log10(flux) + aperCor + skyCorr
real 4   -0.9999995e9 ??
This is a correction based on the median dark sky recorded in science frames compared to the median for all the detectors and as such is an ancillary correction to the gain correction derived from the flatfield (usually twilight flats) data.
skyCorrCat MultiframeDetector WSATransit Percentage sky correction for the catalogue data {catalogue extension keyword:  PERCORR}
corrected photometry = 2.5×log10(flux) + aperCor + skyCorr
real 4   -0.9999995e9 ??
This is a correction based on the median dark sky recorded in science frames compared to the median for all the detectors and as such is an ancillary correction to the gain correction derived from the flatfield (usually twilight flats) data.
skyCorrExt MultiframeDetector WSA Percentage sky correction of the detector {image extension keyword: PERCORR}
corrected photometry = 2.5×log10(flux) + aperCor + skyCorr
real 4   -0.9999995e9 ??
This is a correction based on the median dark sky recorded in science frames compared to the median for all the detectors and as such is an ancillary correction to the gain correction derived from the flatfield (usually twilight flats) data.
skyCorrExt MultiframeDetector WSACalib Percentage sky correction of the detector {image extension keyword: PERCORR}
corrected photometry = 2.5×log10(flux) + aperCor + skyCorr
real 4   -0.9999995e9 ??
This is a correction based on the median dark sky recorded in science frames compared to the median for all the detectors and as such is an ancillary correction to the gain correction derived from the flatfield (usually twilight flats) data.
skyCorrExt MultiframeDetector WSATransit Percentage sky correction of the detector {image extension keyword: PERCORR}
corrected photometry = 2.5×log10(flux) + aperCor + skyCorr
real 4   -0.9999995e9 ??
This is a correction based on the median dark sky recorded in science frames compared to the median for all the detectors and as such is an ancillary correction to the gain correction derived from the flatfield (usually twilight flats) data.
skyID Multiframe WSA UID of library calibration sky sub frame {image extension keyword: SKYSUB} bigint 8   -99999999 ID_FRAME
skyID Multiframe WSACalib UID of library calibration sky sub frame {image extension keyword: SKYSUB} bigint 8   -99999999 ID_FRAME
skyID Multiframe WSATransit UID of library calibration sky sub frame {image extension keyword: SKYSUB} bigint 8   -99999999 ID_FRAME
skyLevel MultiframeDetector WSA Median sky brightness {catalogue extension keyword:  SKYLEVEL} real 4 counts/pixel -0.9999995e9 ??
An automatic 2D background-following algorithm is used to track and "remove" slowly varying background features such as image gradients etc.. The default scale size for background tracking (NBSIZE) is currently set to 64 pixels, coupled with a smidge of non-linear filtering this gives a background tracking scale of order 100 pixels. (A bilinear interpolator is used to generate pixel resolution background maps internally).
skyLevel MultiframeDetector WSACalib Median sky brightness {catalogue extension keyword:  SKYLEVEL} real 4 counts/pixel -0.9999995e9 ??
An automatic 2D background-following algorithm is used to track and "remove" slowly varying background features such as image gradients etc.. The default scale size for background tracking (NBSIZE) is currently set to 64 pixels, coupled with a smidge of non-linear filtering this gives a background tracking scale of order 100 pixels. (A bilinear interpolator is used to generate pixel resolution background maps internally).
skyLevel MultiframeDetector WSATransit Median sky brightness {catalogue extension keyword:  SKYLEVEL} real 4 counts/pixel -0.9999995e9 ??
An automatic 2D background-following algorithm is used to track and "remove" slowly varying background features such as image gradients etc.. The default scale size for background tracking (NBSIZE) is currently set to 64 pixels, coupled with a smidge of non-linear filtering this gives a background tracking scale of order 100 pixels. (A bilinear interpolator is used to generate pixel resolution background maps internally).
skyNoise MultiframeDetector WSA Pixel noise at sky level {catalogue extension keyword:  SKYNOISE} real 4 counts -0.9999995e9 ??
Robust MAD estimator for noise scaled to equivalent Gaussian rms value ie. = MAD × 1.48 after removing large scale sky background variations. MAD = Median of the Absolute Deviations about the median.
skyNoise MultiframeDetector WSACalib Pixel noise at sky level {catalogue extension keyword:  SKYNOISE} real 4 counts -0.9999995e9 ??
Robust MAD estimator for noise scaled to equivalent Gaussian rms value ie. = MAD × 1.48 after removing large scale sky background variations. MAD = Median of the Absolute Deviations about the median.
skyNoise MultiframeDetector WSATransit Pixel noise at sky level {catalogue extension keyword:  SKYNOISE} real 4 counts -0.9999995e9 ??
Robust MAD estimator for noise scaled to equivalent Gaussian rms value ie. = MAD × 1.48 after removing large scale sky background variations. MAD = Median of the Absolute Deviations about the median.
skySubScale MultiframeDetector WSA Scale factor applied to sky subtraction image {image extension keyword: SKYSUB} float 8   -0.9999995e9 ??
skySubScale MultiframeDetector WSACalib Scale factor applied to sky subtraction image {image extension keyword: SKYSUB} float 8   -0.9999995e9 ??
skySubScale MultiframeDetector WSATransit Scale factor applied to sky subtraction image {image extension keyword: SKYSUB} float 8   -0.9999995e9 ??
skyVar UKIDSSDetection WSA local estimate of variation in sky level around image real 4 ADU   INST_SKY_LEVEL
skyVar calDetection, calListRemeasurement WSACalib local estimate of variation in sky level around image {catalogue TType keyword: Sky_rms} real 4 ADU   INST_SKY_LEVEL
skyVar dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement WSA local estimate of variation in sky level around image {catalogue TType keyword: Sky_rms} real 4 ADU   INST_SKY_LEVEL
skyVar ptsDetection WSATransit local estimate of variation in sky level around image {catalogue TType keyword: Sky_rms} real 4 ADU   INST_SKY_LEVEL
skyVar udsDetection WSA local estimate of variation in sky level around image (SE: THRESHOLD) {catalogue TType keyword: Sky_rms} real 4 ADU   INST_SKY_LEVEL
slaveObjID calSourceNeighbours WSACalib The unique ID of the neighbour in calSource (=sourceID) bigint 8     ID_CATALOG
slaveObjID calSourceXSynopticSource WSACalib The unique ID of the neighbour in calSynopticSource (=synopticID) bigint 8     ID_CATALOG
slaveObjID calSourceXtwomass_psc WSACalib The unique ID of the neighbour in TWOMASS..twomass_psc (=pts_key) bigint 8     ID_CATALOG
slaveObjID calSourceXukirtFSstars WSACalib The unique ID of the neighbour in ukirtFSstars bigint 8      
slaveObjID dxsSourceNeighbours WSA The unique ID of the neighbour in dxsSource (=sourceID) bigint 8     ID_CATALOG
slaveObjID dxsSourceXDR7PhotoObj, dxsSourceXStripe82PhotoObjAll, gcsSourceXDR7PhotoObj, lasSourceXDR7PhotoObj WSA The unique ID of the neighbour in BestDR7..PhotoObj (=objID) bigint 8     ID_CATALOG
slaveObjID dxsSourceXDetection WSA The unique ID of the neighbour in dxsDetection (=objID) bigint 8     ID_CATALOG
slaveObjID dxsSourceXtwomass_psc, gcsSourceXtwomass_psc, lasSourceXtwomass_psc WSA The unique ID of the neighbour in TWOMASS..twomass_psc (=pts_key) bigint 8     ID_CATALOG
slaveObjID dxsSourceXtwoxmm, gcsSourceXtwoxmm, lasSourceXtwoxmm WSA The unique ID of the neighbour in XMM..twoxmm (=DETID) bigint 8     ID_CATALOG
slaveObjID gcsSourceNeighbours WSA The unique ID of the neighbour in gcsSource (=sourceID) bigint 8     ID_CATALOG
slaveObjID gcsSourceXDR5PhotoObj, lasSourceXDR5PhotoObj WSA The unique ID of the neighbour in BestDR5..PhotoObj (=objID) bigint 8     ID_CATALOG
slaveObjID lasSourceNeighbours WSA The unique ID of the neighbour in lasSource (=sourceID) bigint 8     ID_CATALOG
slaveObjID lasSourceXDR2PhotoObj WSA The unique ID of the neighbour in BestDR2..PhotoObj (=objID) bigint 8     ID_CATALOG
slaveObjID lasSourceXDR3PhotoObj WSA The unique ID of the neighbour in BestDR3..PhotoObj (=objID) bigint 8     ID_CATALOG
slaveObjID lasSourceXDR5PhotoObjAll WSA The unique ID of the neighbour in BestDR5..PhotoObjAll (=objID) bigint 8     ID_CATALOG
slaveObjID lasSourceXDR7PhotoObjAll, lasSourceXStripe82PhotoObjAll WSA The unique ID of the neighbour in BestDR7..PhotoObjAll (=objID) bigint 8     ID_CATALOG
slaveObjID lasSourceXSegueDR6PhotoObj WSA The unique ID of the neighbour in SegueDR6..PhotoObj (=objID) bigint 8     ID_CATALOG
slaveObjID lasSourceXSegueDR6PhotoObjAll WSA The unique ID of the neighbour in SEGUEDR6..PhotoObjAll (=objID) bigint 8     ID_CATALOG
slaveObjID lasSourceXfirstSource WSA The unique ID of the neighbour in FIRST..firstSource (=seqNo) bigint 8     ID_CATALOG
slaveObjID lasSourceXiras_psc WSA The unique ID of the neighbour in IRAS..iras_psc (=seqNo) bigint 8     ID_CATALOG
slaveObjID lasSourceXmgcDetection WSA The unique ID of the neighbour in MGC..mgcDetection (=objID) bigint 8     ID_CATALOG
slaveObjID lasSourceXnvssSource WSA The unique ID of the neighbour in NVSS..nvssSource (=seqNo) bigint 8     ID_CATALOG
slaveObjID lasSourceXrosat_bsc WSA The unique ID of the neighbour in ROSAT..rosat_bsc (=seqNo) bigint 8     ID_CATALOG
slaveObjID lasSourceXrosat_fsc WSA The unique ID of the neighbour in ROSAT..rosat_fsc (=seqNo) bigint 8     ID_CATALOG
slaveObjID lasSourceXtwomass_xsc WSA The unique ID of the neighbour in TWOMASS..twomass_xsc (=ext_key) bigint 8     ID_CATALOG
smoothing MultiframeDetector WSA FWHM of the smoothing kernel {catalogue extension keyword:  FILTFWHM} real 4 pixels -0.9999995e9  
smoothing MultiframeDetector WSACalib FWHM of the smoothing kernel {catalogue extension keyword:  FILTFWHM} real 4 pixels -0.9999995e9  
smoothing MultiframeDetector WSATransit FWHM of the smoothing kernel {catalogue extension keyword:  FILTFWHM} real 4 pixels -0.9999995e9  
SN1 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Signal/Noise for band 1 flux real 4   -9.99  
SN2 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Signal/Noise for band 2 flux real 4   -9.99  
SN3 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Signal/Noise for band 3 flux real 4   -9.99  
SN3_6 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE 3.6um IRAC (Band 1) Signal/Noise real 4   -9.99  
SN4 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Signal/Noise for band 4 flux real 4   -9.99  
SN4_5 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE 4.5um IRAC (Band 2) Signal/Noise real 4   -9.99  
SN5_8 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE 5.8um IRAC (Band 3) Signal/Noise real 4   -9.99  
SN8_0 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE 8.0um IRAC (Band 4) Signal/Noise real 4   -9.99  
SNH glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE 2MASS All-Sky PSC H Band Signal/Noise real 4   -9.99  
SNJ glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE 2MASS All-Sky PSC J Band Signal/Noise real 4   -9.99  
SNKs glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE 2MASS All-Sky PSC Ks Band Signal/Noise real 4   -9.99  
sourceID calListRemeasurement, calSource, calSourceXSynopticSourceBestMatch, calVariability WSACalib UID (unique over entire WSA via programme ID prefix) of this merged detection as assigned by merge algorithm bigint 8     ID_MAIN
sourceID calSourceRemeasurement WSACalib UID (unique over entire WSA via programme ID prefix) of this list remeasurement bigint 8     ID_MAIN
sourceID dxsJKsource, dxsListRemeasurement, dxsSource, dxsSourceXDetectionBestMatch, dxsVariability, gcsListRemeasurement, gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsListRemeasurement, gpsPointSource, gpsSource, lasExtendedSource, lasListRemeasurement, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, udsListRemeasurement, udsSource, udsSourceXDetectionBestMatch, udsVariability WSA UID (unique over entire WSA via programme ID prefix) of this merged detection as assigned by merge algorithm bigint 8     ID_MAIN
sourceID dxsSourceRemeasurement, gcsSourceRemeasurement, gpsSourceRemeasurement, lasSourceRemeasurement, udsSourceRemeasurement WSA UID (unique over entire WSA via programme ID prefix) of this list remeasurement bigint 8     ID_MAIN
sourceID iras_asc IRAS Source ID varchar 15     ID_ALTERNATIVE
sourceIDName ExternalSurveyTable WSA The source unique identifier in the table varchar 256     ID_TARGET
sourceIDName ExternalSurveyTable WSACalib The source unique identifier in the table varchar 256     ID_TARGET
sourceIDName ExternalSurveyTable WSATransit The source unique identifier in the table varchar 256     ID_TARGET
sourceIDName ProgrammeTable WSA the name of the source varchar 256     ID_TARGET
sourceIDName ProgrammeTable WSACalib the name of the source varchar 256     ID_TARGET
sourceIDName ProgrammeTable WSATransit the name of the source varchar 256     ID_TARGET
sourceRemeasTable Programme WSA Table name of co-located list re-measurements varchar 64     ??
sourceRemeasTable Programme WSACalib Table name of co-located list re-measurements varchar 64     ??
sourceRemeasTable Programme WSATransit Table name of co-located list re-measurements varchar 64     ??
sourceTable Programme WSA Table name of merged sources varchar 64     ??
sourceTable Programme WSACalib Table name of merged sources varchar 64     ??
sourceTable Programme WSATransit Table name of merged sources varchar 64     ??
SPEC_TYPE mgcGalaxyStruct MGC SPD's CONTINUUM type (1=El 15.0, 2=Sa 7.4, 3=SC 2.2) tinyint 1   0  
SPECTRA twoxmm XMM The flag is set to True if this source has a spectrum made in at least one exposure. varchar 5      
SQF3_6 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Source Quality Flag for 3.6um IRAC (Band 1) int 4   -9  
SQF4_5 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Source Quality Flag for 4.5um IRAC (Band 2) int 4   -9  
SQF5_8 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Source Quality Flag for 5.8um IRAC (Band 3) int 4   -9  
SQF8_0 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Source Quality Flag for 8.0um IRAC (Band 4) int 4   -9  
SQFH glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE 2MASS All-Sky PSC H Band Source Quality Flag int 4   -9  
SQFJ glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE 2MASS All-Sky PSC J Band Source Quality Flag int 4   -9  
SQFKs glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE 2MASS All-Sky PSC Ks Band Source Quality Flag int 4   -9  
SQL1 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Source Quality Flag for band 1 flux int 4   -9  
SQL2 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Source Quality Flag for band 2 flux int 4   -9  
SQL3 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Source Quality Flag for band 3 flux int 4   -9  
SQL4 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Source Quality Flag for band 4 flux int 4   -9  
SRC_NUM twoxmm XMM The (decimal) source number in the individual source list for this observation; in the hexadecimal system it identifies the source-specific product files belonging to this detection. int 4      
srcCps rosat_bsc, rosat_fsc ROSAT source countrate in the broad energy band, vignetting corrected real 4 counts/sec   PHOT_COUNT-RATE_X
srcdens1 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Local source density for band 1 real 4 #/sqamin -9.9  
srcdens2 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Local source density for band 2 real 4 #/sqamin -9.9  
srcdens3 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Local source density for band 3 real 4 #/sqamin -9.9  
srcdens3_6 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Local source density for 3.6um IRAC (Band 1) real 4 arcmin**-2 -9.9  
srcdens4 glimpse_hrc_inter, glimpse_mca_inter GLIMPSE Local source density for band 4 real 4 #/sqamin -9.9  
srcdens4_5 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Local source density for 4.5um IRAC (Band 2) real 4 arcmin**-2 -9.9  
srcdens5_8 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Local source density for 5.8um IRAC (Band 3) real 4 arcmin**-2 -9.9  
srcdens8_0 glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE Local source density for 8.0um IRAC (Band 4) real 4 arcmin**-2 -9.9  
SRCID twoxmm XMM A unique number assigned to a group of catalogue entries which are assumed to be the same source. To identify members of the same group the distance in arcseconds between each pair of sources was compared on the two-sigma level of both positional errors. A maximum distance of 7" was assumed, which was reduced to 0.9 * DIST_NN (distance to the nearest neighbour) where necessary. int 4      
srcID rosat_bsc, rosat_fsc ROSAT SASS source number (MASOL number) in SASS field varchar 4     ID_NUMBER
SRCID_2XMMP twoxmm XMM The source ID of the 2XMMp unique source matched within radius of 3" and using the closest candidate. int 4      
srcl rosat_bsc, rosat_fsc ROSAT likelihood of source detection smallint 2     STAT_LIKELIHOOD
srcName glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca GLIMPSE GLIMPSEI Highly Reliable Catalogue source name varchar 32     ID_MAIN
srcName glimpse_hrc_inter GLIMPSE GLIMPSE Highly Reliable Catalogue source name varchar 32     ID_MAIN
srcName glimpse_mca_inter GLIMPSE GLIMPSE More Complete Archive source name varchar 32     ID_MAIN
srcName rosat_bsc, rosat_fsc ROSAT ROSAT All-Sky Survey Catalogue source name varchar 16     ID_MAIN
ssTemp Multiframe WSA CCC 2nd stage temperature {image primary HDU keyword: SS_TEMP} real 4 degrees_Kelvin -0.9999995e9  
ssTemp Multiframe WSACalib CCC 2nd stage temperature {image primary HDU keyword: SS_TEMP} real 4 degrees_Kelvin -0.9999995e9  
ssTemp Multiframe WSATransit CCC 2nd stage temperature {image primary HDU keyword: SS_TEMP} real 4 degrees_Kelvin -0.9999995e9  
stackRadius RequiredStack WSA radius within which intermediate stacks are selected for this deep stack. real 4 deg -0.9999995e9  
stackRadius RequiredStack WSACalib radius within which intermediate stacks are selected for this deep stack. real 4 deg -0.9999995e9  
stackRadius RequiredStack WSATransit radius within which intermediate stacks are selected for this deep stack. real 4 deg -0.9999995e9  
standard Multiframe WSA Is target a standard star observation (0=F, 1=T)? {image primary HDU keyword: STANDARD} tinyint 1     OBS_ID
standard Multiframe WSACalib Is target a standard star observation (0=F, 1=T)? {image primary HDU keyword: STANDARD} tinyint 1     OBS_ID
standard Multiframe WSATransit Is target a standard star observation (0=F, 1=T)? {image primary HDU keyword: STANDARD} tinyint 1     OBS_ID
startCol MultiframeDetector WSA Start column of array readout {image extension keyword: RDOUT_X1} smallint 2     NUMBER
startCol MultiframeDetector WSACalib Start column of array readout {image extension keyword: RDOUT_X1} smallint 2     NUMBER
startCol MultiframeDetector WSATransit Start column of array readout {image extension keyword: RDOUT_X1} smallint 2     NUMBER
startDate AstrCalVers WSA MJD of the start time for this version of the calibration float 8 Julian days   TIME_DATE
startDate AstrCalVers WSACalib MJD of the start time for this version of the calibration float 8 Julian days   TIME_DATE
startDate AstrCalVers WSATransit MJD of the start time for this version of the calibration float 8 Julian days   TIME_DATE
startDate PhotCalVers WSA Date time of start time for this version of the calibration (MM-DD-YYYY) datetime 8 MM-DD-YYYY 12-31-9999 TIME_DATE
startDate PhotCalVers WSACalib Date time of start time for this version of the calibration (MM-DD-YYYY) datetime 8 MM-DD-YYYY 12-31-9999 TIME_DATE
startDate PhotCalVers WSATransit Date time of start time for this version of the calibration (MM-DD-YYYY) datetime 8 MM-DD-YYYY 12-31-9999 TIME_DATE
startRow MultiframeDetector WSA Start row of array readout {image extension keyword: RDOUT_Y1} smallint 2     NUMBER
startRow MultiframeDetector WSACalib Start row of array readout {image extension keyword: RDOUT_Y1} smallint 2     NUMBER
startRow MultiframeDetector WSATransit Start row of array readout {image extension keyword: RDOUT_Y1} smallint 2     NUMBER
status ProgrammeCurationHistory WSA successful (1) or unsuccessful (0) tinyint 1     CODE_MISC
status ProgrammeCurationHistory WSACalib successful (1) or unsuccessful (0) tinyint 1     CODE_MISC
status ProgrammeCurationHistory WSATransit successful (1) or unsuccessful (0) tinyint 1     CODE_MISC
stdCRms CurrentAstrometry WSACalib RMS residual of fit to astrometric standards {image extension keyword: STDCRMS} float 8   -0.9999995e9 FIT_RESIDUAL
stdCRms CurrentAstrometry WSATransit RMS residual of fit to astrometric standards {image extension keyword: STDCRMS} float 8   -0.9999995e9 FIT_RESIDUAL
stdCRms CurrentAstrometry, PreviousAstrometry WSA RMS residual of fit to astrometric standards {image extension keyword: STDCRMS} float 8   -0.9999995e9 FIT_RESIDUAL
STEL mgcDetection MGC Stellaricity real 4      
SUM_FLAG twoxmm XMM The summary flag of the source is derived from EP_FLAG. It is 0 if none of the nine flags was set; it is set to 1 if at least one of the warning flags (flag 1, 2, 3, 9) was set but no possible-spurious-detection flag (flag 7, 8); it is set to 2 if at least one of the possible-spurious-detection flags (flag 7, 8) was set but not the manual flag (flag 11); it is set to 3 if the manual flag (flag 11) was set but no possible-spurious-detection flags (flag 7, 8); it is set to 4 if the manual flag (flag 11) as well as one of the possible-spurious-detection flags (flag 7, 8) is set. The meaning is thus: 0 = good, 1 = source parameters may be affected, 2 = possibly spurious, 3 = located in a area where spurious detection may occur, 4 = located in a area where spurious detection may occur and possibly spurious. . int 4      
sup_ba twomass_xsc 2MASS Minor/major axis ratio fit to 3-sig. super-coadd isophote. real 4     PHYS_AXIS-RATIO
sup_chif_ellf twomass_xsc 2MASS super-coadd % chi-fraction for ellip. fit to 3-sig isophote. real 4     FIT_PARAM_VALUE
sup_dec twomass_xsc 2MASS Super-coadd centroid Dec (J2000 decimal deg). float 8 degrees   POS_EQ_DEC_MAIN
sup_phi twomass_xsc 2MASS Super-coadd angle to major axis (E of N). smallint 2 degrees   POS_POS-ANG
sup_r_3sig twomass_xsc 2MASS Super-coadd 3-sigma isophotal semi-major axis radius. real 4 arcsec   ERROR
sup_ra twomass_xsc 2MASS Super-coadd centroid RA (J2000 decimal deg). float 8 degrees   POS_EQ_RA_MAIN
survey Multiframe WSA Survey description {image primary HDU keyword: SURVEY} varchar 64   NONE ??
survey Multiframe WSACalib Survey description {image primary HDU keyword: SURVEY} varchar 64   NONE ??
survey Multiframe WSATransit Survey description {image primary HDU keyword: SURVEY} varchar 64   NONE ??
surveyID ExternalSurvey WSACalib the unique identifier for the survey int 4     ID_SURVEY
surveyID ExternalSurvey WSATransit the unique identifier for the survey int 4     ID_SURVEY
surveyID ExternalSurvey, ExternalSurveyTable, Release, RequiredNeighbours WSA the unique identifier for the survey int 4     ID_SURVEY
surveyID RequiredListDrivenProduct WSA the unique ID of the external survey (if applicable) int 4   -99999999 ID_SURVEY
surveyID RequiredListDrivenProduct WSACalib the unique ID of the external survey (if applicable) int 4   -99999999 ID_SURVEY
surveyID RequiredListDrivenProduct WSATransit the unique ID of the external survey (if applicable) int 4   -99999999 ID_SURVEY
surveyID Survey WSACalib The unique identifier for the curated survey int 4     ID_SURVEY
surveyID Survey WSATransit The unique identifier for the curated survey int 4     ID_SURVEY
surveyID Survey, SurveyProgrammes WSA The unique identifier for the curated survey int 4     ID_SURVEY
surveyName ExternalSurvey WSA The short name of the survey, eg. SDSS-EDR, SDSS-DR1, USNOB etc. varchar 32     ??
surveyName ExternalSurvey WSACalib The short name of the survey, eg. SDSS-EDR, SDSS-DR1, USNOB etc. varchar 32     ??
surveyName ExternalSurvey WSATransit The short name of the survey, eg. SDSS-EDR, SDSS-DR1, USNOB etc. varchar 32     ??
synFrameSetID calSourceXSynopticSourceBestMatch WSACalib the UID of the relevant frame set bigint 8     ID_FRAME
synFrameSetID calSynopticMergeLog WSACalib frame set ID, unique over the whole WSA via programme ID prefix, assigned by merging procedure bigint 8     ID_FIELD
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, lasSource.frameSetID references lasMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
synFrameSetID calSynopticSource WSACalib UID of the set of frames that this merged source comes from bigint 8     REFER_CODE
Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, lasSource.frameSetID references lasMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
synopticBestMatchTable Programme WSA Table name of merged variable sources varchar 64     ??
synopticBestMatchTable Programme WSACalib Table name of merged variable sources varchar 64     ??
synopticBestMatchTable Programme WSATransit Table name of merged variable sources varchar 64     ??
synopticID calSynopticSource WSACalib UID (unique over entire WSA via programme ID prefix) of this merged detection as assigned by merge algorithm bigint 8     ID_MAIN
synopticSourceTable Programme WSA Table name of merged variable sources varchar 64     ??
synopticSourceTable Programme WSACalib Table name of merged variable sources varchar 64     ??
synopticSourceTable Programme WSATransit Table name of merged variable sources varchar 64     ??
synSeqNum calSourceXSynopticSourceBestMatch, calSynopticSource WSACalib the running number of this source {catalogue TType keyword: Sequence_number}
The running number in this frameSet for ease of reference, in order of matching.
int 4     ID_NUMBER
sys_flg twomass_xsc 2MASS system flag: 0=no system, 1=nearby galaxy flux incl. in mag. smallint 2     CODE_MISC
SYSERR twoxmm XMM The systematic 1 σ error on the detection position in arcseconds. It is set to be 0.35 arcsec if the SAS task eposcorr results in a statistically reliable cross-correlation with USNO B1.0 optical catalogue. Otherwise the error is 1.0 arsec. real 4 arcsec    



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23/02/2010