WSA Browser

Glossary of WSA attributes

This Glossary alphabetically lists all attributes used in the UKIDSSDR9 database(s) held in the WSA. If you would like to have more information about the schema tables please use the UKIDSSDR9 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

Name Schema Table Database Description Type Length Unit Default Value Unified Content Descriptor

S14 nvssSource NVSS Integrated 1.4GHz flux density of radio source real 4 mJy PHOT_FLUX_RADIO_1.4G

satnum wise_prelimsc WISE Minimum sample at which saturation occurs in each band
Four character string, one character per band, that indicates the minimum SUTR sample in which any pixel in the profile-fitting area in all of the single-exposure images used to characterize this source was flagged as having reached the saturation level in the on-board WISE payload processing. If no pixels in a given band are flagged as saturated, the value for that band is "0". char 4

SC_CHI2PROB twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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_DR_FIRST twoxmmi_dr3_v1_0 XMM This flag indicates in which catalogue in the 2XMM catalogue series (starting from 2XMM) this unique source first appeared. The flag is DR1 for 2XMM, DR2 for 2XMMi and DR3 for the present 2XMMi-DR3 catalogue. int 4

SC_DR_LAST twoxmmi_dr3_v1_0 XMM This flag indicates in which catalogue in the 2XMM catalogue series (starting from 2XMM) the parameters of this unique source were last updated (e.g. due to the inclusion of one or more new detections which can add to, or even split, the source). The flag is DR1 for 2XMM, DR2 for 2XMMi and DR3 for the present 2XMMi-DR3 catalogue. int 4

SC_EP_1_FLUX twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 XMM Error on the weighted mean band 9 flux in SC_EP_9_FLUX. real 4 erg/cm**2/s

SC_EXT_ML twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 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_EXTENT twoxmmi_dr3_v1_0 XMM The total band extent of the source SRCID is the weighted average of the EPIC extents of all detections of this source (EP_EXTENT). real 4 arcsec

SC_HR1 twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 XMM Error on the weighted mean hardness ratio in SC_HR1. real 4

SC_HR2 twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 XMM Error on the weighted mean hardness ratio in SC_HR2. real 4

SC_HR3 twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 XMM Error on the weighted mean hardness ratio in SC_HR3. real 4

SC_HR4 twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 XMM Error on the weighted mean hardness ratio in SC_HR4. real 4

SC_POSERR twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 XMM The error of the weighted mean position given in SC_RA and SC_DEC in arcseconds. real 4 arcsec

SC_RA twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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_sixx2_scn 2MASS scan number (unique within date) smallint 2

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_sixx2_xsc 2MASS key to scan data record in "scan DB" int 4

scan_key twomass_xsc 2MASS key to scan data record in "scan DB". int 4 ID_NUMBER

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

sd twomass_sixx2_scn 2MASS direction of scan -- north/south-bound (n/s) varchar 1

sdet twomass_sixx2_psc, twomass_sixx2_xsc 2MASS # of scans in which src was detected in >=1 band smallint 2

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

sdssClass first08Jul16Source FIRST morphological classification in SDSS DR6 (s=stellar, g=nonstellar/galaxy) varchar 1

sdssMag first08Jul16Source FIRST SDSS i magnitude real 4 mag

sdssMatches first08Jul16Source FIRST number of matches within a fiducial radius (8 arcsec) with SDSS DR6 int 4

sdssPrimary dxsSourceXDR7PhotoObj, dxsSourceXDR8PhotoObj, dxsSourceXStripe82PhotoObjAll, gcsSourceXDR5PhotoObj, gcsSourceXDR7PhotoObj, gcsSourceXDR8PhotoObj, lasSourceXDR2PhotoObj, lasSourceXDR3PhotoObj, lasSourceXDR5PhotoObj, lasSourceXDR5PhotoObjAll, lasSourceXDR7PhotoObj, lasSourceXDR7PhotoObjAll, lasSourceXDR8PhotoObj, lasSourceXDR8PhotoObjAll, lasSourceXSegueDR6PhotoObj, lasSourceXSegueDR6PhotoObjAll, lasSourceXStripe82PhotoObjAll WSA SDSS flag for neighbour being primary (1) or secondary (0) tinyint 1 CODE_MISC

sdssSep first08Jul16Source FIRST separation of the nearest match in SDSS DR6 from the FIRST position real 4 arcsec

sdssType dxsSourceXDR7PhotoObj, dxsSourceXDR8PhotoObj, dxsSourceXStripe82PhotoObjAll, gcsSourceXDR5PhotoObj, gcsSourceXDR7PhotoObj, gcsSourceXDR8PhotoObj, lasSourceXDR2PhotoObj, lasSourceXDR3PhotoObj, lasSourceXDR5PhotoObj, lasSourceXDR5PhotoObjAll, lasSourceXDR7PhotoObj, lasSourceXDR7PhotoObjAll, lasSourceXDR8PhotoObj, lasSourceXDR8PhotoObjAll, 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 ??

secFocalOffset Multiframe WSA Secondary mirror focal offset, introduced in May 2010. This will be 0 for normal science frames, but will have other values when the secondary is moved to achieve the best focus {image primary HDU keyword: FOC_TOFF} real 4 -0.9999995e9 ??

secFocalOffset Multiframe WSACalib Secondary mirror focal offset, introduced in May 2010. This will be 0 for normal science frames, but will have other values when the secondary is moved to achieve the best focus {image primary HDU keyword: FOC_TOFF} real 4 -0.9999995e9 ??

secFocalOffset Multiframe WSATransit Secondary mirror focal offset, introduced in May 2010. This will be 0 for normal science frames, but will have other values when the secondary is moved to achieve the best focus {image primary HDU keyword: FOC_TOFF} real 4 -0.9999995e9 ??

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, twoxmm_v1_2 XMM The distance between this source and the matched 1XMM source (MATCH_1XMM) in arcseconds. real 4 arcsec

SEP_2XMMP twoxmm, twoxmm_v1_2 XMM The distance between this source and the matched 2XMMp source (MATCH_2XMMp) in arcseconds. real 4 arcsec

seqNo first08Jul16Source, 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, dxsOrphan, 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

seqNum twomass_sixx2_psc 2MASS Sequential number (unique object ID) int 4

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, 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, 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, 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, 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, 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, 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, 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, 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, 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, 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, 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, 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

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 ??

siga dxsAstrometricInfo, udsAstrometricInfo WSA Error on coefficient a float 8 arcsec -0.9999995e9 ??

sigd dxsAstrometricInfo, udsAstrometricInfo WSA Error on coefficient d float 8 arcsec -0.9999995e9 ??

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 dxsVariability WSA Uncertainty in mean Dec real 4 Degrees -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 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 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.

sigdec wise_prelimsc WISE One-sigma uncertainty in declination coordinate
CAUTION: The declination uncertainty is overestimated for the majority of sources in the Preliminary Release Source Catalog. Sigdec was computed by adding 0.5 arcsec in quadrature to the extraction measurement uncertainty to reflect the impact of the declination bias error known to affect a fraction of source fainter than W1~13.0 mag real 4 arcsec

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 dxsVariability WSA Uncertainty in mean RA real 4 Degrees -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 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 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.

sigra wise_prelimsc WISE One-sigma uncertainty in right ascension coordinate real 4 arcsec

sigradec wise_prelimsc WISE The co-sigma of the equatorial position uncertainties, (sig_ra, sig_dec) real 4 degrees

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, 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, 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 dxsSourceXDR8PhotoObj, gcsSourceXDR8PhotoObj, lasSourceXDR8PhotoObj WSA The unique ID of the neighbour in BestDR8..PhotoObj (=objID) bigint 8 ID_CATALOG

slaveObjID dxsSourceXDetection WSA The unique ID of the neighbour in dxsDetection (=objID) bigint 8 ID_CATALOG

slaveObjID dxsSourceXGR6PhotoObjAll, gcsSourceXGR6PhotoObjAll, lasSourceXGR6PhotoObjAll WSA The unique ID of the neighbour in GALEXGR6..PhotoObjAll (=seqNo) bigint 8 ID_CATALOG

slaveObjID dxsSourceXSSASource, gcsSourceXSSASource, lasSourceXSSASource WSA The unique ID of the neighbour in SSA..Source (=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 dxsSourceXwise_prelimsc, gcsSourceXwise_prelimsc, lasSourceXwise_prelimsc WSA The unique ID of the neighbour in WISE..wise_prelimsc (=pts_key) 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 lasSourceXDR8PhotoObjAll WSA The unique ID of the neighbour in BestDR8..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

source_id wise_prelimsc WISE Unique source ID, formed from a combination of the Atlas Tile ID, coadd_id, and sequential extracted source number, src, within the Tile char 28

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, 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 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

sourceProb first08Jul16Source FIRST probability that the source is spurious (most commonly because it is a sidelobe of of a nearby bright source.) Low values mean the source is unlikely to be spurious. float 8 CODE_MISC

sourceProdType Programme WSA The product type to be used to create the source table. (stack, tile, mosaic) varchar 16 NONE

sourceProdType Programme WSACalib The product type to be used to create the source table. (stack, tile, mosaic) varchar 16 NONE

sourceProdType Programme WSATransit The product type to be used to create the source table. (stack, tile, mosaic) varchar 16 NONE

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, twoxmm_v1_2, twoxmmi_dr3_v1_0 XMM The flag is set to True if this source has a spectrum made in at least one exposure. varchar 5

spos twomass_sixx2_psc, twomass_sixx2_xsc 2MASS # of scans in which src position falls inside coverage area smallint 2

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 wise_prelimsc WISE Sequential number of this source extraction in the Atlas Tile from which this source was extracted, in approximate descending order of W1 source brightness bigint 8

SRC_NUM twoxmm, twoxmm_v1_2, twoxmmi_dr3_v1_0 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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_2XMMi twoxmmi_dr3_v1_0 XMM The unique source ID of the detection, DETID, in the 2XMMi catalogue. Due to the nature of the matching algorithm, some detections were re-assigned to a different source due to the presence of new detections. int 4

SRCID_2XMMP twoxmm, twoxmm_v1_2 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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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_sixx2_xsc 2MASS minor/major axis ratio fit to 3-sig. super-coadd isophote real 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_sixx2_xsc 2MASS super-coadd angle to major axis (E of N) smallint 2 deg

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, twoxmm_v1_2, twoxmmi_dr3_v1_0 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

WFAU, Institute for Astronomy,
Royal Observatory, Blackford Hill
Edinburgh, EH9 3HJ, UK
Tel +44 131 668 8356 (office)
or +44 131 668 8100 (switchboard)

wsa-support@roe.ac.uk
04/04/2012