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 |
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 |
scanlen |
Plate |
SSA |
SuperCOSMOS CCD lane scan length |
smallint |
2 |
pixels |
|
INST_PARAM |
scanMaterial |
Plate |
SSA |
Photographic medium, eg. Original glass, Copy film, Copy glass |
varchar |
16 |
|
|
REMARKS |
scdGrid |
Plate |
SSA |
Non-linear distortion mask filename |
varchar |
80 |
|
|
ID_FILE |
sCorMagB |
CompleteStars, ReliableGalaxies, ReliableStars, Source |
SSA |
B band magnitude assuming object is star |
real |
4 |
mag |
-99.999995 |
PHOT_PHG_BJ |
sCorMagI |
CompleteStars, ReliableGalaxies, ReliableStars, Source |
SSA |
I band magnitude assuming object is star |
real |
4 |
mag |
-99.999995 |
PHOT_PHG_I |
sCorMagR1 |
CompleteStars, ReliableGalaxies, ReliableStars, Source |
SSA |
R1 band magnitude assuming object is star |
real |
4 |
mag |
-99.999995 |
PHOT_PHG_R |
sCorMagR2 |
CompleteStars, ReliableGalaxies, ReliableStars, Source |
SSA |
R2 band magnitude assuming object is star |
real |
4 |
mag |
-99.999995 |
PHOT_PHG_R |
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, gcsSourceXDR5PhotoObj, gcsSourceXDR7PhotoObj, lasSourceXDR2PhotoObj, lasSourceXDR3PhotoObj, lasSourceXDR5PhotoObj, lasSourceXDR5PhotoObjAll, lasSourceXDR7PhotoObj, lasSourceXDR7PhotoObjAll, lasSourceXSegueDR6PhotoObj, lasSourceXSegueDR6PhotoObjAll |
WSA |
SDSS flag for neighbour being primary (1) or secondary (0) |
tinyint |
1 |
|
|
CODE_MISC |
sdssType |
dxsSourceXDR7PhotoObj, gcsSourceXDR5PhotoObj, gcsSourceXDR7PhotoObj, lasSourceXDR2PhotoObj, lasSourceXDR3PhotoObj, lasSourceXDR5PhotoObj, lasSourceXDR5PhotoObjAll, lasSourceXDR7PhotoObj, lasSourceXDR7PhotoObjAll, lasSourceXSegueDR6PhotoObj, lasSourceXSegueDR6PhotoObjAll |
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 |
?? |
seam |
Detection |
SSA |
Seam index: = zero or SSAfield for seamless selection |
smallint |
2 |
|
|
ID_FIELD |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
|
|
shiftPnt |
Plate |
SSA |
Shift of from nominal to fitted plate centre |
float |
8 |
radians |
|
POS_OFFSET |
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 |
CompleteStars, ReliableGalaxies, ReliableStars, Source |
SSA |
Uncertainty in Dec (formal random error not inc. systematic errors) |
float |
8 |
degrees |
|
ERROR |
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 |
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. |
sigMuAcosD |
CompleteStars, ReliableGalaxies, ReliableStars, Source |
SSA |
Error on proper motion in RA direction |
real |
4 |
mas/yr |
-0.99999995e9 |
ERROR |
sigMuD |
CompleteStars, ReliableGalaxies, ReliableStars, Source |
SSA |
Error on proper motion in Dec direction |
real |
4 |
mas/yr |
-0.99999995e9 |
ERROR |
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 |
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 |
CompleteStars, ReliableGalaxies, ReliableStars, Source |
SSA |
Uncertainty in RA (formal random error not inc. systematic errors) |
float |
8 |
degrees |
|
ERROR |
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 |
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. |
sky |
UKIDSSDetection |
WSA |
local interpolated sky level from background tracker |
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. |
skyDefn |
Plate |
SSA |
Method of defining sky, eg. "median" |
varchar |
16 |
|
|
REDUCT_METHOD |
skyFilter |
Plate |
SSA |
Box filter weights for sky determination |
varchar |
16 |
|
|
REDUCT_PARAM |
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. |
skySquare |
Plate |
SSA |
Blocksize (one side) of sky background |
smallint |
2 |
pixels |
|
REDUCT_PARAM |
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 |
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 |
dxsSourceNeighbours |
WSA |
The unique ID of the neighbour in dxsSource (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
dxsSourceXDR7PhotoObj, 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, gpsSourceXtwomass_psc, lasSourceXtwomass_psc, udsSourceXtwomass_psc |
WSA |
The unique ID of the neighbour in TWOMASS..twomass_psc (=pts_key) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
dxsSourceXtwoxmm, gcsSourceXtwoxmm, gpsSourceXtwoxmm, lasSourceXtwoxmm, udsSourceXtwoxmm |
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 |
gpsSourceNeighbours |
WSA |
The unique ID of the neighbour in gpsSource (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
gpsSourceXglimpse1_hrc |
WSA |
The unique ID of the neighbour in GLIMPSE..glimpse1_hrc (=seqNo) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
gpsSourceXglimpse1_mca |
WSA |
The unique ID of the neighbour in GLIMPSE..glimpse1_mca (=seqNo) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
gpsSourceXglimpse2_hrc |
WSA |
The unique ID of the neighbour in GLIMPSE..glimpse2_hrc (=seqNo) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
gpsSourceXglimpse2_mca |
WSA |
The unique ID of the neighbour in GLIMPSE..glimpse2_mca (=seqNo) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
gpsSourceXglimpse_hrc_inter |
WSA |
The unique ID of the neighbour in GLIMPSE..glimpse_hrc_inter (=seqNo) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
gpsSourceXglimpse_mca_inter |
WSA |
The unique ID of the neighbour in GLIMPSE..glimpse_mca_inter (=seqNo) |
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 |
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 |
slaveObjID |
udsSourceNeighbours |
WSA |
The unique ID of the neighbour in udsSource (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
udsSourceXDetection |
WSA |
The unique ID of the neighbour in udsDetection (=objID) |
bigint |
8 |
|
|
ID_CATALOG |
sMag |
Detection |
SSA |
Magnitude calculated on assumption object is star |
real |
4 |
mag |
|
MODEL_MAG_VALUE |
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 |
|
softVersion |
Plate |
SSA |
Software version, eg. /home/scosdev/v033 |
varchar |
18 |
|
|
ID_VERSION |
sosp |
Plate |
SSA |
SuperCOSMOS start of scan CCD pixel number |
smallint |
2 |
|
|
INST_PARAM |
sourceID |
Detection |
SSA |
objID for corresponding merged record in Source |
bigint |
8 |
|
|
ID_ASSOCIATED |
sourceID |
dxsJKsource, dxsSource, dxsSourceXDetectionBestMatch, dxsVariability, gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableGcsPointSource, reliableGpsPointSource, reliableLasPointSource, reliableUdsSource, 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 |
SSAfield |
Detection |
SSA |
SSS field number (ESO/SRC system) that this detection falls in. |
smallint |
2 |
|
|
ID_FIELD |
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 |
|
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 |
starCat |
Plate |
SSA |
Name of reference star catalogue used for astrometric fit |
varchar |
80 |
|
|
ID_CATALOG |
starsInit |
Plate |
SSA |
No. of refstars in initial astrometric solution |
int |
4 |
|
|
NUMBER |
starsSelec |
Plate |
SSA |
No. of refstars initially selected |
int |
4 |
|
|
NUMBER |
starsUsed |
Plate |
SSA |
No. of refstars in final astrometric solution |
int |
4 |
|
|
NUMBER |
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 |
|
|
|
stepsize |
Plate |
SSA |
SuperCOSMOS nominal pixel size |
real |
4 |
microns |
|
INST_PIXSIZE |
stepWdg |
Plate |
SSA |
Intensity calibration step-wedge type, eg. kpno |
varchar |
16 |
|
|
INST_PARAM |
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 |
Detection |
SSA |
The survey that collected the data |
tinyint |
1 |
|
|
ID_SURVEY |
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 |
Plate |
SSA |
Every plate comes from a survey |
tinyint |
1 |
|
|
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 |
SSA |
Unique survey identifier in the SSA |
tinyint |
1 |
|
|
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 |
|
|
?? |
surveyName |
Survey |
SSA |
Survey name, eg. SERC-J/EJ |
varchar |
16 |
|
|
ID_CATALOG |
surveyRef |
Survey |
SSA |
Literature reference for survey |
varchar |
256 |
|
|
REFER_CODE |
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 |
|
|
?? |
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 |
|
|
?? |
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 |
|
|
systemID |
Field |
SSA |
Unique identifier of the system of survey field centres |
tinyint |
1 |
|
|
ID_MAIN |
systemID |
FieldSystem |
SSA |
The system of survey fields used for the survey |
tinyint |
1 |
|
|
ID_MAIN |
systemID |
Survey |
SSA |
The system of survey fields used for the survey |
tinyint |
1 |
|
|
NOTE |