S |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
scrunch |
[nspid]RequiredMosaic |
WSA NonSurvey |
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 |
[nspid]Multiframe |
WSA NonSurvey |
SCSU cab temperature {image primary HDU keyword: SC_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
sdsuNum |
[nspid]MultiframeDetector |
WSA NonSurvey |
Serial number of SDSU controller {image extension keyword: SDSUID} |
varchar |
32 |
|
NONE |
?? |
secondaryTemp |
[nspid]Multiframe |
WSA NonSurvey |
Temperature of secondary {image primary HDU keyword: SECONDAR} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
seeing |
[nspid]MultiframeDetector |
WSA NonSurvey |
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). |
seqNum |
[nspid]Detection |
WSA NonSurvey |
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 |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
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 |
SerFit1DChi2 |
[nspid]Detection |
WSA NonSurvey |
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 |
SerFit2DChi2 |
[nspid]Detection |
WSA NonSurvey |
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 |
SerFitNu1D |
[nspid]Detection |
WSA NonSurvey |
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 |
SerFitNu2D |
[nspid]Detection |
WSA NonSurvey |
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 |
SerFlux1D |
[nspid]Detection |
WSA NonSurvey |
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 |
SerFlux2D |
[nspid]Detection |
WSA NonSurvey |
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 |
SerIdx1D |
[nspid]Detection |
WSA NonSurvey |
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 |
SerIdx2D |
[nspid]Detection |
WSA NonSurvey |
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 |
SerMag1D |
[nspid]Detection |
WSA NonSurvey |
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 |
SerMag2D |
[nspid]Detection |
WSA NonSurvey |
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 |
SerScaleLen1D |
[nspid]Detection |
WSA NonSurvey |
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 |
SerScaleLen2D |
[nspid]Detection |
WSA NonSurvey |
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 |
server |
[nspid]ExternalSurvey |
WSA NonSurvey |
The location of the database: load or public server |
varchar |
16 |
|
|
?? |
shortName |
[nspid]Filter |
WSA NonSurvey |
Short identification name for the filter |
varchar |
4 |
|
|
?? |
sigDec |
[nspid]Variability |
WSA NonSurvey |
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. |
sigMuDec |
[nspid]Variability |
WSA NonSurvey |
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. |
sigMuRa |
[nspid]Variability |
WSA NonSurvey |
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. |
sigRa |
[nspid]Variability |
WSA NonSurvey |
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 |
[nspid]Detection |
WSA NonSurvey |
local interpolated sky level from background tracker {catalogue TType keyword: Sky_level} |
real |
4 |
ADU |
|
INST_SKY_LEVEL |
skyCorrCat |
[nspid]MultiframeDetector |
WSA NonSurvey |
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 |
[nspid]MultiframeDetector |
WSA NonSurvey |
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 |
[nspid]Multiframe |
WSA NonSurvey |
UID of library calibration sky sub frame {image extension keyword: SKYSUB} |
bigint |
8 |
|
-99999999 |
ID_FRAME |
skyLevel |
[nspid]MultiframeDetector |
WSA NonSurvey |
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 |
[nspid]MultiframeDetector |
WSA NonSurvey |
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 |
[nspid]MultiframeDetector |
WSA NonSurvey |
Scale factor applied to sky subtraction image {image extension keyword: SKYSUB} |
float |
8 |
|
-0.9999995e9 |
?? |
skyVar |
[nspid]Detection |
WSA NonSurvey |
local estimate of variation in sky level around image {catalogue TType keyword: Sky_rms} |
real |
4 |
ADU |
|
INST_SKY_LEVEL |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u05a37Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u05b15Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u05b7Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u05bd1Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u05bj4Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u06a24Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u06a48Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u06ah43Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u06b13Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u06b24Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u06b36Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u07b29Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u07b36Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u07bd3Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u07bd4Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in u07bh49Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1625Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1636Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1650Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1652Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1672Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1673Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1674Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1678Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1706Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1707Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1708Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1711Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1731Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1741Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1743Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID of the neighbour in userv1761Source (=sourceID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceXDetection |
WSA NonSurvey |
The unique ID of the neighbour in userv1707Detection (=objID) |
bigint |
8 |
|
|
ID_CATALOG |
slaveObjID |
[nspid]SourceXtwomass_psc |
WSA NonSurvey |
The unique ID of the neighbour in TWOMASS..twomass_psc (=pts_key) |
bigint |
8 |
|
|
ID_CATALOG |
smoothing |
[nspid]MultiframeDetector |
WSA NonSurvey |
FWHM of the smoothing kernel {catalogue extension keyword: FILTFWHM} |
real |
4 |
pixels |
-0.9999995e9 |
|
sourceID |
[nspid]Source, [nspid]SourceXDetectionBestMatch, [nspid]Variability |
WSA NonSurvey |
UID (unique over entire WSA via programme ID prefix) of this merged detection as assigned by merge algorithm |
bigint |
8 |
|
|
ID_MAIN |
sourceIDName |
[nspid]ExternalSurveyTable |
WSA NonSurvey |
The source unique identifier in the table |
varchar |
256 |
|
|
ID_TARGET |
sourceIDName |
[nspid]ProgrammeTable |
WSA NonSurvey |
the name of the source |
varchar |
256 |
|
|
ID_TARGET |
sourceRemeasTable |
[nspid]Programme |
WSA NonSurvey |
Table name of co-located list re-measurements |
varchar |
64 |
|
|
?? |
sourceTable |
[nspid]Programme |
WSA NonSurvey |
Table name of merged sources |
varchar |
64 |
|
|
?? |
ssTemp |
[nspid]Multiframe |
WSA NonSurvey |
CCC 2nd stage temperature {image primary HDU keyword: SS_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
standard |
[nspid]Multiframe |
WSA NonSurvey |
Is target a standard star observation (0=F, 1=T)? {image primary HDU keyword: STANDARD} |
tinyint |
1 |
|
|
OBS_ID |
startCol |
[nspid]MultiframeDetector |
WSA NonSurvey |
Start column of array readout {image extension keyword: RDOUT_X1} |
smallint |
2 |
|
|
NUMBER |
startDate |
[nspid]AstrCalVers |
WSA NonSurvey |
MJD of the start time for this version of the calibration |
float |
8 |
Julian days |
|
TIME_DATE |
startDate |
[nspid]PhotCalVers |
WSA NonSurvey |
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 |
[nspid]MultiframeDetector |
WSA NonSurvey |
Start row of array readout {image extension keyword: RDOUT_Y1} |
smallint |
2 |
|
|
NUMBER |
status |
[nspid]ProgrammeCurationHistory |
WSA NonSurvey |
successful (1) or unsuccessful (0) |
tinyint |
1 |
|
|
CODE_MISC |
stdCRms |
[nspid]CurrentAstrometry, [nspid]PreviousAstrometry |
WSA NonSurvey |
RMS residual of fit to astrometric standards {image extension keyword: STDCRMS} |
float |
8 |
|
-0.9999995e9 |
FIT_RESIDUAL |
survey |
[nspid]Multiframe |
WSA NonSurvey |
Survey description {image primary HDU keyword: SURVEY} |
varchar |
64 |
|
NONE |
?? |
surveyID |
[nspid]ExternalSurvey, [nspid]ExternalSurveyTable, [nspid]Release, [nspid]RequiredNeighbours |
WSA NonSurvey |
the unique identifier for the survey |
int |
4 |
|
|
ID_SURVEY |
surveyID |
[nspid]RequiredListDrivenProduct |
WSA NonSurvey |
the unique ID of the external survey (if applicable) |
int |
4 |
|
-99999999 |
ID_SURVEY |
surveyID |
[nspid]Survey, [nspid]SurveyProgrammes |
WSA NonSurvey |
The unique identifier for the curated survey |
int |
4 |
|
|
ID_SURVEY |
surveyName |
[nspid]ExternalSurvey |
WSA NonSurvey |
The short name of the survey, eg. SDSS-EDR, SDSS-DR1, USNOB etc. |
varchar |
32 |
|
|
?? |
synopticBestMatchTable |
[nspid]Programme |
WSA NonSurvey |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |
synopticSourceTable |
[nspid]Programme |
WSA NonSurvey |
Table name of merged variable sources |
varchar |
64 |
|
|
?? |