Y |
| Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
| y |
allwise_sc |
WISE |
Unit sphere position y value |
float |
8 |
|
|
|
| y_coadd |
twomass_xsc |
TWOMASS |
y (in-scan) position (coadd coord.). |
real |
4 |
arcsec |
|
pos.cartesian;instr.det |
| yABMagLim |
allSkyNIRFrameSetInfo |
VULCANiDR |
AB magnitude limit of pointing in J band |
float |
8 |
mag |
|
|
| yAllAperMag3 |
allSkyNIRSource |
VULCANiDR |
Default point source Y aperture corrected mag (2.0 arcsec aperture diameter) using All Sky calibration If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yAllAperMag3Err |
allSkyNIRSource |
VULCANiDR |
Error in default point/extended source Y mag (2.0 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| yAllAperMag4 |
allSkyNIRSource |
VULCANiDR |
Point source Y aperture corrected mag (2.8 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yAllAperMag4Err |
allSkyNIRSource |
VULCANiDR |
Error in point/extended source Y mag (2.8 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| yAllAperMag6 |
allSkyNIRSource |
VULCANiDR |
Point source Y aperture corrected mag (5.7 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yAllAperMag6Err |
allSkyNIRSource |
VULCANiDR |
Error in point/extended source Y mag (5.7 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| yAllAperMagNoAperCorr3 |
allSkyNIRSource |
VULCANiDR |
Default extended source Y aperture mag (2.0 arcsec aperture diameter) using All Sky calibration If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yAllAperMagNoAperCorr4 |
allSkyNIRSource |
VULCANiDR |
Extended source Y aperture mag (2.8 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yAllAperMagNoAperCorr6 |
allSkyNIRSource |
VULCANiDR |
Extended source Y aperture mag (5.7 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yAllPetroMag |
allSkyNIRSource |
VULCANiDR |
Extended source Y mag (Petrosian) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yAllPetroMagErr |
allSkyNIRSource |
VULCANiDR |
Error in extended source Y mag (Petrosian) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| yApFillFac |
StackObjectAttributes |
PS1DR2 |
Aperture fill factor from y filter stack detection. |
real |
4 |
|
-999 |
|
| yApFlux |
StackObjectAttributes |
PS1DR2 |
Aperture flux from y filter stack detection. |
real |
4 |
Janskys |
-999 |
|
| yApFluxErr |
StackObjectAttributes |
PS1DR2 |
Error in aperture flux from y filter stack detection. |
real |
4 |
Janskys |
-999 |
|
| yApMag |
StackObjectThin |
PS1DR2 |
Aperture magnitude from y filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
| yApMagErr |
StackObjectThin |
PS1DR2 |
Error in aperture magnitude from y filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
| yApRadius |
StackObjectAttributes |
PS1DR2 |
Aperture radius for y filter stack detection. |
real |
4 |
arcsec |
-999 |
|
| yClass |
allSkyNIRSource |
VULCANiDR |
discrete image classification flag in Y |
smallint |
2 |
|
-9999 |
src.class&MagUCD& |
| yClassStat |
allSkyNIRSource |
VULCANiDR |
N(0,1) stellarness-of-profile statistic/SExtractor STAR_CLASS in Y |
real |
4 |
|
-0.9999995e9 |
stat&MagUCD& |
| ydec |
StackObjectThin |
PS1DR2 |
Declination from y filter stack detection. |
float |
8 |
degrees |
-999 |
|
| ydecErr |
StackObjectThin |
PS1DR2 |
Declination error from y filter stack detection. |
real |
4 |
arcsec |
-999 |
|
| yEll |
allSkyNIRSource |
VULCANiDR |
1-b/a, where a/b=semi-major/minor axes in Y |
real |
4 |
|
-0.9999995e9 |
src.ellipticity&MagUCD& |
| yeNum |
allSkyNIRFrameSetInfo |
VULCANiDR |
the extension number of this Y frame |
tinyint |
1 |
|
|
meta.number;em.IR.K |
| yEpoch |
StackObjectThin |
PS1DR2 |
Modified Julian Date of the mean epoch of images contributing to the the y-band stack (equinox J2000). |
float |
8 |
days |
-999 |
|
| yErrBits |
allSkyNIRSource |
VULCANiDR |
processing warning/error bitwise flags in Y |
int |
4 |
|
-99999999 |
meta.code&MagUCD& |
| Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
| yEta |
allSkyNIRSource |
VULCANiDR |
Offset of Y detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff&MagUCD& |
| When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 2.0 (UKIDSS LAS and GPS; UHS; also non-survey programmes) or 1.0 (UKIDSS GPS, DXS and UDS) arcseconds is used, the higher value enabling pairing of moving sources when epoch separations may be several years. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the LAS, you might wish to insist that the offsets in the selected sample are all below 1 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
| yexpTime |
StackObjectAttributes |
PS1DR2 |
Exposure time of the y filter stack. Necessary for converting listed fluxes and magnitudes back to measured ADU counts. |
real |
4 |
seconds |
-999 |
|
| yExtNSigma |
StackObjectAttributes |
PS1DR2 |
An extendedness measure for the y filter stack detection based on the deviation between PSF and Kron (1980) magnitudes, normalized by the PSF magnitude uncertainty. |
real |
4 |
|
-999 |
|
| yFlags |
MeanObject |
PS1DR2 |
Information flag bitmask for mean object from y filter detections. Values listed in ObjectFilterFlags. |
int |
4 |
|
0 |
|
| yGausig |
allSkyNIRSource |
VULCANiDR |
RMS of axes of ellipse fit in Y |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param&MagUCD& |
| yHlCorSMjRadAs |
allSkyNIRSource |
VULCANiDR |
Seeing corrected half-light, semi-major axis in Y band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize;em.opt.I |
| yinfoFlag |
StackObjectThin |
PS1DR2 |
Information flag bitmask indicating details of the y filter stack photometry. Values listed in DetectionFlags. |
bigint |
8 |
|
0 |
|
| yinfoFlag2 |
StackObjectThin |
PS1DR2 |
Information flag bitmask indicating details of the y filter stack photometry. Values listed in DetectionFlags2. |
int |
4 |
|
0 |
|
| yinfoFlag3 |
StackObjectThin |
PS1DR2 |
Information flag bitmask indicating details of the y filter stack photometry. Values listed in DetectionFlags3. |
int |
4 |
|
0 |
|
| yippDetectID |
StackObjectAttributes, StackObjectThin |
PS1DR2 |
IPP internal detection identifier. |
bigint |
8 |
|
|
|
| yKronFlux |
StackObjectAttributes |
PS1DR2 |
Kron (1980) flux from y filter stack detection. |
real |
4 |
Janskys |
-999 |
|
| yKronFluxErr |
StackObjectAttributes |
PS1DR2 |
Error in Kron (1980) flux from y filter stack detection. |
real |
4 |
Janskys |
-999 |
|
| yKronMag |
StackObjectThin |
PS1DR2 |
Kron (1980) magnitude from y filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
| yKronMagErr |
StackObjectThin |
PS1DR2 |
Error in Kron (1980) magnitude from y filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
| yKronRad |
StackObjectAttributes |
PS1DR2 |
Kron (1980) radius from y filter stack detection. |
real |
4 |
arcsec |
-999 |
|
| yMeanApMag |
MeanObject |
PS1DR2 |
Mean aperture magnitude from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| yMeanApMagErr |
MeanObject |
PS1DR2 |
Error in mean aperture magnitude from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| yMeanApMagNpt |
MeanObject |
PS1DR2 |
Number of measurements included in mean aperture magnitude from y filter detections. |
smallint |
2 |
|
-999 |
|
| yMeanApMagStd |
MeanObject |
PS1DR2 |
Standard deviation of aperture magnitudes from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| yMeanKronMag |
MeanObject |
PS1DR2 |
Mean Kron (1980) magnitude from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| yMeanKronMagErr |
MeanObject |
PS1DR2 |
Error in mean Kron (1980) magnitude from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| yMeanKronMagNpt |
MeanObject |
PS1DR2 |
Number of measurements included in mean Kron (1980) magnitude from y filter detections. |
smallint |
2 |
|
-999 |
|
| yMeanKronMagStd |
MeanObject |
PS1DR2 |
Standard deviation of Kron (1980) magnitudes from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| yMeanPSFMag |
MeanObject |
PS1DR2 |
Mean PSF magnitude from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| yMeanPSFMagErr |
MeanObject |
PS1DR2 |
Error in mean PSF magnitude from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| yMeanPSFMagMax |
MeanObject |
PS1DR2 |
Maximum PSF magnitude from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| yMeanPSFMagMin |
MeanObject |
PS1DR2 |
Minimum PSF magnitude from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| yMeanPSFMagNpt |
MeanObject |
PS1DR2 |
Number of measurements included in mean PSF magnitude from y filter detections. |
smallint |
2 |
|
-999 |
|
| yMeanPSFMagStd |
MeanObject |
PS1DR2 |
Standard deviation of PSF magnitudes from y filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
| ymfID |
allSkyNIRFrameSetInfo |
VULCANiDR |
the UID of the relevant Y multiframe |
bigint |
8 |
|
|
meta.id;obs.field;em.IR.K |
| ymjAllExt |
allSkyNIRSource |
VULCANiDR |
Extended source colour Y-J (using aperMagNoAperCorr3) for All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.color&ColorUCD& |
| Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
| ymjAllExtErr |
allSkyNIRSource |
VULCANiDR |
Error on extended source colour Y-J for All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error&ColorUCD& |
| Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
| ymjAllPnt |
allSkyNIRSource |
VULCANiDR |
Point source colour Y-J (using aperMag3) for All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.color&ColorUCD& |
| Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
| ymjAllPntErr |
allSkyNIRSource |
VULCANiDR |
Error on point source colour Y-J for All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error&ColorUCD& |
| Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
| yMjd |
allSkyNIRSource |
VULCANiDR |
Modified Julian Day in Y band |
float |
8 |
days |
-0.9999995e9 |
time.epoch&MagUCD& |
| ymjTelExt |
allSkyNIRSource |
VULCANiDR |
Extended source colour Y-J (using aperMagNoAperCorr3) for original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.color&ColorUCD& |
| Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
| ymjTelExtErr |
allSkyNIRSource |
VULCANiDR |
Error on extended source colour Y-J for original calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error&ColorUCD& |
| Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
| ymjTelPnt |
allSkyNIRSource |
VULCANiDR |
Point source colour Y-J (using aperMag3) for original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.color&ColorUCD& |
| Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
| ymjTelPntErr |
allSkyNIRSource |
VULCANiDR |
Error on point source colour Y-J for original calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error&ColorUCD& |
| Default colours from pairs of adjacent passbands within a given set (e.g. Y-J, J-H and H-K for YJHK) are recorded in the merged source table for ease of querying and speedy querying via indexing of these attributes. Presently, the point-source colours and extended source colours are computed from the aperture corrected AperMag3 fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands) and generally good signal-to-noise. At some point in the future, this may be changed such that point-source colours will be computed from the PSF-fitted measures and extended source colours computed from the 2-d Sersic model profile fits. |
| ymomentR1 |
StackObjectAttributes |
PS1DR2 |
First radial moment for y filter stack detection. |
real |
4 |
arcsec |
-999 |
|
| ymomentRH |
StackObjectAttributes |
PS1DR2 |
Half radial moment (r^0.5 weighting) for y filter stack detection. |
real |
4 |
arcsec^0.5 |
-999 |
|
| ymomentXX |
StackObjectAttributes |
PS1DR2 |
Second moment M_xx for y filter stack detection. |
real |
4 |
arcsec^2 |
-999 |
|
| ymomentXY |
StackObjectAttributes |
PS1DR2 |
Second moment M_xy for y filter stack detection. |
real |
4 |
arcsec^2 |
-999 |
|
| ymomentYY |
StackObjectAttributes |
PS1DR2 |
Second moment M_yy for y filter stack detection. |
real |
4 |
arcsec^2 |
-999 |
|
| yNEpochs |
allSkyNIRFrameSetInfo |
VULCANiDR |
Number of epochs in Y band (0 if no measurements) |
int |
4 |
|
|
|
| ynFrames |
StackObjectThin |
PS1DR2 |
Number of input frames/exposures contributing to the y filter stack detection. |
int |
4 |
|
-999 |
|
| yObs |
allSkyNIRSource |
VULCANiDR |
There are pixels at this position in the Y-band |
tinyint |
1 |
|
0 |
meta.flag |
| yPA |
allSkyNIRSource |
VULCANiDR |
ellipse fit celestial orientation in Y |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng&MagUCD& |
| yPixSize |
CurrentAstrometry |
VULCANiDR |
Angular size of pixels in Y |
real |
4 |
Arcseconds |
-0.9999995e9 |
pos.angDistance |
| yPlateScale |
StackObjectAttributes |
PS1DR2 |
Local plate scale for the y filter stack. |
real |
4 |
arcsec/pixel |
0 |
|
| yPos |
Detection |
PS1DR2 |
PSF y center location. |
real |
4 |
raw pixels |
-999 |
|
| yPosErr |
Detection |
PS1DR2 |
Error in PSF y center location. |
real |
4 |
raw pixels |
-999 |
|
| yppErrBits |
allSkyNIRSource |
VULCANiDR |
additional WFAU post-processing error bits in Y |
int |
4 |
|
0 |
meta.code&MagUCD& |
Post-processing error quality bit flags assigned (NB: from UKIDSS DR2 release onwards) in the WSA curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: | Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | | 1 | 15 | Source in poor flat field region | 32768 | 0x00008000 | All but mosaics | | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues (though deeps excluded prior to DR8) | | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | GPS only | | 2 | 19 | Possible crosstalk artefact/contamination | 524288 | 0x00080000 | All but GPS | | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All but mosaics | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all K band sources in the LAS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
| ypsfChiSq |
StackObjectAttributes |
PS1DR2 |
Reduced chi squared value of the PSF model fit for y filter stack detection. |
real |
4 |
|
-999 |
|
| ypsfCore |
StackObjectAttributes |
PS1DR2 |
PSF core parameter k from y filter stack detection, where F = F0 / (1 + k r^2 + r^3.33). |
real |
4 |
|
-999 |
|
| yPSFFlux |
StackObjectAttributes |
PS1DR2 |
PSF flux from y filter stack detection. |
real |
4 |
Janskys |
-999 |
|
| yPSFFluxErr |
StackObjectAttributes |
PS1DR2 |
Error in PSF flux from y filter stack detection. |
real |
4 |
Janskys |
-999 |
|
| ypsfLikelihood |
StackObjectAttributes |
PS1DR2 |
Likelihood that this y filter stack detection is best fit by a PSF. |
real |
4 |
|
-999 |
|
| yPSFMag |
StackObjectThin |
PS1DR2 |
PSF magnitude from y filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
| yPSFMagErr |
StackObjectThin |
PS1DR2 |
Error in PSF magnitude from y filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
| ypsfMajorFWHM |
StackObjectAttributes |
PS1DR2 |
PSF major axis FWHM from y filter stack detection. |
real |
4 |
arcsec |
-999 |
|
| ypsfMinorFWHM |
StackObjectAttributes |
PS1DR2 |
PSF minor axis FWHM from y filter stack detection. |
real |
4 |
arcsec |
-999 |
|
| ypsfQf |
StackObjectAttributes |
PS1DR2 |
PSF coverage factor for y filter stack detection. |
real |
4 |
|
-999 |
|
| ypsfQfPerfect |
StackObjectAttributes |
PS1DR2 |
PSF-weighted fraction of pixels totally unmasked for y filter stack detection. |
real |
4 |
|
-999 |
|
| ypsfTheta |
StackObjectAttributes |
PS1DR2 |
PSF major axis orientation from y filter stack detection. |
real |
4 |
degrees |
-999 |
|
| yQfPerfect |
MeanObject |
PS1DR2 |
Maximum PSF weighted fraction of pixels totally unmasked from y filter detections. |
real |
4 |
|
-999 |
|
| yra |
StackObjectThin |
PS1DR2 |
Right ascension from y filter stack detection. |
float |
8 |
degrees |
-999 |
|
| yraErr |
StackObjectThin |
PS1DR2 |
Right ascension error from y filter stack detection. |
real |
4 |
arcsec |
-999 |
|
| ySeeing |
allSkyNIRFrameSetInfo |
VULCANiDR |
Y band seeing |
float |
8 |
arcsec |
|
|
| ySeqNum |
allSkyNIRSource |
VULCANiDR |
the running number of the Y detection |
int |
4 |
|
-99999999 |
meta.number&MagUCD& |
| ysky |
StackObjectAttributes |
PS1DR2 |
Residual background sky level at the y filter stack detection. |
real |
4 |
Janskys/arcsec^2 |
-999 |
|
| yskyErr |
StackObjectAttributes |
PS1DR2 |
Error in residual background sky level at the y filter stack detection. |
real |
4 |
Janskys/arcsec^2 |
-999 |
|
| ystackDetectID |
StackObjectAttributes, StackObjectThin |
PS1DR2 |
Unique stack detection identifier. |
bigint |
8 |
|
|
|
| ystackImageID |
StackObjectAttributes, StackObjectThin |
PS1DR2 |
Unique stack identifier for y filter detection. |
bigint |
8 |
|
|
|
| yTelAperMag3 |
allSkyNIRSource |
VULCANiDR |
Default point source Y aperture corrected mag (2.0 arcsec aperture diameter) using original calibration If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yTelAperMag3Err |
allSkyNIRSource |
VULCANiDR |
Error in default point/extended source Y mag (2.0 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| yTelAperMag4 |
allSkyNIRSource |
VULCANiDR |
Point source Y aperture corrected mag (2.8 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yTelAperMag4Err |
allSkyNIRSource |
VULCANiDR |
Error in point/extended source Y mag (2.8 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| yTelAperMag6 |
allSkyNIRSource |
VULCANiDR |
Point source Y aperture corrected mag (5.7 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yTelAperMag6Err |
allSkyNIRSource |
VULCANiDR |
Error in point/extended source Y mag (5.7 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| yTelAperMagNoAperCorr3 |
allSkyNIRSource |
VULCANiDR |
Default extended source Y aperture mag (2.0 arcsec aperture diameter) using original calibration If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yTelAperMagNoAperCorr4 |
allSkyNIRSource |
VULCANiDR |
Extended source Y aperture mag (2.8 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yTelAperMagNoAperCorr6 |
allSkyNIRSource |
VULCANiDR |
Extended source Y aperture mag (5.7 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yTelPetroMag |
allSkyNIRSource |
VULCANiDR |
Extended source Y mag (Petrosian) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| yTelPetroMagErr |
allSkyNIRSource |
VULCANiDR |
Error in extended source Y mag (Petrosian) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| yXi |
allSkyNIRSource |
VULCANiDR |
Offset of Y detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff&MagUCD& |
| When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 2.0 (UKIDSS LAS and GPS; UHS; also non-survey programmes) or 1.0 (UKIDSS GPS, DXS and UDS) arcseconds is used, the higher value enabling pairing of moving sources when epoch separations may be several years. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the LAS, you might wish to insist that the offsets in the selected sample are all below 1 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
| yxPos |
StackObjectAttributes |
PS1DR2 |
PSF x center location from y filter stack detection. |
real |
4 |
sky pixels |
-999 |
|
| yxPosErr |
StackObjectAttributes |
PS1DR2 |
Error in PSF x center location from y filter stack detection. |
real |
4 |
sky pixels |
-999 |
|
| yyPos |
StackObjectAttributes |
PS1DR2 |
PSF y center location from y filter stack detection. |
real |
4 |
sky pixels |
-999 |
|
| yyPosErr |
StackObjectAttributes |
PS1DR2 |
Error in PSF y center location from y filter stack detection. |
real |
4 |
sky pixels |
-999 |
|
| yzp |
StackObjectAttributes |
PS1DR2 |
Photometric zeropoint for the y filter stack. Necessary for converting listed fluxes and magnitudes back to measured ADU counts. |
real |
4 |
magnitudes |
0 |
|