K |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
k_1AperMag1 |
gpsJHKsource, gpsPointSource, reliableGpsPointSource |
WSA |
Extended source 1st epoch K aperture corrected mag (0.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1AperMag1 |
gpsSource |
WSA |
Extended source 1st epoch K aperture corrected mag (0.7 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1AperMag1Err |
gpsJHKsource, gpsPointSource, gpsSource, reliableGpsPointSource |
WSA |
Error in extended source 1st epoch K mag (1.4 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_1AperMag3 |
gcsPointSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Default point/extended source 1st epoch K aperture corrected mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1AperMag3 |
gcsSource, gpsSource |
WSA |
Default point/extended source 1st epoch K aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1AperMag3Err |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Error in default point/extended source 1st epoch K mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_1AperMag4 |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Extended source 1st epoch K aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1AperMag4Err |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Error in extended source 1st epoch K mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_1AperMag6 |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Extended source 1st epoch K aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1AperMag6Err |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Error in extended source 1st epoch K mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_1Class |
gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
discrete image classification flag in 1st epoch K |
smallint |
2 |
|
-9999 |
CLASS_MISC |
k_1ClassStat |
gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsSourceRemeasurement, reliableGcsPointSource |
WSA |
N(0,1) stellarness-of-profile statistic in 1st epoch K |
real |
4 |
|
-0.9999995e9 |
STAT_PROP |
k_1ClassStat |
gpsJHKsource, gpsPointSource, gpsSource, reliableGpsPointSource |
WSA |
S-Extractor classification statistic in 1st epoch K |
real |
4 |
|
-0.9999995e9 |
STAT_PROP |
k_1Deblend |
gcsPointSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
placeholder flag indicating parent/child relation in 1st epoch K |
int |
4 |
|
-99999999 |
CODE_MISC |
k_1Deblend |
gcsSource |
WSA |
placeholder flag indicating parent/child relation in 1st epoch K |
int |
4 |
|
-99999999 |
CODE_MISC |
This CASU pipeline processing source extraction flag is a placeholder only, and is always set to zero in all passbands in the merged source lists. If you need to know when a particular image detection is a component of a deblend or not, test bit 4 of attribute ppErrBits (see corresponding glossary entry) which is set by WFAU's post-processing software based on testing the areal profiles aprof2-8 (these are set by CASU to -1 for deblended components, or positive values for non-deblended detections). We encode this in an information bit of ppErrBits for convenience when querying the merged source tables. |
k_1Ell |
gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
1-b/a, where a/b=semi-major/minor axes in 1st epoch K |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
k_1eNum |
gcsMergeLog, gcsZYJHKmergeLog, gpsJHKmergeLog, gpsMergeLog |
WSA |
the extension number of this 1st epoch K frame |
tinyint |
1 |
|
|
NUMBER |
k_1ErrBits |
gcsPointSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
processing warning/error bitwise flags in 1st epoch K |
int |
4 |
|
-99999999 |
CODE_MISC |
k_1ErrBits |
gcsSource |
WSA |
processing warning/error bitwise flags in 1st epoch K |
int |
4 |
|
-99999999 |
CODE_MISC |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
k_1ErrBits |
gpsSource |
WSA |
processing warning/error bitwise flags in 1st epoch K |
int |
4 |
|
-99999999 |
CODE_MISC |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
k_1Eta |
gcsPointSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Offset of 1st epoch K detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_DEC_OFF |
k_1Eta |
gcsSource, gpsSource |
WSA |
Offset of 1st epoch K detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_DEC_OFF |
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; 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. |
k_1Gausig |
gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
RMS of axes of ellipse fit in 1st epoch K |
real |
4 |
pixels |
-0.9999995e9 |
MORPH_PARAM |
k_1HallMag |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Total point source 1st epoch K mag |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1HallMagErr |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Error in total point source 1st epoch K mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_1Mag |
gcsSourceRemeasurement, gpsSourceRemeasurement |
WSA |
1st epoch K mag (as appropriate for this merged source) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1MagErr |
gcsSourceRemeasurement, gpsSourceRemeasurement |
WSA |
Error in 1st epoch K mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_1mfID |
gcsMergeLog, gcsZYJHKmergeLog, gpsJHKmergeLog, gpsMergeLog |
WSA |
the UID of the relevant 1st epoch K multiframe |
bigint |
8 |
|
|
ID_FRAME |
k_1ObjID |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
the UID of the 1st epoch K detection |
bigint |
8 |
|
-99999999 |
ID_NUMBER |
k_1ObjID |
gcsSourceRemeasurement, gpsSourceRemeasurement |
WSA |
the UID of the 1st epoch K remeasurement |
bigint |
8 |
|
-99999999 |
ID_NUMBER |
k_1PA |
gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
ellipse fit celestial orientation in 1st epoch K |
real |
4 |
Degrees |
-0.9999995e9 |
POS_POS-ANG |
k_1PetroMag |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Extended source 1st epoch K mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1PetroMagErr |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Error in extended source 1st epoch K mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_1ppErrBits |
gcsPointSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
additional WFAU post-processing error bits in 1st epoch K |
int |
4 |
|
0 |
CODE_MISC |
k_1ppErrBits |
gcsSource |
WSA |
additional WFAU post-processing error bits in 1st epoch K |
int |
4 |
|
0 |
CODE_MISC |
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 | LAS, GCS, GPS, DXS | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | LAS, GCS, GPS, DXS | 2 | 16 | Close to saturated | 65536 | 0x00010000 | LAS, GCS, GPS | 2 | 19 | Possible crosstalk artefact/contamination | 524288 | 0x00080000 | LAS, GCS, DXS | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | LAS, GCS, GPS, DXS | 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. |
k_1PsfMag |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Point source profile-fitted 1st epoch K mag |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1PsfMagErr |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Error in point source profile-fitted 1st epoch K mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_1SeqNum |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
the running number of the 1st epoch K detection |
int |
4 |
|
-99999999 |
ID_NUMBER |
k_1SeqNum |
gcsSourceRemeasurement, gpsSourceRemeasurement |
WSA |
the running number of the 1st epoch K remeasurement |
int |
4 |
|
-99999999 |
ID_NUMBER |
k_1SerMag2D |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Extended source 1st epoch K mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_1SerMag2DErr |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Error in extended source 1st epoch K mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_1Xi |
gcsPointSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Offset of 1st epoch K detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_RA_OFF |
k_1Xi |
gcsSource, gpsSource |
WSA |
Offset of 1st epoch K detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_RA_OFF |
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; 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. |
k_2AperMag1 |
gpsJHKsource, gpsPointSource, reliableGpsPointSource |
WSA |
Extended source 2nd epoch K aperture corrected mag (0.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2AperMag1 |
gpsSource |
WSA |
Extended source 2nd epoch K aperture corrected mag (0.7 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2AperMag1Err |
gpsJHKsource, gpsPointSource, gpsSource, reliableGpsPointSource |
WSA |
Error in extended source 2nd epoch K mag (1.4 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_2AperMag3 |
gcsPointSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Default point/extended source 2nd epoch K aperture corrected mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2AperMag3 |
gcsSource, gpsSource |
WSA |
Default point/extended source 2nd epoch K aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2AperMag3Err |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Error in default point/extended source 2nd epoch K mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_2AperMag4 |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Extended source 2nd epoch K aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2AperMag4Err |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Error in extended source 2nd epoch K mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_2AperMag6 |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Extended source 2nd epoch K aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2AperMag6Err |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Error in extended source 2nd epoch K mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_2Class |
gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
discrete image classification flag in 2nd epoch K |
smallint |
2 |
|
-9999 |
CLASS_MISC |
k_2ClassStat |
gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsSourceRemeasurement, reliableGcsPointSource |
WSA |
N(0,1) stellarness-of-profile statistic in 2nd epoch K |
real |
4 |
|
-0.9999995e9 |
STAT_PROP |
k_2ClassStat |
gpsJHKsource, gpsPointSource, gpsSource, reliableGpsPointSource |
WSA |
S-Extractor classification statistic in 2nd epoch K |
real |
4 |
|
-0.9999995e9 |
STAT_PROP |
k_2Deblend |
gcsPointSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
placeholder flag indicating parent/child relation in 2nd epoch K |
int |
4 |
|
-99999999 |
CODE_MISC |
k_2Deblend |
gcsSource |
WSA |
placeholder flag indicating parent/child relation in 2nd epoch K |
int |
4 |
|
-99999999 |
CODE_MISC |
This CASU pipeline processing source extraction flag is a placeholder only, and is always set to zero in all passbands in the merged source lists. If you need to know when a particular image detection is a component of a deblend or not, test bit 4 of attribute ppErrBits (see corresponding glossary entry) which is set by WFAU's post-processing software based on testing the areal profiles aprof2-8 (these are set by CASU to -1 for deblended components, or positive values for non-deblended detections). We encode this in an information bit of ppErrBits for convenience when querying the merged source tables. |
k_2Ell |
gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
1-b/a, where a/b=semi-major/minor axes in 2nd epoch K |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
k_2eNum |
gcsMergeLog, gcsZYJHKmergeLog, gpsJHKmergeLog, gpsMergeLog |
WSA |
the extension number of this 2nd epoch K frame |
tinyint |
1 |
|
|
NUMBER |
k_2ErrBits |
gcsPointSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
processing warning/error bitwise flags in 2nd epoch K |
int |
4 |
|
-99999999 |
CODE_MISC |
k_2ErrBits |
gcsSource |
WSA |
processing warning/error bitwise flags in 2nd epoch K |
int |
4 |
|
-99999999 |
CODE_MISC |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
k_2ErrBits |
gpsSource |
WSA |
processing warning/error bitwise flags in 2nd epoch K |
int |
4 |
|
-99999999 |
CODE_MISC |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
k_2Eta |
gcsPointSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Offset of 2nd epoch K detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_DEC_OFF |
k_2Eta |
gcsSource, gpsSource |
WSA |
Offset of 2nd epoch K detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_DEC_OFF |
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; 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. |
k_2Gausig |
gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
RMS of axes of ellipse fit in 2nd epoch K |
real |
4 |
pixels |
-0.9999995e9 |
MORPH_PARAM |
k_2HallMag |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Total point source 2nd epoch K mag |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2HallMagErr |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Error in total point source 2nd epoch K mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_2Mag |
gcsSourceRemeasurement, gpsSourceRemeasurement |
WSA |
2nd epoch K mag (as appropriate for this merged source) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2MagErr |
gcsSourceRemeasurement, gpsSourceRemeasurement |
WSA |
Error in 2nd epoch K mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_2mfID |
gcsMergeLog, gcsZYJHKmergeLog, gpsJHKmergeLog, gpsMergeLog |
WSA |
the UID of the relevant 2nd epoch K multiframe |
bigint |
8 |
|
|
ID_FRAME |
k_2mrat |
twomass_scn |
2MASS |
Ks-band average 2nd image moment ratio. |
real |
4 |
|
|
FIT_PARAM_VALUE |
k_2ObjID |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
the UID of the 2nd epoch K detection |
bigint |
8 |
|
-99999999 |
ID_NUMBER |
k_2ObjID |
gcsSourceRemeasurement, gpsSourceRemeasurement |
WSA |
the UID of the 2nd epoch K remeasurement |
bigint |
8 |
|
-99999999 |
ID_NUMBER |
k_2PA |
gcsPointSource, gcsSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
ellipse fit celestial orientation in 2nd epoch K |
real |
4 |
Degrees |
-0.9999995e9 |
POS_POS-ANG |
k_2PetroMag |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Extended source 2nd epoch K mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2PetroMagErr |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Error in extended source 2nd epoch K mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_2ppErrBits |
gcsPointSource, gcsSourceRemeasurement, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, gpsSourceRemeasurement, reliableGcsPointSource, reliableGpsPointSource |
WSA |
additional WFAU post-processing error bits in 2nd epoch K |
int |
4 |
|
0 |
CODE_MISC |
k_2ppErrBits |
gcsSource |
WSA |
additional WFAU post-processing error bits in 2nd epoch K |
int |
4 |
|
0 |
CODE_MISC |
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 | LAS, GCS, GPS, DXS | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | LAS, GCS, GPS, DXS | 2 | 16 | Close to saturated | 65536 | 0x00010000 | LAS, GCS, GPS | 2 | 19 | Possible crosstalk artefact/contamination | 524288 | 0x00080000 | LAS, GCS, DXS | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | LAS, GCS, GPS, DXS | 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. |
k_2PsfMag |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Point source profile-fitted 2nd epoch K mag |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2PsfMagErr |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Error in point source profile-fitted 2nd epoch K mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_2SeqNum |
gcsPointSource, gcsSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, gpsSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
the running number of the 2nd epoch K detection |
int |
4 |
|
-99999999 |
ID_NUMBER |
k_2SeqNum |
gcsSourceRemeasurement, gpsSourceRemeasurement |
WSA |
the running number of the 2nd epoch K remeasurement |
int |
4 |
|
-99999999 |
ID_NUMBER |
k_2SerMag2D |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Extended source 2nd epoch K mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
k_2SerMag2DErr |
gcsPointSource, gcsSource, gcsZYJHKsource, reliableGcsPointSource |
WSA |
Error in extended source 2nd epoch K mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
k_2Xi |
gcsPointSource, gcsZYJHKsource, gpsJHKsource, gpsPointSource, reliableGcsPointSource, reliableGpsPointSource |
WSA |
Offset of 2nd epoch K detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_RA_OFF |
k_2Xi |
gcsSource, gpsSource |
WSA |
Offset of 2nd epoch K detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_RA_OFF |
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; 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. |
k_5sig_ba |
twomass_xsc |
2MASS |
K minor/major axis ratio fit to the 5-sigma isophote. |
real |
4 |
|
|
PHYS_AXIS-RATIO |
k_5sig_phi |
twomass_xsc |
2MASS |
K angle to 5-sigma major axis (E of N). |
smallint |
2 |
degrees |
|
ERROR |
k_5surf |
twomass_xsc |
2MASS |
K central surface brightness (r<=5). |
real |
4 |
mag |
|
PHOT_SB_GENERAL |
k_ba |
twomass_xsc |
2MASS |
K minor/major axis ratio fit to the 3-sigma isophote. |
real |
4 |
|
|
PHYS_AXIS-RATIO |
k_back |
twomass_xsc |
2MASS |
K coadd median background. |
real |
4 |
|
|
CODE_MISC |
k_bisym_chi |
twomass_xsc |
2MASS |
K bi-symmetric cross-correlation chi. |
real |
4 |
|
|
FIT_PARAM_VALUE |
k_bisym_rat |
twomass_xsc |
2MASS |
K bi-symmetric flux ratio. |
real |
4 |
|
|
PHOT_FLUX_RATIO |
k_bndg_amp |
twomass_xsc |
2MASS |
K banding maximum FT amplitude on this side of coadd. |
real |
4 |
DN |
|
FIT_PARAM_VALUE |
k_bndg_per |
twomass_xsc |
2MASS |
K banding Fourier Transf. period on this side of coadd. |
int |
4 |
arcsec |
|
FIT_PARAM_VALUE |
k_chif_ellf |
twomass_xsc |
2MASS |
K % chi-fraction for elliptical fit to 3-sig isophote. |
real |
4 |
|
|
FIT_PARAM_VALUE |
k_cmsig |
twomass_psc |
2MASS |
Corrected photometric uncertainty for the default Ks-band magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_con_indx |
twomass_xsc |
2MASS |
K concentration index r_75%/r_25%. |
real |
4 |
|
|
PHYS_CONCENT_INDEX |
k_d_area |
twomass_xsc |
2MASS |
K 5-sigma to 3-sigma differential area. |
smallint |
2 |
|
|
FIT_RESIDUAL |
k_flg_10 |
twomass_xsc |
2MASS |
K confusion flag for 10 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_15 |
twomass_xsc |
2MASS |
K confusion flag for 15 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_20 |
twomass_xsc |
2MASS |
K confusion flag for 20 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_25 |
twomass_xsc |
2MASS |
K confusion flag for 25 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_30 |
twomass_xsc |
2MASS |
K confusion flag for 30 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_40 |
twomass_xsc |
2MASS |
K confusion flag for 40 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_5 |
twomass_xsc |
2MASS |
K confusion flag for 5 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_50 |
twomass_xsc |
2MASS |
K confusion flag for 50 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_60 |
twomass_xsc |
2MASS |
K confusion flag for 60 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_7 |
twomass_xsc |
2MASS |
K confusion flag for 7 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_70 |
twomass_xsc |
2MASS |
K confusion flag for 70 arcsec circular ap. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_c |
twomass_xsc |
2MASS |
K confusion flag for Kron circular mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_e |
twomass_xsc |
2MASS |
K confusion flag for Kron elliptical mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_fc |
twomass_xsc |
2MASS |
K confusion flag for fiducial Kron circ. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_fe |
twomass_xsc |
2MASS |
K confusion flag for fiducial Kron ell. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_i20c |
twomass_xsc |
2MASS |
K confusion flag for 20mag/sq." iso. circ. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_i20e |
twomass_xsc |
2MASS |
K confusion flag for 20mag/sq." iso. ell. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_i21c |
twomass_xsc |
2MASS |
K confusion flag for 21mag/sq." iso. circ. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_i21e |
twomass_xsc |
2MASS |
K confusion flag for 21mag/sq." iso. ell. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_j21fc |
twomass_xsc |
2MASS |
K confusion flag for 21mag/sq." iso. fid. circ. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_j21fe |
twomass_xsc |
2MASS |
K confusion flag for 21mag/sq." iso. fid. ell. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_k20fc |
twomass_xsc |
2MASS |
K confusion flag for 20mag/sq." iso. fid. circ. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_flg_k20fe |
twomass_xsc |
2MASS |
K confusion flag for 20mag/sq." iso. fid. ell. mag. |
smallint |
2 |
|
|
CODE_MISC |
k_m |
twomass_psc |
2MASS |
Default Ks-band magnitude |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_10 |
twomass_xsc |
2MASS |
K 10 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_15 |
twomass_xsc |
2MASS |
K 15 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_20 |
twomass_xsc |
2MASS |
K 20 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_25 |
twomass_xsc |
2MASS |
K 25 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_30 |
twomass_xsc |
2MASS |
K 30 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_40 |
twomass_xsc |
2MASS |
K 40 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_5 |
twomass_xsc |
2MASS |
K 5 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_50 |
twomass_xsc |
2MASS |
K 50 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_60 |
twomass_xsc |
2MASS |
K 60 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_7 |
twomass_xsc |
2MASS |
K 7 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_70 |
twomass_xsc |
2MASS |
K 70 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_c |
twomass_xsc |
2MASS |
K Kron circular aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_e |
twomass_xsc |
2MASS |
K Kron elliptical aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_ext |
twomass_xsc |
2MASS |
K mag from fit extrapolation. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_fc |
twomass_xsc |
2MASS |
K fiducial Kron circular magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_fe |
twomass_xsc |
2MASS |
K fiducial Kron ell. mag aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_i20c |
twomass_xsc |
2MASS |
K 20mag/sq." isophotal circular ap. magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_i20e |
twomass_xsc |
2MASS |
K 20mag/sq." isophotal elliptical ap. magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_i21c |
twomass_xsc |
2MASS |
K 21mag/sq." isophotal circular ap. magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_i21e |
twomass_xsc |
2MASS |
K 21mag/sq." isophotal elliptical ap. magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_j21fc |
twomass_xsc |
2MASS |
K 21mag/sq." isophotal fiducial circ. ap. mag. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_j21fe |
twomass_xsc |
2MASS |
K 21mag/sq." isophotal fiducial ell. ap. magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_k20fc |
twomass_xsc |
2MASS |
K 20mag/sq." isophotal fiducial circ. ap. mag. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_k20fe |
twomass_xsc |
2MASS |
K 20mag/sq." isophotal fiducial ell. ap. magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_stdap |
twomass_psc |
2MASS |
Ks-band "standard" aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_m_sys |
twomass_xsc |
2MASS |
K system photometry magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_mnsurfb_eff |
twomass_xsc |
2MASS |
K mean surface brightness at the half-light radius. |
real |
4 |
mag |
|
PHOT_SB_GENERAL |
k_msig_10 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 10 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_15 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 15 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_20 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 20 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_25 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 25 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_30 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 30 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_40 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 40 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_5 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 5 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_50 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 50 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_60 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 60 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_7 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 7 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_70 |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 70 arcsec circular ap. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_c |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in Kron circular mag. |
real |
4 |
mag |
|
ERROR |
k_msig_e |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in Kron elliptical mag. |
real |
4 |
mag |
|
ERROR |
k_msig_ext |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in mag from fit extrapolation. |
real |
4 |
mag |
|
ERROR |
k_msig_fc |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in fiducial Kron circ. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_fe |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in fiducial Kron ell. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_i20c |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 20mag/sq." iso. circ. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_i20e |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 20mag/sq." iso. ell. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_i21c |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 21mag/sq." iso. circ. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_i21e |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 21mag/sq." iso. ell. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_j21fc |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 21mag/sq." iso.fid.circ.mag. |
real |
4 |
mag |
|
ERROR |
k_msig_j21fe |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 21mag/sq." iso.fid.ell.mag. |
real |
4 |
mag |
|
ERROR |
k_msig_k20fc |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 20mag/sq." iso.fid.circ. mag. |
real |
4 |
mag |
|
ERROR |
k_msig_k20fe |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in 20mag/sq." iso.fid.ell.mag. |
real |
4 |
mag |
|
ERROR |
k_msig_stdap |
twomass_psc |
2MASS |
Uncertainty in the Ks-band standard aperture magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_msig_sys |
twomass_xsc |
2MASS |
K 1-sigma uncertainty in system photometry mag. |
real |
4 |
mag |
|
ERROR |
k_msigcom |
twomass_psc |
2MASS |
Combined, or total photometric uncertainty for the default Ks-band magnitude. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_msnr10 |
twomass_scn |
2MASS |
The estimated Ks-band magnitude at which SNR=10 is achieved for this scan. |
real |
4 |
mag |
|
SPECT_FLUX_VALUE |
k_n_snr10 |
twomass_scn |
2MASS |
Number of point sources at Ks-band with SNR>10 (instrumental mag <=14.3) |
int |
4 |
|
|
NUMBER |
k_pchi |
twomass_xsc |
2MASS |
K chi^2 of fit to rad. profile (LCSB: alpha scale len). |
real |
4 |
|
|
FIT_PARAM_VALUE |
k_peak |
twomass_xsc |
2MASS |
K peak pixel brightness. |
real |
4 |
mag |
|
PHOT_SB_GENERAL |
k_perc_darea |
twomass_xsc |
2MASS |
K 5-sigma to 3-sigma percent area change. |
smallint |
2 |
|
|
FIT_PARAM |
k_phi |
twomass_xsc |
2MASS |
K angle to 3-sigma major axis (E of N). |
smallint |
2 |
degrees |
|
POS_POS-ANG |
k_psfchi |
twomass_psc |
2MASS |
Reduced chi-squared goodness-of-fit value for the Ks-band profile-fit photometry made on the 1.3 s "Read_2" exposures. |
real |
4 |
|
|
FIT_PARAM_VALUE |
k_psp |
twomass_scn |
2MASS |
Ks-band photometric sensitivity paramater (PSP). |
real |
4 |
|
|
INST_SENSITIVITY |
k_pts_noise |
twomass_scn |
2MASS |
Base-10 logarithm of the mode of the noise distribution for all point source detections in the scan, where the noise is estimated from the measured Ks-band photometric errors and is expressed in units of mJy. |
real |
4 |
|
|
INST_NOISE |
k_r_c |
twomass_xsc |
2MASS |
K Kron circular aperture radius. |
real |
4 |
arcsec |
|
EXTENSION_RAD |
k_r_e |
twomass_xsc |
2MASS |
K Kron elliptical aperture semi-major axis. |
real |
4 |
arcsec |
|
EXTENSION_RAD |
k_r_eff |
twomass_xsc |
2MASS |
K half-light (integrated half-flux point) radius. |
real |
4 |
arcsec |
|
EXTENSION_RAD |
k_r_i20c |
twomass_xsc |
2MASS |
K 20mag/sq." isophotal circular aperture radius. |
real |
4 |
arcsec |
|
EXTENSION_RAD |
k_r_i20e |
twomass_xsc |
2MASS |
K 20mag/sq." isophotal elliptical ap. semi-major axis. |
real |
4 |
arcsec |
|
EXTENSION_RAD |
k_r_i21c |
twomass_xsc |
2MASS |
K 21mag/sq." isophotal circular aperture radius. |
real |
4 |
arcsec |
|
EXTENSION_RAD |
k_r_i21e |
twomass_xsc |
2MASS |
K 21mag/sq." isophotal elliptical ap. semi-major axis. |
real |
4 |
arcsec |
|
EXTENSION_RAD |
k_resid_ann |
twomass_xsc |
2MASS |
K residual annulus background median. |
real |
4 |
DN |
|
CODE_MISC |
k_sc_1mm |
twomass_xsc |
2MASS |
K 1st moment (score) (LCSB: super blk 2,4,8 SNR). |
real |
4 |
|
|
CODE_MISC |
k_sc_2mm |
twomass_xsc |
2MASS |
K 2nd moment (score) (LCSB: SNRMAX - super SNR max). |
real |
4 |
|
|
CODE_MISC |
k_sc_msh |
twomass_xsc |
2MASS |
K median shape score. |
real |
4 |
|
|
CODE_MISC |
k_sc_mxdn |
twomass_xsc |
2MASS |
K mxdn (score) (LCSB: BSNR - block/smoothed SNR). |
real |
4 |
|
|
CODE_MISC |
k_sc_r1 |
twomass_xsc |
2MASS |
K r1 (score). |
real |
4 |
|
|
CODE_MISC |
k_sc_r23 |
twomass_xsc |
2MASS |
K r23 (score) (LCSB: TSNR - integrated SNR for r=15). |
real |
4 |
|
|
CODE_MISC |
k_sc_sh |
twomass_xsc |
2MASS |
K shape (score). |
real |
4 |
|
|
CODE_MISC |
k_sc_vint |
twomass_xsc |
2MASS |
K vint (score). |
real |
4 |
|
|
CODE_MISC |
k_sc_wsh |
twomass_xsc |
2MASS |
K wsh (score) (LCSB: PSNR - peak raw SNR). |
real |
4 |
|
|
CODE_MISC |
k_seetrack |
twomass_xsc |
2MASS |
K band seetracking score. |
real |
4 |
|
|
CODE_MISC |
k_sh0 |
twomass_xsc |
2MASS |
K ridge shape (LCSB: BSNR limit). |
real |
4 |
|
|
FIT_PARAM |
k_shape_avg |
twomass_scn |
2MASS |
Ks-band average seeing shape for scan. |
real |
4 |
|
|
INST_SEEING |
k_shape_rms |
twomass_scn |
2MASS |
RMS-error of Ks-band average seeing shape. |
real |
4 |
|
|
INST_SEEING |
k_sig_sh0 |
twomass_xsc |
2MASS |
K ridge shape sigma (LCSB: B2SNR limit). |
real |
4 |
|
|
FIT_PARAM |
k_snr |
twomass_psc |
2MASS |
Ks-band "scan" signal-to-noise ratio. |
real |
4 |
mag |
|
INST_NOISE |
k_subst2 |
twomass_xsc |
2MASS |
K residual background #2 (score). |
real |
4 |
|
|
CODE_MISC |
k_zp_ap |
twomass_scn |
2MASS |
Photometric zero-point for Ks-band aperture photometry. |
real |
4 |
mag |
|
PHOT_ZP |
k_zperr_ap |
twomass_scn |
2MASS |
RMS-error of zero-point for Ks-band aperture photometry |
real |
4 |
mag |
|
FIT_ERROR |
kAperMag3 |
dxsJKsource, lasExtendedSource, lasPointSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource |
WSA |
Default point/extended source K aperture corrected mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kAperMag3 |
dxsSource, lasSource |
WSA |
Default point/extended source K aperture corrected mag (2.0 arcsec aperture diameter) If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kAperMag3 |
reliableUdsSource |
WSA |
Default point/extended source K mag, no aperture correction applied |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kAperMag3 |
udsSource |
WSA |
Default point/extended source K mag, no aperture correction applied If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kAperMag3Err |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource |
WSA |
Error in default point/extended source K mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kAperMag4 |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource |
WSA |
Extended source K aperture corrected mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kAperMag4 |
reliableUdsSource, udsSource |
WSA |
Extended source K mag, no aperture correction applied |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kAperMag4Err |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource |
WSA |
Error in extended source K mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kAperMag6 |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource |
WSA |
Extended source K aperture corrected mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kAperMag6 |
reliableUdsSource, udsSource |
WSA |
Extended source K mag, no aperture correction applied |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kAperMag6Err |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource |
WSA |
Error in extended source K mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kaStrat |
dxsVarFrameSetInfo, udsVarFrameSetInfo |
WSA |
Strateva parameter a in K band, see Sesar et al. 2007. |
real |
4 |
|
-0.9999995e9 |
|
kbestAper |
dxsVariability, udsVariability |
WSA |
Best aperture (1-6) for photometric statistics in the K band |
int |
4 |
|
-9999 |
|
kbStrat |
dxsVarFrameSetInfo, udsVarFrameSetInfo |
WSA |
Strateva parameter b in K band, see Sesar et al. 2007. |
real |
4 |
|
-0.9999995e9 |
|
kchiSq |
dxsVarFrameSetInfo, udsVarFrameSetInfo |
WSA |
Fit of Strateva function to data in K band |
real |
4 |
|
-0.9999995e9 |
|
kchiSqpd |
dxsVariability, udsVariability |
WSA |
Chi square (per degree of freedom) fit to data (mean and expected rms) |
real |
4 |
|
0.9999995e9 |
|
kClass |
dxsJKsource, dxsSource, dxsSourceRemeasurement, lasExtendedSource, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource, udsSourceRemeasurement |
WSA |
discrete image classification flag in K |
smallint |
2 |
|
-9999 |
CLASS_MISC |
kClassStat |
dxsJKsource, dxsSource, dxsSourceRemeasurement, lasExtendedSource, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKsource, reliableDxsSource, reliableLasPointSource, udsSourceRemeasurement |
WSA |
N(0,1) stellarness-of-profile statistic in K |
real |
4 |
|
-0.9999995e9 |
STAT_PROP |
kClassStat |
reliableUdsSource, udsSource |
WSA |
S-Extractor classification statistic in K |
real |
4 |
|
-0.9999995e9 |
STAT_PROP |
kcStrat |
dxsVarFrameSetInfo, udsVarFrameSetInfo |
WSA |
Strateva parameter a in K band, see Sesar et al. 2007. |
real |
4 |
|
-0.9999995e9 |
|
kDeblend |
dxsJKsource, dxsSourceRemeasurement, lasExtendedSource, lasPointSource, lasSourceRemeasurement, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource, udsSourceRemeasurement |
WSA |
placeholder flag indicating parent/child relation in K |
int |
4 |
|
-99999999 |
CODE_MISC |
kDeblend |
dxsSource, lasSource |
WSA |
placeholder flag indicating parent/child relation in K |
int |
4 |
|
-99999999 |
CODE_MISC |
This CASU pipeline processing source extraction flag is a placeholder only, and is always set to zero in all passbands in the merged source lists. If you need to know when a particular image detection is a component of a deblend or not, test bit 4 of attribute ppErrBits (see corresponding glossary entry) which is set by WFAU's post-processing software based on testing the areal profiles aprof2-8 (these are set by CASU to -1 for deblended components, or positive values for non-deblended detections). We encode this in an information bit of ppErrBits for convenience when querying the merged source tables. |
kEll |
dxsJKsource, dxsSource, dxsSourceRemeasurement, lasExtendedSource, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource, udsSourceRemeasurement |
WSA |
1-b/a, where a/b=semi-major/minor axes in K |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
keNum |
dxsJKmergeLog, dxsMergeLog, lasMergeLog, lasYJHKmergeLog, udsMergeLog |
WSA |
the extension number of this K frame |
tinyint |
1 |
|
|
NUMBER |
kErrBits |
dxsJKsource, dxsSourceRemeasurement, lasExtendedSource, lasPointSource, lasSourceRemeasurement, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSourceRemeasurement |
WSA |
processing warning/error bitwise flags in K |
int |
4 |
|
-99999999 |
CODE_MISC |
kErrBits |
dxsSource, lasSource |
WSA |
processing warning/error bitwise flags in K |
int |
4 |
|
-99999999 |
CODE_MISC |
Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
kErrBits |
udsSource |
WSA |
processing warning/error bitwise flags in K |
int |
4 |
|
-99999999 |
CODE_MISC |
This uses the FLAGS attribute in SE. The individual bit flags that this can be decomposed into are as follows: Bit Flag | Meaning | | 1 | The object has neighbours, bright enough and close enough to significantly bias the MAG_AUTO photometry or bad pixels (more than 10% of photometry affected). | | 2 | The object was originally blended with another | | 4 | At least one pixel is saturated (or very close to) | | 8 | The object is truncated (too close to an image boundary) | | 16 | Object's aperture data are incomplete or corrupted | | 32 | Object's isophotal data are imcomplete or corrupted. This is an old flag inherited from SE v1.0, and is kept for compatability reasons. It doesn't have any consequence for the extracted parameters. | | 64 | Memory overflow occurred during deblending | | 128 | Memory overflow occurred during extraction | |
|
kEta |
dxsJKsource, lasExtendedSource, lasPointSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource |
WSA |
Offset of K detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_DEC_OFF |
kEta |
dxsSource, lasSource, udsSource |
WSA |
Offset of K detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_DEC_OFF |
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; 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. |
kexpML |
dxsVarFrameSetInfo, udsVarFrameSetInfo |
WSA |
Expected magnitude limit of frameSet in this in K band. |
real |
4 |
|
-0.9999995e9 |
|
kExpRms |
dxsVariability, udsVariability |
WSA |
Rms calculated from polynomial fit to minimum RMS as a function of magnitude in K band |
real |
4 |
mag |
-0.9999995e9 |
|
kGausig |
dxsJKsource, dxsSource, dxsSourceRemeasurement, lasExtendedSource, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource, udsSourceRemeasurement |
WSA |
RMS of axes of ellipse fit in K |
real |
4 |
pixels |
-0.9999995e9 |
MORPH_PARAM |
kHallMag |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource |
WSA |
Total point source K mag |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kHallMag |
reliableUdsSource, udsSource |
WSA |
Not available in SE output |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kHallMagErr |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource |
WSA |
Error in total point source K mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kHallMagErr |
reliableUdsSource, udsSource |
WSA |
Not available in SE output |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kIntRms |
dxsVariability, udsVariability |
WSA |
Intrinsic rms in K-band |
real |
4 |
mag |
-0.9999995e9 |
|
kMag |
dxsSourceRemeasurement, lasSourceRemeasurement, udsSourceRemeasurement |
WSA |
K mag (as appropriate for this merged source) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kMag |
ukirtFSstars |
WSA |
K band total magnitude on the MKO(UFTI) system |
real |
4 |
mag |
|
PHOT_INT-MAG |
kMagErr |
dxsSourceRemeasurement, lasSourceRemeasurement, udsSourceRemeasurement |
WSA |
Error in K mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kMagErr |
ukirtFSstars |
WSA |
K band magnitude error |
real |
4 |
mag |
|
ERROR |
kMagMAD |
dxsVariability, udsVariability |
WSA |
Median Absolute Deviation of K magnitude |
real |
4 |
mag |
-0.9999995e9 |
|
kMagRms |
dxsVariability, udsVariability |
WSA |
rms of K magnitude |
real |
4 |
mag |
-0.9999995e9 |
|
kmaxCadence |
dxsVariability, udsVariability |
WSA |
maximum gap between observations |
real |
4 |
days |
-0.9999995e9 |
|
kmeanMag |
dxsVariability, udsVariability |
WSA |
Mean K magnitude |
real |
4 |
mag |
-0.9999995e9 |
|
kmedCadence |
dxsVariability, udsVariability |
WSA |
median gap between observations |
real |
4 |
days |
-0.9999995e9 |
|
kmedianMag |
dxsVariability, udsVariability |
WSA |
Median K magnitude |
real |
4 |
mag |
-0.9999995e9 |
|
kmfID |
dxsJKmergeLog, dxsMergeLog, lasMergeLog, lasYJHKmergeLog, udsMergeLog |
WSA |
the UID of the relevant K multiframe |
bigint |
8 |
|
|
ID_FRAME |
kminCadence |
dxsVariability, udsVariability |
WSA |
minimum gap between observations |
real |
4 |
days |
-0.9999995e9 |
|
knDof |
dxsVarFrameSetInfo, udsVarFrameSetInfo |
WSA |
Number of degrees of freedom of fit in K band. |
smallint |
2 |
|
-9999 |
|
kndof |
dxsVariability, udsVariability |
WSA |
Number of degrees of freedom for chisquare |
int |
4 |
|
-9999 |
|
knFlaggedObs |
dxsVariability |
WSA |
Number of detections in K band flagged as potentially spurious by dxsDetection.ppErrBits |
int |
4 |
|
0 |
|
knFlaggedObs |
udsVariability |
WSA |
Number of detections in K band flagged as potentially spurious by udsDetection.ppErrBits |
int |
4 |
|
0 |
|
knGoodObs |
dxsVariability, udsVariability |
WSA |
Number of good detections in K band |
int |
4 |
|
0 |
|
knMissingObs |
dxsVariability, udsVariability |
WSA |
Number of K band frames that this object should have been detected on and was not |
int |
4 |
|
0 |
|
kObjID |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource |
WSA |
the UID of the K detection |
bigint |
8 |
|
-99999999 |
ID_NUMBER |
kObjID |
dxsSourceRemeasurement, lasSourceRemeasurement, udsSourceRemeasurement |
WSA |
the UID of the K remeasurement |
bigint |
8 |
|
-99999999 |
ID_NUMBER |
kPA |
dxsJKsource, dxsSource, dxsSourceRemeasurement, lasExtendedSource, lasPointSource, lasSource, lasSourceRemeasurement, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource, udsSourceRemeasurement |
WSA |
ellipse fit celestial orientation in K |
real |
4 |
Degrees |
-0.9999995e9 |
POS_POS-ANG |
kPetroMag |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource |
WSA |
Extended source K mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kPetroMagErr |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource |
WSA |
Error in extended source K mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kppErrBits |
dxsJKsource, dxsSourceRemeasurement, lasExtendedSource, lasPointSource, lasSourceRemeasurement, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource, udsSourceRemeasurement |
WSA |
additional WFAU post-processing error bits in K |
int |
4 |
|
0 |
CODE_MISC |
kppErrBits |
dxsSource, lasSource |
WSA |
additional WFAU post-processing error bits in K |
int |
4 |
|
0 |
CODE_MISC |
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 | LAS, GCS, GPS, DXS | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | LAS, GCS, GPS, DXS | 2 | 16 | Close to saturated | 65536 | 0x00010000 | LAS, GCS, GPS | 2 | 19 | Possible crosstalk artefact/contamination | 524288 | 0x00080000 | LAS, GCS, DXS | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | LAS, GCS, GPS, DXS | 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. |
kprobVar |
dxsVariability, udsVariability |
WSA |
Probability of variable from chi-square (and other data) |
real |
4 |
|
0.9999995e9 |
|
kPsfMag |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource |
WSA |
Point source profile-fitted K mag |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kPsfMag |
reliableUdsSource, udsSource |
WSA |
Not available in SE output |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kPsfMagErr |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource |
WSA |
Error in point source profile-fitted K mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kPsfMagErr |
reliableUdsSource, udsSource |
WSA |
Not available in SE output |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kronFlux |
UKIDSSDetection |
WSA |
flux within circular aperture to k × r_k ; k = 2 |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
kronFlux |
dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement |
WSA |
flux within circular aperture to k × r_k ; k = 2 {catalogue TType keyword: Kron_flux} |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
kronFlux |
ptsDetection |
WSATransit |
flux within circular aperture to k × r_k ; k = 2 {catalogue TType keyword: Kron_flux} |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
kronFlux |
udsDetection |
WSA |
flux within Kron radius circular aperture (SE: FLUX_AUTO) {catalogue TType keyword: Kron_flux} |
real |
4 |
ADU |
|
PHOT_INTENSITY_ADU |
kronFluxErr |
UKIDSSDetection |
WSA |
error on Kron flux |
real |
4 |
ADU |
|
ERROR |
kronFluxErr |
dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement |
WSA |
error on Kron flux {catalogue TType keyword: Kron_flux_err} |
real |
4 |
ADU |
|
ERROR |
kronFluxErr |
ptsDetection |
WSATransit |
error on Kron flux {catalogue TType keyword: Kron_flux_err} |
real |
4 |
ADU |
|
ERROR |
kronFluxErr |
udsDetection |
WSA |
error on Kron flux (SE: FLUXERR_AUTO) {catalogue TType keyword: Kron_flux_err} |
real |
4 |
ADU |
|
ERROR |
kronMag |
dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, UKIDSSDetection, udsDetection, udsListRemeasurement |
WSA |
Calibrated Kron magnitude within circular aperture r_k |
real |
4 |
mag |
|
PHOT_INT-MAG |
kronMag |
ptsDetection |
WSATransit |
Calibrated Kron magnitude within circular aperture r_k |
real |
4 |
mag |
|
PHOT_INT-MAG |
kronMagErr |
dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, UKIDSSDetection, udsDetection, udsListRemeasurement |
WSA |
error on calibrated Kron magnitude |
real |
4 |
mag |
|
ERROR |
kronMagErr |
ptsDetection |
WSATransit |
error on calibrated Kron magnitude |
real |
4 |
mag |
|
ERROR |
kronRad |
UKIDSSDetection |
WSA |
r_k as defined in Bertin and Arnouts 1996 A&A Supp 117 393 |
real |
4 |
pixels |
|
EXTENSION_RAD |
kronRad |
dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsListRemeasurement |
WSA |
r_k as defined in Bertin and Arnouts 1996 A&A Supp 117 393 {catalogue TType keyword: Kron_radius} |
real |
4 |
pixels |
|
EXTENSION_RAD |
kronRad |
ptsDetection |
WSATransit |
r_k as defined in Bertin and Arnouts 1996 A&A Supp 117 393 {catalogue TType keyword: Kron_radius} |
real |
4 |
pixels |
|
EXTENSION_RAD |
kronRad |
udsDetection |
WSA |
Kron radius as defined in SE by Graham and Driver (2005) (SE: KRON_RADIUS*A_IMAGE) {catalogue TType keyword: Kron_radius} r_k = ∑R² I(R) / ∑R I(R) |
real |
4 |
pixels |
|
EXTENSION_RAD |
Since <FLUX>_RADIUS is expressed in multiples of the major axis, <FLUX>_RADIUS is multiplied by A_IMAGE to convert to pixels. |
kSeqNum |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource, udsSource |
WSA |
the running number of the K detection |
int |
4 |
|
-99999999 |
ID_NUMBER |
kSeqNum |
dxsSourceRemeasurement, lasSourceRemeasurement, udsSourceRemeasurement |
WSA |
the running number of the K remeasurement |
int |
4 |
|
-99999999 |
ID_NUMBER |
kSerMag2D |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource |
WSA |
Extended source K mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kSerMag2D |
reliableUdsSource, udsSource |
WSA |
Not available in SE output |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
kSerMag2DErr |
dxsJKsource, dxsSource, lasExtendedSource, lasPointSource, lasSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource |
WSA |
Error in extended source K mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kSerMag2DErr |
reliableUdsSource, udsSource |
WSA |
Not available in SE output |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
kskewness |
dxsVariability, udsVariability |
WSA |
Skewness in K band (see Sesar et al. 2007) |
real |
4 |
|
-0.9999995e9 |
|
ktotalPeriod |
dxsVariability, udsVariability |
WSA |
total period of observations (last obs-first obs) |
real |
4 |
days |
-0.9999995e9 |
|
kVarClass |
dxsVariability, udsVariability |
WSA |
Classification of variability in this band |
smallint |
2 |
|
-9999 |
|
kXi |
dxsJKsource, lasExtendedSource, lasPointSource, lasYJHKsource, reliableDxsSource, reliableLasPointSource, reliableUdsSource |
WSA |
Offset of K detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_RA_OFF |
kXi |
dxsSource, lasSource, udsSource |
WSA |
Offset of K detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_RA_OFF |
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; 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. |