J |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
jAperMag3 |
[nspid]Source |
WSA NonSurvey |
Extended source J mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
jAperMag3Err |
[nspid]Source |
WSA NonSurvey |
Error in extended source J mag (2.0 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
jAperMag4 |
[nspid]Source |
WSA NonSurvey |
Extended source J mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
jAperMag4Err |
[nspid]Source |
WSA NonSurvey |
Error in extended source J mag (2.8 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
jAperMag6 |
[nspid]Source |
WSA NonSurvey |
Extended source J mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
jAperMag6Err |
[nspid]Source |
WSA NonSurvey |
Error in extended source J mag (5.7 arcsec aperture diameter) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
jClass |
[nspid]Source |
WSA NonSurvey |
discrete image classification flag in J |
smallint |
2 |
|
-9999 |
CLASS_MISC |
jClassStat |
[nspid]Source |
WSA NonSurvey |
N(0,1) stellarness-of-profile statistic in J |
real |
4 |
|
-0.9999995e9 |
STAT_PROP |
jDeblend |
[nspid]Source |
WSA NonSurvey |
flag indicating parent/child relation in J |
int |
4 |
|
-99999999 |
CODE_MISC |
jEll |
[nspid]Source |
WSA NonSurvey |
1-b/a, where a/b=semi-major/minor axes in J |
real |
4 |
|
-0.9999995e9 |
PHYS_ELLIPTICITY |
jeNum |
[nspid]MergeLog |
WSA NonSurvey |
the extension number of this J detector |
tinyint |
1 |
|
|
NUMBER |
jErrBits |
[nspid]Source |
WSA NonSurvey |
processing warning/error bitwise flags in J |
int |
4 |
|
-99999999 |
CODE_MISC |
jEta |
[nspid]Source |
WSA NonSurvey |
Offset of J 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 typically 5 arcseconds is used, 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, 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. |
jGausig |
[nspid]Source |
WSA NonSurvey |
RMS of axes of ellipse fit in J |
real |
4 |
pixels |
-0.9999995e9 |
MORPH_PARAM |
jHallMag |
[nspid]Source |
WSA NonSurvey |
Point source J mag |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
jHallMagErr |
[nspid]Source |
WSA NonSurvey |
Error in point source J mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
jitterID |
[nspid]Multiframe |
WSA NonSurvey |
Serial number in this telescope jitter pattern {image primary HDU keyword: JITTER_I} |
smallint |
2 |
|
-9999 |
ID_NUMBER |
jitterX |
[nspid]Multiframe |
WSA NonSurvey |
X (RA) offset in tel jitter pattern {image primary HDU keyword: JITTER_X} |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_RA_OFF |
jitterY |
[nspid]Multiframe |
WSA NonSurvey |
Y (Dec) offset in tel jitter pattern {image primary HDU keyword: JITTER_Y} |
real |
4 |
arcsec |
-0.9999995e9 |
POS_EQ_DEC_OFF |
jmfID |
[nspid]MergeLog |
WSA NonSurvey |
the UID of the relevant J multiframe |
bigint |
8 |
|
|
ID_FRAME |
jmhExt |
[nspid]Source |
WSA NonSurvey |
Extended source colour J-H |
real |
4 |
mag |
-0.9999995e9 |
PHOT_COLOR |
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 are computed from the seeing-matched aperture measure (the "Hall" magnitude) while the extended source colours are computed from the fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands). 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. |
jmhExtErr |
[nspid]Source |
WSA NonSurvey |
Error on extended source colour J-H |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
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 are computed from the seeing-matched aperture measure (the "Hall" magnitude) while the extended source colours are computed from the fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands). 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. |
jmhPnt |
[nspid]Source |
WSA NonSurvey |
Point source colour J-H |
real |
4 |
mag |
-0.9999995e9 |
PHOT_COLOR |
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 are computed from the seeing-matched aperture measure (the "Hall" magnitude) while the extended source colours are computed from the fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands). 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. |
jmhPntErr |
[nspid]Source |
WSA NonSurvey |
Error on point source colour J-H |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
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 are computed from the seeing-matched aperture measure (the "Hall" magnitude) while the extended source colours are computed from the fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands). 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. |
jmkExt |
[nspid]Source |
WSA NonSurvey |
Extended source colour J-K |
real |
4 |
mag |
-0.9999995e9 |
PHOT_COLOR |
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 are computed from the seeing-matched aperture measure (the "Hall" magnitude) while the extended source colours are computed from the fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands). 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. |
jmkExtErr |
[nspid]Source |
WSA NonSurvey |
Error on extended source colour J-K |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
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 are computed from the seeing-matched aperture measure (the "Hall" magnitude) while the extended source colours are computed from the fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands). 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. |
jmkPnt |
[nspid]Source |
WSA NonSurvey |
Point source colour J-K |
real |
4 |
mag |
-0.9999995e9 |
PHOT_COLOR |
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 are computed from the seeing-matched aperture measure (the "Hall" magnitude) while the extended source colours are computed from the fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands). 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. |
jmkPntErr |
[nspid]Source |
WSA NonSurvey |
Error on point source colour J-K |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
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 are computed from the seeing-matched aperture measure (the "Hall" magnitude) while the extended source colours are computed from the fixed 2 arcsec aperture diameter measures (for consistent measurement across all passbands). 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. |
jObjID |
[nspid]Source |
WSA NonSurvey |
the UID of the J detection |
bigint |
8 |
|
-99999999 |
ID_NUMBER |
joinCriterion |
[nspid]RequiredNeighbours |
WSA NonSurvey |
The join criterion (search radius for matches) |
real |
4 |
arcminutes |
|
?? |
joinType |
[nspid]RequiredNeighbours |
WSA NonSurvey |
The type of join: 0 (default) or N for special join |
smallint |
2 |
|
|
?? |
jPA |
[nspid]Source |
WSA NonSurvey |
ellipse fit celestial orientation in J |
real |
4 |
Degrees |
-0.9999995e9 |
POS_POS-ANG |
jPetroMag |
[nspid]Source |
WSA NonSurvey |
Extended source J mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
jPetroMagErr |
[nspid]Source |
WSA NonSurvey |
Error in extended source J mag (Petrosian) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
jppErrBits |
[nspid]Source |
WSA NonSurvey |
additional WFAU post-processing error bits in J |
int |
4 |
|
-99999999 |
CODE_MISC |
jPsfMag |
[nspid]Source |
WSA NonSurvey |
Point source profile-fitted J mag |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
jPsfMagErr |
[nspid]Source |
WSA NonSurvey |
Error in point source profile-fitted J mag |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
jSeqNum |
[nspid]Source |
WSA NonSurvey |
the running number of the J detection |
int |
4 |
|
-99999999 |
ID_NUMBER |
jSerMag2D |
[nspid]Source |
WSA NonSurvey |
Extended source J mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
PHOT_MAG |
jSerMag2DErr |
[nspid]Source |
WSA NonSurvey |
Error in extended source J mag (profile-fitted) |
real |
4 |
mag |
-0.9999995e9 |
ERROR |
julianDayNum |
[nspid]CurrentNightlyExt, [nspid]DetectorSetUp, [nspid]MultiframeSetUp, [nspid]PreviousNightlyExt |
WSA NonSurvey |
the Julian Day number of the UKIRT night {image primary HDU keyword: UTDATE} |
int |
4 |
Julian days |
|
TIME_DATE |
julianDayNum |
[nspid]Multiframe |
WSA NonSurvey |
the Julian Day number of the UKIRT night |
int |
4 |
Julian days |
|
TIME_DATE |
julianDayNum |
[nspid]MultiframeDetector |
WSA NonSurvey |
Julian Day number of the UKIRT night {image primary HDU keyword: UTDATE} |
int |
4 |
Julian days |
|
TIME_DATE |
jXi |
[nspid]Source |
WSA NonSurvey |
Offset of J 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 typically 5 arcseconds is used, 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, 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. |