M |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
M1 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Number of detections for band 1 |
int |
4 |
|
-9 |
|
M2 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Number of detections for band 2 |
int |
4 |
|
-9 |
|
m2u |
Multiframe |
WSA |
Raw position of M2 U (N-S tilt) {image primary HDU keyword: M2_U} |
real |
4 |
mrad |
-0.9999995e9 |
|
m2v |
Multiframe |
WSA |
Raw position of M2 V (E-W tilt) {image primary HDU keyword: M2_V} |
real |
4 |
mrad |
-0.9999995e9 |
|
m2w |
Multiframe |
WSA |
Raw position of M2 W (axial rotation) {image primary HDU keyword: M2_W} |
real |
4 |
mrad |
-0.9999995e9 |
|
m2x |
Multiframe |
WSA |
Raw position of M2 X (E-W) {image primary HDU keyword: M2_X} |
real |
4 |
millimetres |
-0.9999995e9 |
|
m2y |
Multiframe |
WSA |
Raw position of M2 Y (N-S) {image primary HDU keyword: M2_Y} |
real |
4 |
millimetres |
-0.9999995e9 |
|
m2z |
Multiframe |
WSA |
Raw position of M2 Z (focus) {image primary HDU keyword: M2_Z} |
real |
4 |
millimetres |
-0.9999995e9 |
|
M3 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Number of detections for band 3 |
int |
4 |
|
-9 |
|
M3Temp |
Multiframe |
WSA |
M3 temperature {image primary HDU keyword: M3_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
M4 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Number of detections for band 4 |
int |
4 |
|
-9 |
|
mag1 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Magnitude in IRAC band 1 |
real |
4 |
mag |
99.999 |
|
mag1_err |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
1sigma mag error (IRAC band 1) |
real |
4 |
mag |
99.999 |
|
mag2 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Magnitude in IRAC band 2 |
real |
4 |
mag |
99.999 |
|
mag2_err |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
1sigma mag error (IRAC band 2) |
real |
4 |
mag |
99.999 |
|
mag3 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Magnitude in IRAC band 3 |
real |
4 |
mag |
99.999 |
|
mag3_err |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
1sigma mag error (IRAC band 3) |
real |
4 |
mag |
99.999 |
|
mag4 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Magnitude in IRAC band 4 |
real |
4 |
mag |
99.999 |
|
mag4_err |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
1sigma mag error (IRAC band 4) |
real |
4 |
mag |
99.999 |
|
magCol |
Plate |
SSA |
Name of magnitude column in reference catalogue |
varchar |
16 |
|
|
REMARKS |
magLimit |
Survey |
SSA |
Nominal mag limit of survey, eg. 22.5 for Bj |
real |
4 |
|
|
PHOT_MAG_LIMIT |
magMax |
Plate |
SSA |
Maximum instrumental mag in IAM file |
real |
4 |
|
|
PHOT_MAG_LIMIT |
magMin |
Plate |
SSA |
Minimum instrumental mag in IAM file |
real |
4 |
|
|
PHOT_MAG_LIMIT |
maj |
firstSource |
FIRST |
major axes derived from the elliptical Gaussian model for the source after deconvolution. |
real |
4 |
arcsec |
|
EXTENSION_FWHM_MAJ |
major |
iras_psc |
IRAS |
Uncertainty ellipse major axis |
smallint |
2 |
arcsec |
|
ERROR |
maskID |
Multiframe |
WSA |
UID of library object mask frame {image extension keyword: CIR_OPM} |
bigint |
8 |
|
-99999999 |
ID_FRAME |
masterObjID |
dxsSourceNeighbours, dxsSourceXtwomass_psc |
WSA |
The unique ID in dxsSource (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
gcsSourceNeighbours, gcsSourceXtwomass_psc |
WSA |
The unique ID in gcsSource (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
gpsSourceNeighbours, gpsSourceXglimpse_hrc_inter, gpsSourceXglimpse_mca_inter, gpsSourceXtwomass_psc |
WSA |
The unique ID in gpsSource (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
lasSourceNeighbours, lasSourceXDR2PhotoObj, lasSourceXSSASource, lasSourceXfirstSource, lasSourceXiras_psc, lasSourceXrosat_bsc, lasSourceXrosat_fsc, lasSourceXtwomass_psc, lasSourceXtwomass_xsc |
WSA |
The unique ID in lasSource (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
udsSourceNeighbours, udsSourceXtwomass_psc |
WSA |
The unique ID in udsSource (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
maxDec |
CurrentAstrometry, PreviousAstrometry |
WSA |
The maximum Dec (J2000) on the device |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
maxIter |
Plate |
SSA |
Maximum no. of iterations for non-linear astrometric fit |
int |
4 |
|
|
NUMBER |
maxRa |
CurrentAstrometry, PreviousAstrometry |
WSA |
The maximum RA (J2000) on the device |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_RA_OTHER |
meanClass |
Source |
SSA |
Estimate of image class based on unit-weighted mean of individual classes |
tinyint |
1 |
|
|
CLASS_OBJECT |
mergedClass |
dxsSource, gcsSource, gpsSource, lasSource, udsSource |
WSA |
Class flag from available measurements (1|0|-1|-2|-3|-9=galaxy|noise|stellar|probableStar|probableGalaxy|saturated) |
smallint |
2 |
|
|
CODE_MISC |
Individual detection classifications are combined in the source merging process to produce a set of attributes for each merged source as follows. Presently, a basic classification table is defined that assigns reasonably accurate, self-consistent probability values for a given classification code: Flag | Meaning | Probability (%) | | | Star | Galaxy | Noise | Saturated | -9 | Saturated | 0.0 | 0.0 | 5.0 | 95.0 | -3 | Probable galaxy | 25.0 | 70.0 | 5.0 | 0.0 | -2 | Probable star | 70.0 | 25.0 | 5.0 | 0.0 | -1 | Star | 90.0 | 5.0 | 5.0 | 0.0 | 0 | Noise | 5.0 | 5.0 | 90.0 | 0.0 | +1 | Galaxy | 5.0 | 90.0 | 5.0 | 0.0 | Then, each separately available classification is combined for a merged source using Bayesian classification rules, assuming each datum is independent: P(classk)=ΠiP(classk)i / ΣkΠiP(classk)i where classk is one of star|galaxy|noise|saturated, and i denotes the ith single detection passband measurement available (the non-zero entries are necessary for the independent measures method to work, since some cases might otherwise be mutually exclusive). For example, if an object is classed in J|H|K as -1|-2|+1 it would have merged classification probabilities of pStar=73.5%, pGalaxy=26.2%, pNoise=0.3% and pSaturated=0.0%. Decision thresholds for the resulting discrete classification flag mergedClass are 90% for definitive and 70% for probable; hence the above example would be classified (not unreasonably) as probably a star (mergedClass=-2). An additional decision rule enforces mergedClass=-9 (saturated) when any individual classification flag indicates saturation. |
mergedClass |
dxsSourceRemeasurement, gcsSourceRemeasurement, gpsSourceRemeasurement, lasSourceRemeasurement, udsSourceRemeasurement |
WSA |
Class flag based on list remeasurement prescription |
smallint |
2 |
|
|
CODE_MISC |
mergedClassStat |
dxsSource, gcsSource, gpsSource, lasSource, udsSource |
WSA |
Merged N(0,1) stellarness-of-profile statistic |
real |
4 |
|
-0.9999995e9 |
STAT_PROP |
This profile classification statistic is a continuously distributed, Gaussian N(0,1) (i.e. zero mean, unit variance) statistic formed from the available individual classification statistics by averaging them and dividing by N1/2. |
mergeLogTable |
Programme |
WSA |
Table name of curation log for source merging |
varchar |
64 |
|
|
?? |
mergeSwVersion |
dxsMergeLog, gcsMergeLog, gpsMergeLog, lasMergeLog, udsMergeLog |
WSA |
version number of the software used to merge the frames |
real |
4 |
|
|
ID_VERSION |
method |
RequiredDiffImage |
WSA |
CASU difference image tool option string specifying the method to employ (recommended value=adaptive/back/zerosky) |
varchar |
64 |
|
|
?? |
MF1 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Flux calc mathod flag for band 1 flux |
int |
4 |
|
-9 |
|
MF2 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Flux calc mathod flag for band 2 flux |
int |
4 |
|
-9 |
|
MF3 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Flux calc mathod flag for band 3 flux |
int |
4 |
|
-9 |
|
MF4 |
glimpse_hrc_inter, glimpse_mca_inter |
GLIMPSE |
Flux calc mathod flag for band 4 flux |
int |
4 |
|
-9 |
|
mFlag |
rosat_bsc, rosat_fsc |
ROSAT |
source missed by SASS |
varchar |
1 |
|
|
CODE_MISC |
mHcon |
iras_psc |
IRAS |
Possible number of HCONs |
tinyint |
1 |
|
|
NUMBER |
min |
firstSource |
FIRST |
minor axes derived from the elliptical Gaussian model for the source after deconvolution. |
real |
4 |
arcsec |
|
EXTENSION_FWHM_MIN |
minDec |
CurrentAstrometry, PreviousAstrometry |
WSA |
The minimum Dec (J2000) on the device |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
minImageSize |
MultiframeDetector |
WSA |
Minimum size for images {catalogue extension keyword: MINPIX} |
int |
4 |
pixels |
-99999999 |
?? |
User-selectable parameter, in conjunction with the threshold above this determines how deep and how small "real" images can be. This default precludes many of the few pixel-hit cosmic rays from being considered since "real" images must have 4 contiguous simply-connected pixels in the union of the detection filter and data domains. For more details on image detection and parametersiation see the papers in CASU WFCAM/VISTA Publications. |
minor |
iras_psc |
IRAS |
Uncertainty ellipse minor axis |
smallint |
2 |
arcsec |
|
ERROR |
minRa |
CurrentAstrometry, PreviousAstrometry |
WSA |
The minimum RA (J2000) on the device |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_RA_OTHER |
mirrBottTempNW |
Multiframe |
WSA |
Mirror bottom temp. NW {image primary HDU keyword: MIRRBTNW} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mirrTempNE |
Multiframe |
WSA |
Mirror temperature NE {image primary HDU keyword: MIRRNE} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mirrTempNW |
Multiframe |
WSA |
Mirror temperature NW {image primary HDU keyword: MIRRNW} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mirrTempSE |
Multiframe |
WSA |
Mirror temperature SE {image primary HDU keyword: MIRRSE} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mirrTempSW |
Multiframe |
WSA |
Mirror temperature SW {image primary HDU keyword: MIRRSW} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mirrTopTempNW |
Multiframe |
WSA |
Mirror top temp. NW {image primary HDU keyword: MIRRTPNW} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mjd |
Plate |
SSA |
Modified Julian Date at mid exposure |
float |
8 |
Julian days |
|
TIME_DATE |
mjdObs |
Multiframe |
WSA |
Modified Julian Date of the observation {image primary HDU keyword: MJD-OBS} |
float |
8 |
|
-0.9999995e9 |
TIME_DATE |
modDate |
rosat_bsc, rosat_fsc |
ROSAT |
date when source properties were changed (MM-DD-YYYY) |
datetime |
8 |
mm-dd-yyyy |
|
TIME_DATE |
morphClassFlag |
MultiframeDetector |
WSA |
Image morphological classifier flag, set if the classifier has been run. If so an object classification flag and a stellarness index is included in the binary table columns. {catalogue extension keyword: CLASSIFD} |
tinyint |
1 |
|
0 |
CODE_MISC |
mosaicID |
MosaicImage |
WSA |
the unique ID number identifying all stored mosaic images |
bigint |
8 |
|
|
ID_FRAME |
mosaicStacks |
RequiredMosaic |
WSA |
Indicates if stacks are to be mosaiced (=1) or not (=0) |
tinyint |
1 |
|
|
?? |
mp_flg |
twomass_psc |
2MASS |
Minor Planet Flag. |
smallint |
2 |
|
|
CODE_MISC |
mp_key |
twomass_xsc |
2MASS |
key to minor planet prediction DB record. |
int |
4 |
|
|
ID_NUMBER |
msbID |
Multiframe |
WSA |
Id min.-schedulable block {image primary HDU keyword: MSBID} |
varchar |
64 |
|
NONE |
ID_NUMBER |
muAcosD |
Source |
SSA |
Proper motion in RA direction |
real |
4 |
mas/yr |
-0.99999995e9 |
POS_EQ_PMRA |
muD |
Source |
SSA |
Proper motion in Dec direction |
real |
4 |
mas/yr |
-0.99999995e9 |
POS_EQ_PMDEC |
muDec |
gcsSource, gpsSource, lasSource |
WSA |
Proper motion in Dec direction |
real |
4 |
mas/yr |
-0.9999995e9 |
POS_EQ_PMDEC |
multiframeID |
CurrentAstrometry, dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, MultiframeDetector, PreviousAstrometry, ProgrammeFrame, udsDetection, udsListRemeasurement |
WSA |
the UID of the relevant multiframe |
bigint |
8 |
|
|
ID_FRAME |
multiframeID |
Multiframe |
WSA |
UID of the multiframe (assigned sequentially by the archive ingest process) |
bigint |
8 |
|
|
ID_FRAME |
multiframeID |
Provenance |
WSA |
the UID of the component frame |
bigint |
8 |
|
|
ID_FRAME |
muRa |
gcsSource, gpsSource, lasSource |
WSA |
Proper motion in RA direction |
real |
4 |
mas/yr |
-0.9999995e9 |
POS_EQ_PMRA |