M |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
m2u |
[nspid]Multiframe |
WSA NonSurvey |
Raw position of M2 U (N-S tilt) {image primary HDU keyword: M2_U} |
real |
4 |
mrad |
-0.9999995e9 |
|
m2v |
[nspid]Multiframe |
WSA NonSurvey |
Raw position of M2 V (E-W tilt) {image primary HDU keyword: M2_V} |
real |
4 |
mrad |
-0.9999995e9 |
|
m2w |
[nspid]Multiframe |
WSA NonSurvey |
Raw position of M2 W (axial rotation) {image primary HDU keyword: M2_W} |
real |
4 |
mrad |
-0.9999995e9 |
|
m2x |
[nspid]Multiframe |
WSA NonSurvey |
Raw position of M2 X (E-W) {image primary HDU keyword: M2_X} |
real |
4 |
millimetres |
-0.9999995e9 |
|
m2y |
[nspid]Multiframe |
WSA NonSurvey |
Raw position of M2 Y (N-S) {image primary HDU keyword: M2_Y} |
real |
4 |
millimetres |
-0.9999995e9 |
|
m2z |
[nspid]Multiframe |
WSA NonSurvey |
Raw position of M2 Z (focus) {image primary HDU keyword: M2_Z} |
real |
4 |
millimetres |
-0.9999995e9 |
|
M3Temp |
[nspid]Multiframe |
WSA NonSurvey |
M3 temperature {image primary HDU keyword: M3_TEMP} |
real |
4 |
degrees_Kelvin |
-0.9999995e9 |
|
maskID |
[nspid]Multiframe |
WSA NonSurvey |
UID of library object mask frame {image extension keyword: CIR_OPM} |
bigint |
8 |
|
-99999999 |
ID_FRAME |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05ah16aSource (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05ah18aSource (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05ah44bSource (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05b12Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05b13Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05b15Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05b17Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05b19Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05b3Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05b7Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05bd1Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05bh24Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05bh47Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05bh53Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05bj1Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05bj3Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u05bj4Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06a10Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06a12Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06a24Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06a35Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06a3Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06a40Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06a48Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06ad5Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06ah13Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06ah43Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06aj2Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06b12Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06b13Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06b24Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06b30Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06b36Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06b40Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06bh22Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u06bj5Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07a24Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07ah16Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07ah30Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07ah32Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07ah51Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07ah8Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07b11Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07b13Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07b20Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07b29Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07b36Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07b5Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07b6Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07bd2Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07bd3Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07bd4Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u07bh49Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08a14Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08a15Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08a1Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08a32Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08b14Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08b33Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08b5Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08bh27Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08bh2Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08bh45Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08bh55Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08bh9Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u08bj10Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u09a1Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u09a2Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u09a5Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u09ad1Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in u09ak1Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in ucmp4Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1625Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1636Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1639Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1650Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1652Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1671Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1672Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1673Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1674Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1675Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1677Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1678Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1706Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1707Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1708Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1709Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1711Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1720Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1721Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1731Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1735Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1736Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1737Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1741Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1743Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1747Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1759Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1761Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1764Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1781Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1782Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1788Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1799Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1800Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1801Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1802Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1820Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1831Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours |
WSA NonSurvey |
The unique ID in userv1836Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours, [nspid]SourceXDetection |
WSA NonSurvey |
The unique ID in u05a3Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
masterObjID |
[nspid]SourceNeighbours, [nspid]SourceXtwomass_psc |
WSA NonSurvey |
The unique ID in u05a37Source (=sourceID) |
bigint |
8 |
|
|
ID_MAIN |
maxDec |
[nspid]CurrentAstrometry, [nspid]PreviousAstrometry |
WSA NonSurvey |
The maximum Dec (J2000) on the device |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
maxPllx |
[nspid]Variability |
WSA NonSurvey |
Upper limit of 90% confidence interval for parallax measurement |
real |
4 |
mas |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
maxRa |
[nspid]CurrentAstrometry, [nspid]PreviousAstrometry |
WSA NonSurvey |
The maximum RA (J2000) on the device |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_RA_OTHER |
maxSeeing |
[nspid]RequiredMosaic, [nspid]RequiredStack |
WSA NonSurvey |
The maximum allowed seeing for intermediate stacks |
real |
4 |
arcsec |
|
|
maxStelEll |
[nspid]RequiredMosaic, [nspid]RequiredStack |
WSA NonSurvey |
The maximum allowed stellar ellipticity for intermediate stacks |
real |
4 |
|
|
|
mergedClass |
[nspid]Source |
WSA NonSurvey |
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. |
mergedClassStat |
[nspid]Source |
WSA NonSurvey |
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 multiplying by N1/2 such that cuts on mergedClassStat result in completeness being independent of number of frames an object appears on, but with reliability improving with the number of frames. |
mergeLogTable |
[nspid]Programme |
WSA NonSurvey |
Table name of curation log for source merging |
varchar |
64 |
|
|
?? |
mergeSwVersion |
[nspid]MergeLog |
WSA NonSurvey |
version number of the software used to merge the frames |
real |
4 |
|
|
ID_VERSION |
method |
[nspid]RequiredDiffImage |
WSA NonSurvey |
CASU difference image tool option string specifying the method to employ (recommended value=adaptive/back/zerosky) |
varchar |
64 |
|
|
?? |
minDec |
[nspid]CurrentAstrometry, [nspid]PreviousAstrometry |
WSA NonSurvey |
The minimum Dec (J2000) on the device |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
minImageSize |
[nspid]MultiframeDetector |
WSA NonSurvey |
Minimum size for images {catalogue extension keyword: MINPIX} |
int |
4 |
pixels |
-99999999 |
?? |
Tunable parameter, in conjunction with the threshold above this determines how deep and how small "real" images can be. The 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. |
minPllx |
[nspid]Variability |
WSA NonSurvey |
Lower limit of 90% confidence interval for parallax measurement |
real |
4 |
mas |
-0.9999995e9 |
|
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
minRa |
[nspid]CurrentAstrometry, [nspid]PreviousAstrometry |
WSA NonSurvey |
The minimum RA (J2000) on the device |
float |
8 |
Degrees |
-0.9999995e9 |
POS_EQ_RA_OTHER |
mirrBottTempNW |
[nspid]Multiframe |
WSA NonSurvey |
Mirror bottom temp. NW {image primary HDU keyword: MIRRBTNW} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mirrTempNE |
[nspid]Multiframe |
WSA NonSurvey |
Mirror temperature NE {image primary HDU keyword: MIRR_NE} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mirrTempNW |
[nspid]Multiframe |
WSA NonSurvey |
Mirror temperature NW {image primary HDU keyword: MIRR_NW} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mirrTempSE |
[nspid]Multiframe |
WSA NonSurvey |
Mirror temperature SE {image primary HDU keyword: MIRR_SE} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mirrTempSW |
[nspid]Multiframe |
WSA NonSurvey |
Mirror temperature SW {image primary HDU keyword: MIRR_SW} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mirrTopTempNW |
[nspid]Multiframe |
WSA NonSurvey |
Mirror top temp. NW {image primary HDU keyword: MIRRTPNW} |
real |
4 |
degrees_Celsius |
-0.9999995e9 |
PHYS_TEMP_MISC |
mjdObs |
[nspid]Multiframe |
WSA NonSurvey |
Modified Julian Date of the observation {image primary HDU keyword: MJD-OBS} |
float |
8 |
|
-0.9999995e9 |
TIME_DATE |
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05a3Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05ah16aSource variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05ah18aSource variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05ah44bSource variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05b12Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05b13Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05b17Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05b19Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05b3Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05bh24Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05bh47Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05bh53Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05bj1Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u05bj3Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06a10Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06a12Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06a35Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06a3Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06a40Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06ad5Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06ah13Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06aj2Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06b12Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06b30Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06b40Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06bh22Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u06bj5Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07a24Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07ah16Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07ah30Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07ah32Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07ah51Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07ah8Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07b11Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07b13Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07b20Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07b5Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07b6Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u07bd2Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u08a15Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u08bh2Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u08bh45Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u08bh9Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u08bj10Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u09a1Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u09a5Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in u09ak1Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in ucmp4Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1639Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1671Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1675Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1677Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1707Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1709Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1720Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1721Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1735Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1736Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1737Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1747Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1759Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1799Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1800Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1801Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1802Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1820Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
modelDistSecs |
[nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
separation from expected position given astrometric model in userv1836Source variability. |
real |
4 |
arcsec |
-0.9999995e9 |
|
morphClassFlag |
[nspid]MultiframeDetector |
WSA NonSurvey |
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 |
mosaicTool |
[nspid]Programme |
WSA NonSurvey |
Name of mosaicing tool to be used |
varchar |
8 |
|
NONE |
?? |
motionModel |
[nspid]VarFrameSetInfo |
WSA NonSurvey |
Motion model used to produce BestMatch table. Values: static;proper motion;proper motion and parallax. |
varchar |
32 |
|
static |
|
Motion model for frameset in question. This can be static: all objects in the frameset are assumed to be stationary; proper motion: all objects in the frameset are fit for a linear proper motion; proper motion and parallax: all objects in the frameset are fit for a linear proper motion and a parallax. In all cases, objects are assumed to be stars with small values of proper motion and parallax. |
msbID |
[nspid]Multiframe |
WSA NonSurvey |
Id min.-schedulable block {image primary HDU keyword: MSBID} |
varchar |
64 |
|
NONE |
ID_NUMBER |
msbRejected |
[nspid]Multiframe |
WSA NonSurvey |
Cause of MSB rejection, default if not rejected {image primary HDU keyword: MSBFUD} |
varchar |
256 |
|
NONE |
|
muDec |
[nspid]Variability |
WSA NonSurvey |
Proper motion in Dec |
real |
4 |
mas/yr |
-0.9999995e9 |
POS_EQ_PMDEC |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |
multiframeID |
[nspid]CurrentAstrometry, [nspid]Detection, [nspid]MultiframeDetector, [nspid]PreviousAstrometry, [nspid]PreviousMFDZP, [nspid]ProgrammeFrame, [nspid]SourceXDetectionBestMatch |
WSA NonSurvey |
the UID of the relevant multiframe |
bigint |
8 |
|
|
ID_FRAME |
multiframeID |
[nspid]Multiframe |
WSA NonSurvey |
UID of the multiframe (assigned sequentially by the archive ingest process) |
bigint |
8 |
|
|
ID_FRAME |
multiframeID |
[nspid]Provenance |
WSA NonSurvey |
the UID of the component frame |
bigint |
8 |
|
|
ID_FRAME |
muRa |
[nspid]Variability |
WSA NonSurvey |
Proper motion in RA |
real |
4 |
mas/yr |
-0.9999995e9 |
POS_EQ_PMRA |
The Variability table contains statistics from the set of observations of each source. At present, the mean ra and dec and the error in two tangential directions are calculated. The "ra" direction is defined as tangential to both the radial direction and the cartesian z-axis and the "dec" direction is defined as both the radial direction and the "ra" direction. Since the current model is just the mean and standard deviation of the data, then the chi-squared of the fit=1. Data from good frames across all bands go into the astrometric model determination. This will include bands in non-synoptic filters: the one observation in these bands can help. In future releases a fit will be made to the rms data as a function of magnitude in each band, as has already happened for photometric data and a motion model that incorporates proper motion (and possibly parallax) will be used. The motion model is a parameter in the VarFrameSetInfo table. |