O |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
object |
[nspid]Multiframe |
WSA NonSurvey |
Object name from telescope {image primary HDU keyword: OBJECT} |
varchar |
64 |
|
NONE |
meta.id |
objectID |
[nspid]MapApertureIDshighzQsoMap |
WSA NonSurvey |
The UID of the object within this survey programme table |
bigint |
8 |
|
|
|
objID |
[nspid]Detection |
WSA NonSurvey |
Unique identifier for this detection or default for no detection |
bigint |
8 |
|
-99999999 |
ID_MAIN |
This attribute is included to provide a single identification number for real detection rows (objID>0) when making cross-neighbour tables between source and detection. In general, users should NOT use this attribute for look-ups between the source and detection tables, because every detector frame has a default row in the detection table, so there are many, many thousands of rows with objID=-99999999 in each detection table which will be associated with every look-up of objID=-99999999 from source (i.e. those rows for which there is no detection or no frame in a particular passband). See the glossary entry for objID in source tables for more information. |
objID |
[nspid]FSstars |
WSA NonSurvey |
Faint standard unique identifier (FS number; see Hawarden et al. 2001, MN, 325, 563) |
bigint |
8 |
|
|
|
objID |
[nspid]UKIDSSDetection |
WSA NonSurvey |
Unique identifier for this detection or default for no detection |
bigint |
8 |
|
-99999999 |
ID_MAIN |
objIDName |
[nspid]MapSurveyTables |
WSA NonSurvey |
The source unique identifier in the table |
varchar |
16 |
|
|
ID_TARGET |
obReqs |
[nspid]RequiredFilters |
WSA NonSurvey |
For wide shallow surveys with small number of epochs, what MSB requirements for each epoch. |
varchar |
32 |
|
NONE |
meta.note |
observed |
[nspid]StdFieldInfo |
WSA NonSurvey |
yes or no identifier - have the secondary standards been set up? |
tinyint |
1 |
|
0 |
|
observer |
[nspid]Multiframe |
WSA NonSurvey |
Observers names {image primary HDU keyword: OBSERVER} |
varchar |
64 |
|
NONE |
obs.observer |
obsNum |
[nspid]Multiframe |
WSA NonSurvey |
Observation number {image primary HDU keyword: OBSNUM} |
int |
4 |
|
-99999999 |
meta.number |
obsref |
[nspid]Multiframe |
WSA NonSurvey |
PATT or other reference {image primary HDU keyword: OBSREF} |
varchar |
64 |
|
NONE |
meta.bib |
obstype |
[nspid]Multiframe |
WSA NonSurvey |
Type (BIAS|DARK|ARC|FLAT|OBJECT|SKY) {image primary HDU keyword: OBSTYPE} |
varchar |
32 |
|
|
?? |
oneSecMLVg |
[nspid]Filter |
WSA NonSurvey |
The Vega magnitude limit of a 1s exposure in this filter |
real |
4 |
mag |
-0.9999995e9 |
|
orbitID |
[nspid]SatelliteOrbits |
WSA NonSurvey |
UID of the orbit as assigned by fitting algorith |
bigint |
8 |
|
|
ID_MAIN |
orbitID |
[nspid]SatelliteOrbitsTrails |
WSA NonSurvey |
UID of orbit |
bigint |
8 |
|
|
ID_MAIN |
orient |
[nspid]AstrometricInfo |
WSA NonSurvey |
Orientation of axes |
float |
8 |
radians |
-0.9999995e9 |
?? |
orientation |
[nspid]RequiredMosaicTopLevel |
WSA NonSurvey |
Orientation of image x-axis to N-S. If default, use natural orientation of input images. |
real |
4 |
deg |
-0.9999995e9 |
|
origin |
[nspid]Multiframe |
WSA NonSurvey |
Origin of this FITS file (eg. UKIRT) {image primary HDU keyword: ORIGIN} |
varchar |
32 |
|
NONE |
|
overLaps |
[nspid]RequiredMapAverages |
WSA NonSurvey |
Average over overlaps (use with average over deep frames and source merging) 0/N N/Y |
tinyint |
1 |
|
0 |
|