C |
| Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
| c_strat |
twomass_scn |
TWOMASS |
Flag indicating the calibration strategy for this night's data. |
smallint |
2 |
|
|
meta.code |
| c_strat |
twomass_sixx2_scn |
TWOMASS |
calibration strategy, north only (0=old, 1=new) |
smallint |
2 |
|
|
|
| cat |
twomass_sixx2_psc, twomass_sixx2_scn, twomass_sixx2_xsc |
TWOMASS |
Catalog indicator 1=catalog, 0=not catalog |
smallint |
2 |
|
|
|
| catalogueSchema |
Programme |
VULCANiDR |
Script file that describes the catalogue schema |
varchar |
64 |
|
|
?? |
| cc_flags |
allwise_sc |
WISE |
Contamination and confusion flag. Four character string, one character per band [W1/W2/W3/W4], that indicates that the photometry and/or position measurements of a source may be contaminated or biased due to proximity to an image artifact. CAUTION: Non-zero cc_flags values in any band indicate the the measurement in that band may be contaminated and the photometry should be used with caution. |
varchar |
4 |
|
|
|
The type of artifact that may contaminate the measurements is denoted by the following codes. Lower-case letters correspond to instances in which the source detection in a band is believed to be real but the measurement may be contaminated by the artifact. Upper-case letters are instances in which the source detection in a band may be a spurious detection of an artifact. - D,d - Diffraction spike. Source may be a spurious detection of (D) or contaminated by (d) a diffraction spike from a nearby bright star on the same image, or
- P,p - Persistence. Source may be a spurious detection of (P) or contaminated by (p) a short-term latent image left by a bright source, or
- H,h - Halo. Source may be a spurious detection of (H) or contaminated by (h) the scattered light halo surrounding a nearby bright source, or
- O,o (letter "o") - Optical ghost. Source may be a spurious detection of (O) or contaminated by (o) an optical ghost image caused by a nearby bright source, or
- 0 (number zero) - Source is unaffected by known artifacts.
A source extraction may be affected by more than one type of artifact or condition. In this event, the cc_flags value in each band is set in the following priority order: D,P,H,O,d,p,h,o,0. The full tally of artifacts affecting a source in each band is given in the w?cc_map and w?cc_map_str columns. A source can appear in the AllWISE Source Catalog even if it is flagged as a spurious artifact detection in a band if there is a reliable detection in another band that is not flagged as a spurious artifact detection. Entries in the AllWISE Reject Table may be flagged as spurious detections of artifacts in all bands. |
| cc_flags |
catwise_2020, catwise_prelim |
WISE |
worst case 4 character cc_flag from AllWISE |
varchar |
16 |
|
|
|
| cc_flags |
wise_allskysc |
WISE |
Contamination and confusion flag. Four character strong, one character per band [W1/W2/W3/W4], that indicates that the photometry and/or position measurements of a source may be contaminated or biased due to proximity to an image artifact. CAUTION: Non-zero cc_flags values in any band indicate the the measurement in that band may be contaminated and the photometry should be used with caution. |
char |
4 |
|
|
|
| cc_flags |
wise_prelimsc |
WISE |
Contamination and confusion flag Four character strong, one character per band [W1/W2/W3/W4], that indicates that the photometry and/or position measurements of a source may be contaminated or biased due to proximity to an image artifact |
char |
4 |
|
|
|
| cc_flg |
twomass_psc |
TWOMASS |
Contamination and confusion flag. |
varchar |
3 |
|
|
meta.code |
| cc_flg |
twomass_sixx2_psc |
TWOMASS |
indicates JHK artifact contamination and/or confusion |
varchar |
3 |
|
|
|
| cc_flg |
twomass_sixx2_xsc |
TWOMASS |
indicates artifact contamination and/or confusion |
varchar |
1 |
|
|
|
| cc_flg |
twomass_xsc |
TWOMASS |
indicates artifact contamination and/or confusion. |
varchar |
1 |
|
|
meta.code |
| cd11 |
CurrentAstrometry |
VULCANiDR |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_1} |
float |
8 |
|
-0.9999995e9 |
pos.wcs.cdmatrix |
| cd12 |
CurrentAstrometry |
VULCANiDR |
Element of the linear transformation matrix (with scale) {image extension keyword: CD1_2} |
float |
8 |
|
-0.9999995e9 |
pos.wcs.cdmatrix |
| cd21 |
CurrentAstrometry |
VULCANiDR |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_1} |
float |
8 |
|
-0.9999995e9 |
pos.wcs.cdmatrix |
| cd22 |
CurrentAstrometry |
VULCANiDR |
Element of the linear transformation matrix (with scale) {image extension keyword: CD2_2} |
float |
8 |
|
-0.9999995e9 |
pos.wcs.cdmatrix |
| chi2 |
allSkyNIRSource |
VULCANiDR |
Chi-squared value of proper motion solution |
real |
4 |
|
-0.9999995e9 |
stat.fit.chi2 |
| chi2pmdec |
catwise_2020, catwise_prelim |
WISE |
chi-square for PMRA difference (1 DF) |
real |
4 |
|
|
|
| chi2pmra |
catwise_2020, catwise_prelim |
WISE |
chi-square for PMRA difference (1 DF) |
real |
4 |
|
|
|
| classprob_dsc_combmod_binarystar |
gaia_source |
GAIADR3 |
Overall class probability from DSC of being a binary star |
real |
4 |
|
|
stat.probability |
| classprob_dsc_combmod_galaxy |
gaia_source |
GAIADR3 |
Overall class probability from DSC of being a galaxy |
real |
4 |
|
|
stat.probability |
| classprob_dsc_combmod_quasar |
gaia_source |
GAIADR3 |
Overall class probability from DSC of being a quasar |
real |
4 |
|
|
stat.probability |
| classprob_dsc_combmod_star |
gaia_source |
GAIADR3 |
Overall class probability from DSC of being a single star (but not a white dwarf) |
real |
4 |
|
|
stat.probability |
| classprob_dsc_combmod_whitedwarf |
gaia_source |
GAIADR3 |
Overall class probability from DSC of being a white dwarf |
real |
4 |
|
|
stat.probability |
| clat |
twomass_sixx2_psc, twomass_sixx2_scn |
TWOMASS |
The computed dec (J2000 EQ) of scan center in sexigesimal. |
varchar |
16 |
|
|
|
| clat |
twomass_sixx2_xsc |
TWOMASS |
The computed dec (J2000 EQ) in sexigesimal. |
varchar |
16 |
|
|
|
| cld |
twomass_scn |
TWOMASS |
Special flag indicating whether or not a cloud was found in the scan after comparison of its photometry to that of overlapping scans in the database. |
smallint |
2 |
|
|
meta.code |
| cld |
twomass_sixx2_scn |
TWOMASS |
downgrade from DB photom. overlap comparison (clouds) (0|1) |
smallint |
2 |
|
|
|
| clon |
twomass_sixx2_psc, twomass_sixx2_scn |
TWOMASS |
The computed ra (J2000 EQ) of scan center in sexigesimal. |
varchar |
16 |
|
|
|
| clon |
twomass_sixx2_xsc |
TWOMASS |
The computed ra (J2000 EQ) in sexigesimal. |
varchar |
16 |
|
|
|
| cntr |
allwise_sc |
WISE |
Unique identification number for this object in the AllWISE Catalog/Reject Table. This number is formed from the source_id, which is in turn formed from the coadd_id and source number, src. |
bigint |
8 |
|
|
|
| The cntr value is formed by making the source_id into an integer, in the format: RRRRsDDDtrevIIIIII, where For example, a source in the Tile 3041m137_ac51, with a source_id of '3041m137_ac51-012345', has a cntr value of 3041013701351012345. NOTE: AllWISE Catalog and Reject Table entries are cross-referenced with the Multiepoch Photometry (MEP) Database via the cntr identifier. The Catalog/Reject Table cntr value is referred to as cntr_mf in the MEP Database. |
| cntr |
catwise_2020, catwise_prelim |
WISE |
Unique identifier |
int |
4 |
|
|
|
| cntr |
twomass_sixx2_scn, twomass_sixx2_xsc |
TWOMASS |
entry counter (key) number (unique within table) |
int |
4 |
|
|
|
| cntr |
wise_allskysc |
WISE |
Unique identification number for the Catalog source This number is formed entirely from the source_id, which is in turn formed from the coadd_id and source number src. On average, sources with cntr values close to each other are also close to each other on the sky, except at Tile boundaries. |
bigint |
8 |
|
|
meta.id;meta.main |
| cntr |
wise_prelimsc |
WISE |
Unique identification number for the Catalog source This number is formed entirely from the source_id, which is in turn formed from the coadd_id and source number src. On average, sources with cntr values close to each other are also close to each other on the sky, except at Tile boundaries |
bigint |
8 |
|
|
meta.id;meta.main |
| coadd |
twomass_psc |
TWOMASS |
Sequence number of the Atlas Image in which the position of this source falls. |
smallint |
2 |
|
|
meta.number |
| coadd |
twomass_xsc |
TWOMASS |
3-digit coadd number (unique within scan). |
smallint |
2 |
|
|
meta.number |
| coadd_id |
allwise_sc |
WISE |
Atlas Tile identifier from which source was extracted. |
varchar |
20 |
|
|
|
| The identifier has the general form: RRRRsDDD_[trev], where |
| coadd_id |
wise_allskysc |
WISE |
Atlas Tile identifier from which source was extracted. |
char |
20 |
|
|
|
| coadd_id |
wise_prelimsc |
WISE |
Atlas Tile identifier from which source was extracted |
char |
20 |
|
|
|
| coadd_key |
twomass_psc |
TWOMASS |
Unique identification number of the record in the Atlas Image Data Table (NOT YET AVAILABLE) that corresponds to Image in which the position of this source falls. |
int |
4 |
|
|
meta.id |
| coadd_key |
twomass_xsc |
TWOMASS |
key to coadd data record in "scan DB". |
int |
4 |
|
|
meta.id |
| comment |
ArchiveCurationHistory |
VULCANiDR |
Comment string supplied by the curator |
varchar |
256 |
|
|
?? |
| contam_flg |
twomass_xsc |
TWOMASS |
contamination flag: 0=no stars, 1=stellar flux incl. in mag. |
smallint |
2 |
|
|
meta.code |
| coord1 |
ExternalSurveyTable |
VULCANiDR |
The attribute name of the first (longitudinal) spherical co-ordinate, e.g. equatorial RA |
varchar |
32 |
|
'ra' |
?? |
| coord2 |
ExternalSurveyTable |
VULCANiDR |
The attribute name of the second (latitudinal) spherical co-ordinate, e.g. equatorial Dec |
varchar |
32 |
|
'dec' |
?? |
| crPixX |
CurrentAstrometry |
VULCANiDR |
Pixel coordinate of the reference point on axis 1 {image extension keyword: CRPIX1} |
float |
8 |
pixels |
-0.9999995e9 |
pos.cartesian.x;instr.det |
| crPixY |
CurrentAstrometry |
VULCANiDR |
Pixel coordinate of the reference point on axis 2 {image extension keyword: CRPIX2} |
float |
8 |
pixels |
-0.9999995e9 |
pos.cartesian.y;instr.det |
| crValX |
CurrentAstrometry |
VULCANiDR |
Coordinate value at reference point on axis 1 {image extension keyword: CRVAL1} |
float |
8 |
|
-0.9999995e9 |
pos.cartesian.x;instr.det |
| crValY |
CurrentAstrometry |
VULCANiDR |
Coordinate value at reference point on axis 2 {image extension keyword: CRVAL2} |
float |
8 |
|
-0.9999995e9 |
pos.cartesian.y;instr.det |
| cTypeX |
CurrentAstrometry |
VULCANiDR |
G&C WCS type, eg 'RA---ZPN' {image extension keyword: CTYPE1} |
varchar |
8 |
|
'NONE' |
pos.eq.ra;meta.main |
| cTypeY |
CurrentAstrometry |
VULCANiDR |
G&C WCS type, eg 'DEC--ZPN' {image extension keyword: CTYPE2} |
varchar |
8 |
|
'NONE' |
pos.eq.dec;meta.main |
| cuEventID |
ArchiveCurationHistory, AstrometricInfo, ProgrammeCurationHistory |
VULCANiDR |
UID of curation event giving rise to this record |
int |
4 |
|
|
meta.bib |
| cuEventID |
allSkyNIRFrameSetInfo, allSkyNIRSource |
VULCANiDR |
UID of curation event giving rise to this record |
int |
4 |
|
|
meta.id |
| cuID |
ArchiveCurationHistory, CurationTask |
VULCANiDR |
the unique curation task ID |
smallint |
2 |
|
|
meta.bib |
| curator |
ArchiveCurationHistory |
VULCANiDR |
The archive curation scientist responsible for this event |
varchar |
16 |
|
|
?? |
| cutOff |
Filter |
VULCANiDR |
The 50% cut-off wavelength of the filter |
real |
4 |
microns |
|
?? |
| cutOn |
Filter |
VULCANiDR |
The 50% cut-on wavelength of the filter |
real |
4 |
microns |
|
?? |
| cx |
ObjectThin |
PS1DR2 |
Cartesian x on a unit sphere. |
float |
8 |
|
|
pos.cartesian.x;pos.eq |
| cx |
allSkyNIRFrameSetInfo, allSkyNIRSource |
VULCANiDR |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.x;pos.eq |
| cx |
catwise_2020, catwise_prelim |
WISE |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
| cx |
gaia_source |
GAIADR3 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
| cx |
twomass_psc, twomass_scn, twomass_sixx2_psc, twomass_sixx2_scn, twomass_sixx2_xsc, twomass_xsc |
TWOMASS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
| cx |
wise_allskysc, wise_prelimsc |
WISE |
unit vector of spherical co-ordinates (similar to x in IPAC IRSA schema, but recomputed) |
float |
8 |
|
|
pos.distance;pos.cartesian.x |
| cy |
ObjectThin |
PS1DR2 |
Cartesian y on a unit sphere. |
float |
8 |
|
|
pos.cartesian.y;pos.eq |
| cy |
allSkyNIRFrameSetInfo, allSkyNIRSource |
VULCANiDR |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.y;pos.eq |
| cy |
catwise_2020, catwise_prelim |
WISE |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
| cy |
gaia_source |
GAIADR3 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
| cy |
twomass_psc, twomass_scn, twomass_sixx2_psc, twomass_sixx2_scn, twomass_sixx2_xsc, twomass_xsc |
TWOMASS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
| cy |
wise_allskysc, wise_prelimsc |
WISE |
unit vector of spherical co-ordinates (similar to y in IPAC IRSA schema, but recomputed) |
float |
8 |
|
|
pos.distance;pos.cartesian.y |
| cz |
ObjectThin |
PS1DR2 |
Cartesian z on a unit sphere. |
float |
8 |
|
|
pos.cartesian.y;pos.eq |
| cz |
allSkyNIRFrameSetInfo, allSkyNIRSource |
VULCANiDR |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.cartesian.z;pos.eq |
| cz |
catwise_2020, catwise_prelim |
WISE |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.z |
| cz |
gaia_source |
GAIADR3 |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.z |
| cz |
twomass_psc, twomass_scn, twomass_sixx2_psc, twomass_sixx2_scn, twomass_sixx2_xsc, twomass_xsc |
TWOMASS |
unit vector of spherical co-ordinates |
float |
8 |
|
|
pos.distance;pos.cartesian.z |
| cz |
wise_allskysc, wise_prelimsc |
WISE |
unit vector of spherical co-ordinates (similar to z in IPAC IRSA schema, but recomputed) |
float |
8 |
|
|
pos.distance;pos.cartesian.z |