E |
| Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
| e_score |
twomass_xsc |
TWOMASS |
extended score: 1(extended) < e_score < 2(point-like). |
real |
4 |
|
|
meta.code |
| ebpminrp_gspphot |
gaia_source |
GAIADR3 |
Reddening E(BP-RP) from GSP-Phot Aeneas best library using BP/RP spectra |
real |
4 |
mag |
|
phot.color.excess |
| ebpminrp_gspphot_lower |
gaia_source |
GAIADR3 |
Lower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas best library using BP/RP spectra |
real |
4 |
mag |
|
phot.color.excess;stat.min |
| ebpminrp_gspphot_upper |
gaia_source |
GAIADR3 |
Upper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas best library using BP/RP spectra |
real |
4 |
mag |
|
phot.color.excess;stat.max |
| eBV |
allSkyNIRSource |
VULCANiDR |
The galactic dust extinction value measured from the Schlegel, Finkbeiner & Davis (1998) maps. This uses the correction given in Bonifacio, Monai & Beers (2000). This correction reduces the extinction value in regions of high extinction (E(B-V)>0.1) |
real |
4 |
|
-0.9999995e9 |
phys.absorption.gal |
| ecl_lat |
gaia_source |
GAIADR3 |
Ecliptic latitude |
float |
8 |
degrees |
|
pos.ecliptic.lat |
| ecl_lon |
gaia_source |
GAIADR3 |
Ecliptic longitude |
float |
8 |
degrees |
|
pos.ecliptic.lon |
| elat |
allwise_sc |
WISE |
Ecliptic latitude computed from the non-moving source fit equatorial position. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
deg |
|
|
| elat |
catwise_2020, catwise_prelim |
WISE |
ecliptic latitude |
float |
8 |
deg |
|
|
| elat |
wise_allskysc |
WISE |
Ecliptic latitude. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
degrees |
|
|
| elat |
wise_prelimsc |
WISE |
Ecliptic latitude. CAUTION: This coordinate should not be used as an astrometric reference |
float |
8 |
degrees |
|
|
| elat_avg |
catwise_2020, catwise_prelim |
WISE |
averaged ecliptic latitude |
float |
8 |
deg |
|
|
| elatSig |
catwise_2020, catwise_prelim |
WISE |
one-sigma uncertainty in elat |
real |
4 |
arcsec |
|
|
| ellfit_flg |
twomass_xsc |
TWOMASS |
ellipse fitting contamination flag. |
smallint |
2 |
|
|
meta.code |
| elon |
allwise_sc |
WISE |
Ecliptic longitude computed from the non-moving source fit equatorial position. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
deg |
|
|
| elon |
catwise_2020, catwise_prelim |
WISE |
ecliptic longitude |
float |
8 |
deg |
|
|
| elon |
wise_allskysc |
WISE |
Ecliptic longitude. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
degrees |
|
|
| elon |
wise_prelimsc |
WISE |
Ecliptic longitude. CAUTION: This coordinate should not be used as an astrometric reference |
float |
8 |
degrees |
|
|
| elon_avg |
catwise_2020, catwise_prelim |
WISE |
averaged ecliptic longitude |
float |
8 |
deg |
|
|
| elonSig |
catwise_2020, catwise_prelim |
WISE |
one-sigma uncertainty in elon |
real |
4 |
arcsec |
|
|
| epoch |
allSkyNIRSource |
VULCANiDR |
Epoch of position measurement |
float |
8 |
Years |
|
time.epoch |
| epochMean |
ObjectThin |
PS1DR2 |
Modified Julian Date of the mean epoch corresponding to raMean, decMean (equinox J2000). Note that Gaia DR1 data is sometimes included in the mean position; in those cases, the epochMean value is near the Gaia DR1 epoch 2015.5 = MJD 15023. As a result, epochMean is not necessarily near the mean value of the PS1 measurement dates. |
float |
8 |
days |
-999 |
|
| err_ang |
twomass_psc |
TWOMASS |
Position angle on the sky of the semi-major axis of the position uncertainty ellipse (East of North) |
smallint |
2 |
degrees |
|
pos.posAng |
| err_ang |
twomass_sixx2_psc |
TWOMASS |
angle of error ellipse major axis (E of N) |
smallint |
2 |
deg |
|
|
| err_maj |
twomass_psc |
TWOMASS |
Semi-major axis length of the one sigma position uncertainty ellipse |
real |
4 |
arcsec |
|
phys.angSize;src |
| err_maj |
twomass_sixx2_psc |
TWOMASS |
major axis of 1-sigma error ellipse |
real |
4 |
arcsec |
|
|
| err_min |
twomass_psc |
TWOMASS |
Semi-minor axis length of the one sigma position uncertainty ellipse |
real |
4 |
arcsec |
|
phys.angSize;src |
| err_min |
twomass_sixx2_psc |
TWOMASS |
minor axis of 1-sigma error ellipse |
real |
4 |
arcsec |
|
|
| expTime |
Detection |
PS1DR2 |
Exposure time of the frame/exposure. Necessary for converting listed fluxes and magnitudes back to measured ADU counts. |
real |
4 |
seconds |
-999 |
|
| ext_flg |
allwise_sc |
WISE |
Extended source flag. This is an integer flag, the value of which indicates whether or not the morphology of a source is consistent with the WISE point spread function in any band, or whether the source is associated with or superimposed on a previously known extended object from the 2MASS Extended Source Catalog (XSC). CAUTION: WISE profile-fit (w?mpro) and standard aperture (w?mag) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. If a source entry has ext_flg>0, you may wish to examine the large aperture photometry, or the elliptical aperture photometry which are measured using areas that are scaled from 2MASS XSC morphologies. |
int |
4 |
|
|
|
The values of the ext_flg indicate the following conditions: - 0 - The source shape is consistent with a point-source and the source is not associated with or superimposed on a 2MASS XSC source
- 1 - The profile-fit photometry goodness-of-fit, w?rchi2, is >3.0 in one or more bands.
- 2 - The source falls within the extrapolated isophotal footprint of a 2MASS XSC source.
- 3 - The profile-fit photometry goodness-of-fit,w?rchi2, is >3.0 in one or more bands, and the source falls within the extrapolated isophotal footprint of a 2MASS XSC source.
- 4 - The source position falls within 5" of a 2MASS XSC source.
- 5 - The profile-fit photometry goodness-of-fit,w?rchi2, is >3.0 in one or more bands, and the source position falls within 5" of a 2MASS XSC source.
|
| ext_flg |
wise_allskysc |
WISE |
Extended source flag. This flag indicates whether or not the morphology of a source is consistent with the WISE point spread function in any band or whether the source is associated with or superimposed on a previously known extended object from the 2MASS Extended Source Catalog (XSC): 0 - The source shape is consistent with a point-source; 1 - The source shape is not consistent with a point-source; 2 - The source falls within the extrapolated isophotal footprint of a 2MASS XSC source; 3 - The profile-fit photometry goodness-of-fit, w?rchi2, is >3.0 in one or more bands, and The source falls within the extrapolated isophotal footprint of a 2MASS XSC source; 4 - The source position falls within 5" of a 2MASS XSC source; 5 - The profile-fit photometry goodness-of-fit, w?rchi2, is >3.0 in one or more bands, and the source position falls within 5" of a 2MASS XSC source. CAUTION: WISE profile-fit (w?mpro) and standard aperture (w?mag) measurements are optimized for point sources and will systematically underestimate the true flux of resolved objects. |
tinyint |
1 |
|
|
|
| ext_flg |
wise_prelimsc |
WISE |
Extended source flag This flag indicates whether or not the morphology of a source is consistent with the WISE point spread function in any band: 0 - The source shape is consistent with a point-source; 1 - The source shape is not consistent with a point-source |
tinyint |
1 |
|
|
|
| ext_key |
twomass_psc |
TWOMASS |
Unique identification number of the record in the XSC that corresponds to this point source. |
int |
4 |
|
|
meta.id |
| ext_key |
twomass_xsc |
TWOMASS |
entry counter (key) number (unique within table). |
int |
4 |
|
|
meta.id |
| extinctionMapList |
Programme |
VULCANiDR |
A list of 3D extinction maps that should be matched to this survey |
varchar |
32 |
|
NONE |
meta.id |
| extNSigma |
Detection |
PS1DR2 |
An extendedness measure based on the deviation between PSF and Kron (1980) magnitudes, normalized by the PSF magnitude uncertainty. |
real |
4 |
|
0 |
|
| extNum |
AstrometricInfo |
VULCANiDR |
the extension number of this frame |
tinyint |
1 |
|
|
meta.number |
| extNum |
CurrentAstrometry, MultiframeDetector |
VULCANiDR |
the extension number of this frame |
tinyint |
1 |
|
0 |
meta.number |
| extProgID |
RequiredNeighbours |
VULCANiDR |
the unique programme ID for second table if there are multiple programmes in the neighbour survey |
int |
4 |
|
-99999999 |
meta.id |
| extractor |
allSkyNIRFrameSetInfo |
VULCANiDR |
Extractor used, CASU/SEX |
varchar |
4 |
|
|
|
| extTableID |
ExternalSurveyTable, RequiredNeighbours |
VULCANiDR |
the unique table ID |
int |
4 |
|
|
meta.id;meta.main |
| extTableName |
ExternalSurveyTable |
VULCANiDR |
the name of the table |
varchar |
256 |
|
|
meta.id;meta.dataset |