Contains the parameters provided for each source in the CatWISE 2020 source catalogue. |
This table contains the parameters provided for each source in the CatWISE 2020 Source Catalogue. The CatWISE2020 Catalog consists of 1,890,715,640 sources over the entire sky selected from WISE and NEOWISE survey data at 3.4 and 4.6 microns (W1 and W2) collected from 2010 Jan. 7 to 2018 Dec. 13. This dataset includes six times as many exposures and spans over sixteen times as large a time baseline as the AllWISE catalog. CatWISE adapts AllWISE software to measure the sources in co-added images created from six-month subsets of these data, each representing one coverage of the inertial sky, or epoch. CatWISE2020 includes the measured motion of sources over the 8 year span of the data, typically in 12 epochs. The scatter with respect to Spitzer photometry at faint magnitudes in fields out of the Galactic plane and at low ecliptic latitude (corresponding to lower WISE coverage depth) is similar to that for the CatWISE Preliminary Catalog, reaching 0.217 mag (equivalent to SNR 5) at approximately W1=17.7 and W2=16.5, vs. W1=16.9 and W2=15.9 for AllWISE. The 90% completeness depth for CatWISE2020 is at roughly W1=17.7 and W2=17.3, about 1.7 mag deeper than in the Preliminary Catalog. From comparison to Gaia, the motions are over a dozen times more accurate than those from AllWISE. Required constraints:
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Name | Type | Length | Unit | Description | Default Value | Unified Content Descriptor |
---|---|---|---|---|---|---|
source_name | varchar | 21 | source hexagesimal designation | |||
source_id | varchar | 25 | tile name + processing code + wphot index | |||
ra | float | 8 | deg | right ascension (ICRS) | ||
dec | float | 8 | deg | declination (ICRS) | ||
sigra | real | 4 | arcsec | uncertainty in ra (arcsec) | ||
sigdec | real | 4 | arcsec | uncertainty in dec (arcsec) | ||
sigradec | real | 4 | arcsec | uncertainty cross-term (arcsec) | ||
wx | real | 4 | pix | x-pixel coordinate | ||
wy | real | 4 | pix | y-pixel coordinate | ||
w1sky | real | 4 | dn | frame sky background value, band-1 | ||
w1sigsk | real | 4 | dn | frame sky background value uncertainty, band-1 | ||
w1conf | real | 4 | dn | frame sky confusion based on the UNC images | ||
w2sky | real | 4 | dn | frame sky background value, band-2 | ||
w2sigsk | real | 4 | dn | frame sky background value uncertainty, band-2 | ||
w2conf | real | 4 | dn | frame sky confusion based on the UNC images | ||
w1fitr | real | 4 | asec | fitting radius, band-1 (clipped at 999.99) | ||
w2fitr | real | 4 | asec | fitting radius, band-2 (clipped at 999.99) | ||
w1snr | real | 4 | S/N ratio, band-1 | |||
w2snr | real | 4 | S/N ratio, band-2 | |||
w1flux | real | 4 | dn | WPRO raw flux, band-1 | ||
w1sigflux | real | 4 | dn | WPRO raw flux uncertainty, band-1 | ||
w2flux | real | 4 | dn | WPRO raw flux, band-2 | ||
w2sigflux | real | 4 | dn | WPRO raw flux uncertainty, band-2 | ||
w1mpro | real | 4 | mag | WPRO flux in mag units, band-1 | ||
w1sigmpro | real | 4 | mag | WPRO flux uncertainty in mag units, band-1 | ||
w1rchi2 | real | 4 | WPRO reduced chi^2, band-1 | |||
w2mpro | real | 4 | mag | WPRO flux in mag units, band-2 | ||
w2sigmpro | real | 4 | mag | WPRO flux uncertainty in mag units, band-2 | ||
w2rchi2 | real | 4 | WPRO reduced chi^2, band-2 | |||
rchi2 | real | 4 | reduced chi squared, total | |||
nb | int | 4 | number of blend components used in each fit | |||
na | int | 4 | number of actively deblended components | |||
w1Sat | real | 4 | fraction of pixels saturated, band-1 | |||
w2Sat | real | 4 | fraction of pixels saturated, band-2 | |||
w1mag | real | 4 | mag | standard aperture mag w/ correction applied | ||
w1sigm | real | 4 | mag | standard aperture mag uncertainty, band-1 | ||
w1flg | int | 4 | standard aperture flag, band-1 | |||
w1Cov | real | 4 | mean coverage depth, band-1 | |||
w2mag | real | 4 | mag | standard aperture mag w/ correction applied | ||
w2sigm | real | 4 | mag | standard aperture mag uncertainty, band-2 | ||
w2flg | int | 4 | standard aperture flag, band-2 | |||
w2Cov | real | 4 | mean coverage depth, band-2 | |||
w1mag_1 | real | 4 | mag | Aper 1 (5.50 arcsec), aperture mag, band-1 | ||
w1sigm_1 | real | 4 | mag | Aper 1 (5.50 arcsec), aperture mag uncertainty, band-1 | ||
w1flg_1 | int | 4 | Aper 1 (5.50 arcsec), aperture flag, band-1 | |||
w2mag_1 | real | 4 | mag | Aper 1 (5.50 arcsec), aperture mag, band-2 | ||
w2sigm_1 | real | 4 | mag | Aper 1 (5.50 arcsec), aperture mag uncertainty, band-2 | ||
w2flg_1 | int | 4 | Aper 1 (5.50 arcsec), aperture flag, band-2 | |||
w1mag_2 | real | 4 | mag | Aper 2 (8.25 arcsec), aperture mag, band-1 | ||
w1sigm_2 | real | 4 | mag | Aper 2 (8.25 arcsec), aperture mag uncertainty, band-1 | ||
w1flg_2 | int | 4 | Aper 2 (8.25 arcsec), aperture flag, band-1 | |||
w2mag_2 | real | 4 | mag | Aper 2 (8.25 arcsec), aperture mag, band-2 | ||
w2sigm_2 | real | 4 | mag | Aper 2 (8.25 arcsec), aperture mag uncertainty, band-2 | ||
w2flg_2 | int | 4 | Aper 2 (8.25 arcsec), aperture flag, band-2 | |||
w1mag_3 | real | 4 | mag | Aper 3 (11.00 arcsec), aperture mag, band-1 | ||
w1sigm_3 | real | 4 | mag | Aper 3 (11.00 arcsec), aperture mag uncertainty, band-1 | ||
w1flg_3 | int | 4 | Aper 3 (11.00 arcsec), aperture flag, band-1 | |||
w2mag_3 | real | 4 | mag | Aper 3 (11.00 arcsec), aperture mag, band-2 | ||
w2sigm_3 | real | 4 | mag | Aper 3 (11.00 arcsec), aperture mag uncertainty, band-2 | ||
w2flg_3 | int | 4 | Aper 3 (11.00 arcsec), aperture flag, band-2 | |||
w1mag_4 | real | 4 | mag | Aper 4 (13.75 arcsec), aperture mag, band-1 | ||
w1sigm_4 | real | 4 | mag | Aper 4 (13.75 arcsec), aperture mag uncertainty, band-1 | ||
w1flg_4 | int | 4 | Aper 4 (13.75 arcsec), aperture flag, band-1 | |||
w2mag_4 | real | 4 | mag | Aper 4 (13.75 arcsec), aperture mag, band-2 | ||
w2sigm_4 | real | 4 | mag | Aper 4 (13.75 arcsec), aperture mag uncertainty, band-2 | ||
w2flg_4 | int | 4 | Aper 4 (13.75 arcsec), aperture flag, band-2 | |||
w1mag_5 | real | 4 | mag | Aper 5 (16.50 arcsec), aperture mag, band-1 | ||
w1sigm_5 | real | 4 | mag | Aper 5 (16.50 arcsec), aperture mag uncertainty, band-1 | ||
w1flg_5 | int | 4 | Aper 5 (16.50 arcsec), aperture flag, band-1 | |||
w2mag_5 | real | 4 | mag | Aper 5 (16.50 arcsec), aperture mag, band-2 | ||
w2sigm_5 | real | 4 | mag | Aper 5 (16.50 arcsec), aperture mag uncertainty, band-2 | ||
w2flg_5 | int | 4 | Aper 5 (16.50 arcsec), aperture flag, band-2 | |||
w1mag_6 | real | 4 | mag | Aper 6 (19.25 arcsec), aperture mag, band-1 | ||
w1sigm_6 | real | 4 | mag | Aper 6 (19.25 arcsec), aperture mag uncertainty, band-1 | ||
w1flg_6 | int | 4 | Aper 6 (19.25 arcsec), aperture flag, band-1 | |||
w2mag_6 | real | 4 | mag | Aper 6 (19.25 arcsec), aperture mag, band-2 | ||
w2sigm_6 | real | 4 | mag | Aper 6 (19.25 arcsec), aperture mag uncertainty, band-2 | ||
w2flg_6 | int | 4 | Aper 6 (19.25 arcsec), aperture flag, band-2 | |||
w1mag_7 | real | 4 | mag | Aper 7 (22.00 arcsec), aperture mag, band-1 | ||
w1sigm_7 | real | 4 | mag | Aper 7 (22.00 arcsec), aperture mag uncertainty, band-1 | ||
w1flg_7 | int | 4 | Aper 7 (22.00 arcsec), aperture flag, band-1 | |||
w2mag_7 | real | 4 | mag | Aper 7 (22.00 arcsec), aperture mag, band-2 | ||
w2sigm_7 | real | 4 | mag | Aper 7 (22.00 arcsec), aperture mag uncertainty, band-2 | ||
w2flg_7 | int | 4 | Aper 7 (22.00 arcsec), aperture flag, band-2 | |||
w1mag_8 | real | 4 | mag | Aper 8 (24.75 arcsec), aperture mag, band-1 | ||
w1sigm_8 | real | 4 | mag | Aper 8 (24.75 arcsec), aperture mag uncertainty, band-1 | ||
w1flg_8 | int | 4 | Aper 8 (24.75 arcsec), aperture flag, band-1 | |||
w2mag_8 | real | 4 | mag | Aper 8 (24.75 arcsec), aperture mag, band-2 | ||
w2sigm_8 | real | 4 | mag | Aper 8 (24.75 arcsec), aperture mag uncertainty, band-2 | ||
w2flg_8 | int | 4 | Aper 8 (24.75 arcsec), aperture flag, band-2 | |||
w1NM | int | 4 | WPRO, N (of M), band-1 | |||
w1M | int | 4 | WPRO, M , band-1 | |||
w1magP | real | 4 | mag | WPRO repeatability mag; band-1 | ||
w1sigP1 | real | 4 | mag | WPRO mag population sigma; band-1 | ||
w1sigP2 | real | 4 | mag | WPRO mag uncertainty of the mean; band-1 | ||
w1k | real | 4 | Stetson k index for variability; band-1 | |||
w1Ndf | int | 4 | No. degrees of freedom in var chi-square; band-1 | |||
w1mLQ | real | 4 | -log(Q), Q = 1-P(chi-square); band-1 | |||
w1mJDmin | float | 8 | minimum mJD; band-1 | |||
w1mJDmax | float | 8 | maximum mJD; band-1 | |||
w1mJDmea | float | 8 | mean mJD; band-1 | |||
w2NM | int | 4 | WPRO, N (of M), band-2 | |||
w2M | int | 4 | WPRO, M , band-2 | |||
w2magP | real | 4 | mag | WPRO repeatability mag; band-2 | ||
w2sigP1 | real | 4 | mag | WPRO mag population sigma; band-2 | ||
w2sigP2 | real | 4 | mag | WPRO mag uncertainty of the mean; band-2 | ||
w2k | real | 4 | Stetson k index for variability; band-2 | |||
w2Ndf | int | 4 | No. degrees of freedom in var chi-square; band-2 | |||
w2mLQ | real | 4 | -log(Q), Q = 1-P(chi-square); band-2 | |||
w2mJDmin | float | 8 | minimum mJD; band-2 | |||
w2mJDmax | float | 8 | maximum mJD; band-2 | |||
w2mJDmean | float | 8 | mean mJD; band-2 | |||
rho12 | int | 4 | % | W1W2 correlation coefficient | ||
q12 | int | 4 | -log10(1-P(rho12)) given no real correlation | |||
nIters | int | 4 | number of chi-square-minimization iterations | |||
nSteps | int | 4 | number of steps in all iterations | |||
mdetID | int | 4 | source ID in mdet list | |||
p1 | real | 4 | arcsec | P vector component 1 | ||
p2 | real | 4 | arcsec | P vector component 2 | ||
MeanObsMJD | float | 8 | MJD | mean observation epoch | ||
ra_pm | float | 8 | deg | right ascension (J2000) | ||
dec_pm | float | 8 | deg | declination (J2000) | ||
sigra_pm | real | 4 | arcsec | uncertainty in ra_pm | ||
sigdec_pm | real | 4 | arcsec | uncertainty in dec_pm | ||
sigradec_pm | real | 4 | arcsec | uncertainty cross-term | ||
PMRA | real | 4 | arcsec/yr | motion in ra | ||
PMDec | real | 4 | arcsec/yr | proper motion in dec | ||
sigPMRA | real | 4 | arcsec/yr | uncertainty in PMRA | ||
sigPMDec | real | 4 | arcsec/yr | uncertainty in PMDec | ||
w1snr_pm | real | 4 | flux S/N ratio, band-1 | |||
w2snr_pm | real | 4 | flux S/N ratio, band-2 | |||
w1flux_pm | real | 4 | dn | WPRO raw flux, band-1 | ||
w1sigflux_pm | real | 4 | dn | WPRO raw flux uncertainty, band-1 | ||
w2flux_pm | real | 4 | dn | WPRO raw flux, band-2 | ||
w2sigflux_pm | real | 4 | dn | fit WPRO raw flux uncertainty, band-2 | ||
w1mpro_pm | real | 4 | mag | WPRO flux in mag units, band-1 | ||
w1sigmpro_pm | real | 4 | mag | WPRO flux uncertainty in mag units, band-1 | ||
w1rchi2_pm | real | 4 | WPRO reduced chi^2, band-1 | |||
w2mpro_pm | real | 4 | mag | WPRO flux in mag units, band-2 | ||
w2sigmpro_pm | real | 4 | mag | WPRO flux uncertainty in mag units, band-2 | ||
w2rchi2_pm | real | 4 | WPRO reduced chi^2, band-2 | |||
rchi2_pm | real | 4 | reduced chi squared, total | |||
pmcode | varchar | 5 | quality of the PM solution | |||
nIters_pm | int | 4 | number of chi-square-minimization iterations | |||
nSteps_pm | int | 4 | number of steps in all iterations | |||
dist | real | 4 | arcsec | radial distance between apparitions | ||
dw1mag | real | 4 | mag | w1mpro difference | ||
rch2w1 | real | 4 | chi-square for dw1mag (1 DF) | |||
dw2mag | real | 4 | mag | w2mpro difference | ||
rch2w2 | real | 4 | chi-square for dw2mag (1 DF) | |||
elon_avg | float | 8 | deg | averaged ecliptic longitude | ||
elonSig | real | 4 | arcsec | one-sigma uncertainty in elon | ||
elat_avg | float | 8 | deg | averaged ecliptic latitude | ||
elatSig | real | 4 | arcsec | one-sigma uncertainty in elat | ||
Delon | real | 4 | arcsec | desc-asce ecliptic longitude | ||
DelonSig | real | 4 | arcsec | one-sigma uncertainty in Delon | ||
Delat | real | 4 | arcsec | desc-asce ecliptic latitude | ||
DelatSig | real | 4 | arcsec | one-sigma uncertainty in Delat | ||
DelonSNR | real | 4 | |Delon|/DelonSig | |||
DelatSNR | real | 4 | |Delat|/DelatSig | |||
chi2pmra | real | 4 | chi-square for PMRA difference (1 DF) | |||
chi2pmdec | real | 4 | chi-square for PMRA difference (1 DF) | |||
ka | int | 4 | astrometry usage code (0: neither the ascending nor the descending scan provided a solution; 1: only the ascending scan provided a solution; 2: only the descending scan provided a solution; 3: both scans provided solutions which were combined in the relevant way) | |||
k1 | int | 4 | W1 photometry usage code (0: neither the ascending nor the descending scan provided a solution; 1: only the ascending scan provided a solution; 2: only the descending scan provided a solution; 3: both scans provided solutions which were combined in the relevant way) | |||
k2 | int | 4 | W2 photometry usage code (0: neither the ascending nor the descending scan provided a solution; 1: only the ascending scan provided a solution; 2: only the descending scan provided a solution; 3: both scans provided solutions which were combined in the relevant way) | |||
km | int | 4 | proper motion usage code (0: neither the ascending nor the descending scan provided a solution; 1: only the ascending scan provided a solution; 2: only the descending scan provided a solution; 3: both scans provided solutions which were combined in the relevant way) | |||
par_pm | real | 4 | arcsec | parallax from PM desc-asce elon | ||
par_pmSig | real | 4 | arcsec | one-sigma uncertainty in par_pm | ||
par_stat | real | 4 | arcsec | parallax estimate from stationary solution | ||
par_sigma | real | 4 | arcsec | one-sigma uncertainty in par_stat | ||
dist_x | real | 4 | arcsec | distance between CatWISE and AllWISE source | ||
cc_flags | varchar | 16 | worst case 4 character cc_flag from AllWISE | |||
w1cc_map | int | 4 | worst case w1cc_map from AllWISE | |||
w1cc_map_str | varchar | 20 | worst case w1cc_map_str from AllWISE | |||
w2cc_map | int | 4 | worst case w2cc_map from AllWISE | |||
w2cc_map_str | varchar | 20 | worst case w2cc_map_str from AllWISE | |||
n_aw | int | 4 | number of AllWISE matches within 2.75 asec | |||
ab_flags | varchar | 9 | Two character (W1 W2) artifact flag | |||
w1ab_map | int | 4 | w1 artifact code value | |||
w1ab_map_str | varchar | 13 | w1 artifact string | |||
w2ab_map | int | 4 | w2 artifact code value | |||
w2ab_map_str | varchar | 13 | w2 artifact string | |||
glon | float | 8 | deg | galactic longitude | ||
glat | float | 8 | deg | galactic latitude | ||
elon | float | 8 | deg | ecliptic longitude | ||
elat | float | 8 | deg | ecliptic latitude | ||
unwise_objid | varchar | 20 | unWISE catalog object ID | |||
cx | float | 8 | unit vector of spherical co-ordinates | pos.distance;pos.cartesian.x | ||
cy | float | 8 | unit vector of spherical co-ordinates | pos.distance;pos.cartesian.y | ||
cz | float | 8 | unit vector of spherical co-ordinates | pos.distance;pos.cartesian.z | ||
htmID | bigint | 8 | Level 20 Hierarchical Triangular Mesh (HTM) index for equatorial co-ordinates | pos.eq | ||
cntr | int | 4 | Unique identifier | |||
Total length | 974 |