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TABLE  wiseForcedTarget

WISE forced-photometry of SDSS primary sources.
This table contains one entry for each SDSS primary object. See http://arxiv.org/abs/1410.7397 for the method.

nametypelengthunitucddescription
objIDbigint8  Unique SDSS identifier composed from [skyVersion,rerun,run,camcol,field,obj].
rafloat8deg SDSS right ascension, J2000
decfloat8deg SDSS declination, J2000
has_wise_photbit1  Does WISE forced photometry exist for this source?
xreal4  FITS pixel coordinate in the unWISE tile
yreal4  FITS pixel coordinate in the unWISE tile
treated_as_pointsourcebit1  Was this source treated as a point source for photometry purposes?
coadd_idchar8  unWISE tile identification, RRRR[pm]DDD, RRRR = int(10 * RA), DDD = int(10 * Dec), [pm] = sign(Dec), eg 2052p620
w1_nanomaggiesreal4Vega mag W1 flux. Fluxes are presented in the Vega system, NOT AB. 1 nmgy means Vega mag 22.5
w1_nanomaggies_ivarreal41/(Vega mag)^2 Inverse-variance uncertainty for w1_nanomaggies
w1_magreal4Vega mag W1 magnitude. w1_nanomaggies converted to (Vega) magnitudes.
w1_mag_errreal4Vega mag W1 magnitude uncertainty
w1_prochi2real4  Profile-weighted chi-squared (goodness of fit)
w1_pronpixreal4  Profile-weighted number of WISE exposures in coadd
w1_profracfluxreal4  Profile-weighted fraction of flux coming from other sources; blendedness measure.
w1_profluxreal4  Profile-weighted flux coming from other sources
w1_npixreal4  Number of pixels used in fit
w2_nanomaggiesreal4Vega mag W2 flux. Fluxes are presented in the Vega system, NOT AB. 1 nmgy means Vega mag 22.5
w2_nanomaggies_ivarreal41/(Vega mag)^2 Inverse-variance uncertainty for w2_nanomaggies
w2_magreal4Vega mag W2 magnitude. w2_nanomaggies converted to (Vega) magnitudes.
w2_mag_errreal4Vega mag W2 magnitude uncertainty
w2_prochi2real4  Profile-weighted chi-squared (goodness of fit)
w2_pronpixreal4  Profile-weighted number of WISE exposures in coadd
w2_profracfluxreal4  Profile-weighted fraction of flux coming from other sources; blendedness measure.
w2_profluxreal4  Profile-weighted flux coming from other sources
w2_npixreal4  Number of pixels used in fit