Photometric redshifts in Stripe 82 2017-11-18T01:02:03 1000 This is a catalogue of photometric redshifts of galaxies in the Stripe 82 obtained when morphology (galaxy size, ellipticity, Sérsic index, and surface brightness) are included in training on galaxy samples from the SDSS and the CFHT Stripe-82 Survey (CS82). Our redshifts yield a 68th percentile error of 0.058(1 + z), and a outlier fraction of 5.2 per cent. Soo, John Y H; Moraes, Bruno; Joachimi, Benjamin; Hartley, William; Lahav, Ofer; Charbonnier, Aldée; Makler, Martín; Pereira, Maria E S; Comparat, Johan; Erben, Thomas; Leauthaud, Alexie; Shan, Huanyuan; Van Waerbeke, Ludovic The distributions :math:`P(z)` used to estimate z_phot and z_morph are available as FITS binary tables from `pz_phot`_ (1.4 GB) and `pz_morph`_ (0.8 GB), respectively. .. _pz_phot: /\schema/q/cone/static/cs82_pz_morph.fits.gz .. _pz_morph: /\schema/q/cone/static/cs82_pz_phot.fits.gz The data in the \schema.main table is also available as a FITS binary table: `phz.fits`_ (0.7 GB). .. _phz.fits: /\schema/q/cone/static/cs82_phz.fits.gz redshift-surveys broad-band-photometry galaxy-distances galaxy-structure Optical 2018MNRAS.475.3613S band, ucd u, em.opt.U g, em.opt.V r, em.opt.R i, em.opt.I z, em.opt.I CS82 cone 317.7168 -0.9739 0.001 data cone/scs.xml row = self.getFirstVOTableRow() self.assertEqual(row["objid_cs82"], '76059981') self.assertAlmostEqual(row['spread_model_ser'], 0.012096334248781204) cone/form 68124213<", # Matched object ">14.4<", # lensFit, formatted ">21.265<", # kron i ">19.8<" # surface brightness ) ]]>