Duncan, K. J.K. J.Duncan0000-0001-9139-2342Kondapally, R.R.Kondapally0000-0002-9553-7999Brown, M. J. I.M. J. I.Brown0000-0001-9680-7092BONATO, MATTEOMATTEOBONATOBest, P. N.P. N.BestRoettgering, H. J. A.H. J. A.RoettgeringBONDI, MARCOMARCOBONDIBowler, R. A. A.R. A. A.BowlerCochrane, R. K.R. K.CochraneGuerkan, G.G.GuerkanHardcastle, M. J.M. J.HardcastleJarvis, M. J.M. J.JarvisKunert-Bajraszewska, M.M.Kunert-BajraszewskaLeslie, S. K.S. K.LeslieMalek, K.K.MalekMorabito, L. K.L. K.MorabitoO'Sullivan, S. P.S. P.O'SullivanPRANDONI, ISABELLAISABELLAPRANDONISabater, J.J.SabaterShimwell, T. W.T. W.ShimwellSmith, D. J. B.D. J. B.SmithWang, L.L.WangWolowska, A.A.Wolowska2022-02-252022-02-252020http://hdl.handle.net/20.500.12386/31495Photometric redshifts are calculated using the optical photometry catalogs presented in Kondapally et al. (Paper III. 2020, in prep.), using a hybrid template + machine learning approach. Stellar masses assume a Chabrier (2003PASP..115..763C) initial mass function. Values presented have not been corrected to total fluxes/magnitudes. <P />(3 data files).enDatabase10.26093/cds/vizier.36480004http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/648/A42020yCat..36480004DFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering