Lehmer, B. D.B. D.Lehmer0000-0003-3096-9966Basu-Zych, A. R.A. R.Basu-ZychMineo, S.S.MineoBrandt, W. N.W. N.BrandtEufrasio, R. T.R. T.EufrasioFragos, T.T.FragosHornschemeier, A. E.A. E.HornschemeierLuo, B.B.LuoXue, Y. Q.Y. Q.XueBauer, F. E.F. E.BauerGilfanov, M.M.GilfanovRanalli, P.P.RanalliSchneider, D. P.D. P.SchneiderShemmer, O.O.ShemmerTOZZI, PaoloPaoloTOZZITrump, J. R.J. R.TrumpVignali, C.C.VignaliWang, J. -X.J. -X.WangYukita, M.M.YukitaZezas, A.A.Zezas2020-05-062020-05-062016http://hdl.handle.net/20.500.12386/24544We began with an initial sample of 32508 galaxies in the Great Observatories Origins Deep Survey South (GOODS-S) footprint as presented in Section 2 of Xue et al. (2012, J/ApJ/758/129). We cut our initial sample to the 24941 objects that were within 7' of the mean ~6Ms CDF-S aimpoint, a region where the Chandra point-spread function (PSF) is sharpest and the corresponding X-ray sensitivity is highest. See text for further explanations.enDatabasehttp://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/ApJ/825/72016yCat..18250007LFIS/05 - ASTRONOMIA E ASTROFISICAScienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation