BARONCHELLI, IVANOIVANOBARONCHELLI0000-0002-0501-8256Rodighiero, G.G.Rodighiero0000-0003-0556-2929Teplitz, H. I.H. I.Teplitz0000-0001-9139-2342Scarlata, C. M.C. M.Scarlata0000-0001-8600-7008Franceschini, A.A.Franceschini0000-0001-9553-8804Berta, S.S.Berta0000-0002-3585-866XBarrufet, L.L.BarrufetVaccari, M.M.VaccariBonato, M.M.BonatoCiesla, L.L.CieslaZanella, A.A.ZanellaCarraro, R.R.CarraroMancini, C.C.ManciniPuglisi, A.A.PuglisiMalkan, M.M.MalkanMei, S.S.MeiMarchetti, L.L.MarchettiColbert, J.J.ColbertSedgwick, C.C.SedgwickSerjeant, S.S.SerjeantPearson, C.C.PearsonRadovich, M.M.RadovichGrado, A.A.GradoLimatola, L.L.LimatolaCovone, G.G.Covone2020-10-052020-10-052018http://hdl.handle.net/20.500.12386/27582The Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole field (SEP) covers an area of 7.74 sq. deg to a depth of ~5.80 microJy (3sigma) at 3.6 microns and 5.25 microJy at 4.5 microns. The 90% and 50% completeness limits are at 14 and 9 microJy, respectively. The multiwavelength catalog includes the WFI-Rc, MIPS-24 micron, SPIRE 250, 350 and 500 micron fluxes of the counterparts that were identified by searching for the closest neighbor. <P />The indicator P quantifies the reliability of each association (example, for P1: SPIRE to MIPS) considering both the distance between the SPIRE source and the closest MIPS association and the presence of further possible MIPS associations in the MIPS-SPIRE searching radius. <P />For bands other than IRAC 3.6 microns, a null flux means no coverage in that band, while a flux of zero means that the position is covered in that band but the source is not detected. <P />(1 data file).enDatabase10.26093/cds/vizier.18570064https://cdsarc.unistra.fr/viz-bin/cat/J/ApJ/857/642018yCat..18570064BFIS/05 - ASTRONOMIA E ASTROFISICA