Shu, X. W.X. W.ShuElbaz, D.D.ElbazBourne, N.N.BourneSchreiber, C.C.SchreiberWang, T.T.WangDunlop, J. S.J. S.DunlopFONTANA, AdrianoAdrianoFONTANALeiton, R.R.LeitonPannella, M.M.PannellaOkumura, K.K.OkumuraMichałowski, M. J.M. J.MichałowskiSANTINI, PaolaPaolaSANTINIMERLIN, EmilianoEmilianoMERLINBuitrago, F.F.BuitragoBruce, V. A.V. A.BruceAmorin, R.R.AmorinCASTELLANO, MARCOMARCOCASTELLANODerriere, S.S.DerriereCOMASTRI, AndreaAndreaCOMASTRICappelluti, N.N.CappellutiWang, J. X.J. X.WangFerguson, H. C.H. C.Ferguson2020-07-062020-07-0620160067-0049http://hdl.handle.net/20.500.12386/26349We present a new method to search for candidate z ≳ 2 Herschel 500 μm sources in the Great Observatories Origins Deep Survey-North field using a S<SUB>500 μm</SUB>/S<SUB>24 μm</SUB> “color deconfusion” technique. Potential high-z sources are selected against low-redshift ones from their large 500 to 24 μm flux density ratios. By effectively reducing the contribution from low-redshift populations to the observed 500 μm emission, we are able to identify counterparts to high-z 500 μm sources whose 24 μm fluxes are relatively faint. The recovery of known z ≳ 4 starbursts confirms the efficiency of this approach in selecting high-z Herschel sources. The resulting sample consists of 34 dusty star-forming galaxies at z ≳ 2. The inferred infrared luminosities are in the range 1.5 × 10<SUP>12</SUP>-1.8 × 10<SUP>13</SUP> L<SUB>☉</SUB>, corresponding to dust-obscured star formation rates (SFRs) of ∼260-3100 M<SUB>☉</SUB> yr<SUP>-1</SUP> for a Salpeter initial mass function. Comparison with previous SCUBA 850 μ {{m}}-selected galaxy samples shows that our method is more efficient at selecting high-z dusty galaxies, with a median redshift of z=3.07+/- 0.83 and with 10 of the sources at z ≳ 4. We find that at a fixed luminosity, the dust temperature is ∼5 K cooler than that expected from the {T}<SUB>d</SUB>-{L}<SUB>{{IR</SUB>}} relation at z\quad ≲ 1, though different temperature selection effects should be taken into account. The radio-detected subsample (excluding three strong active galactic nucleus) follows the far-infrared (far-IR)/radio correlation at lower redshifts, and no evolution with redshift is observed out to z∼ 5, suggesting that the far-IR emission is star formation dominated. The contribution of the high-z Herschel 500 μm sources to the cosmic SFR density is comparable to that of (sub)millimeter galaxy populations at z∼ 2.5 and at least 40% of the extinction-corrected UV samples at z∼ 4. Further investigation into the nature of these high-z dusty galaxies will be crucial for our understanding of the star formation histories and the buildup of stellar mass at the earliest cosmic epochs.STAMPAenArticle10.3847/0067-0049/222/1/42-s2.0-84955451286000368982300004https://iopscience.iop.org/article/10.3847/0067-0049/222/1/4https://arxiv.org/abs/1512.001672016ApJS..222....4SFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering