Spitzer Observations of Massive, Red Galaxies at High Redshift
Casey Papovich
(1)
,
Leonidas A. Moustakas
(2)
,
Mark Dickinson
(3)
,
E. Le Floc'H
(1, 4)
,
George H. Rieke
(1)
,
Emmanuele Daddi
(3)
,
David M. Alexander
(5)
,
F. Bauer
(6)
,
W. N. Brandt
(7)
,
Tomas Dahlén
(8)
,
E. Egami
(1)
,
Peter Eisenhardt
(2)
,
David Elbaz
(9)
,
Henry C. Ferguson
(8)
,
M. Giavalisco
(8)
,
Ray A. Lucas
(8)
,
Bahram Mobasher
(8)
,
Pablo G. Pérez-González
(1)
,
Amelia Stutz
(1)
,
M. J. Rieke
(1)
,
H. Yan
(10)
1
Steward Observatory
2 JPL - Jet Propulsion Laboratory
3 NOAO - National Optical Astronomy Observatory, Tucson
4 GEPI - Galaxies, Etoiles, Physique, Instrumentation
5 IoA - Institute of Astronomy, University of Cambridge
6 Columbia Astrophysics Laboratory, Columbia University, New York
7 Pennsylvania State University, Department of Astronomy & Astrophysics
8 STSci - Space Telescope Science Institute
9 CEA - Commissariat à l'énergie atomique et aux énergies alternatives
10 SSC - Spitzer Science Center, California Institute of Technology
2 JPL - Jet Propulsion Laboratory
3 NOAO - National Optical Astronomy Observatory, Tucson
4 GEPI - Galaxies, Etoiles, Physique, Instrumentation
5 IoA - Institute of Astronomy, University of Cambridge
6 Columbia Astrophysics Laboratory, Columbia University, New York
7 Pennsylvania State University, Department of Astronomy & Astrophysics
8 STSci - Space Telescope Science Institute
9 CEA - Commissariat à l'énergie atomique et aux énergies alternatives
10 SSC - Spitzer Science Center, California Institute of Technology
Résumé
We study massive galaxies at z~1-3.5 using HST optical imaging, ground-based near-IR imaging, and Spitzer observations at 3-24 mum. From Ks-selected galaxies in the ~=130 arcmin2 GOODS-S field, we identify 153 distant red galaxies (DRGs) with (J-Ks)Vega>=2.3. This sample is approximately complete in stellar mass for passively evolving galaxies above 1011 Msolar and z~4-6 mag) starbursts (at zmed~1.7). Very few DRGs (=1011 Msolar have specific star formation rates (SFRs per unit mass) including the reradiated far-IR emission that range from 0.2 to 10 Gyr-1. Based on the X-ray luminosities and rest-frame near-IR colors, roughly one-quarter of the DRGs contain AGNs, implying that the growth of supermassive black holes coincides with the formation of massive galaxies. At 1.5=1011 Msolar have an integrated specific SFR less than the global value and more than an order of magnitude lower than that for massive DRGs. At z