The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day

Schreiber, C.; Pannella, M.; Elbaz, D.; Béthermin, M.; Inami, H.; Dickinson, M.; Magnelli, B.; Wang, T.; Aussel, H.; Daddi, E.; Juneau, S.; Shu, X.; Sargent, M. T.; Buat, V.; Faber, S. M.; Ferguson, H. C.; Giavalisco, M.; Koekemoer, A. M.; Magdis, G.; Morrison, G. E.; Papovich, C.; Santini, P.; Scott, D.

doi:10.1051/0004-6361/201425017

articleAstronomy and AstrophysicsFeb 25, 2015BRONZE OA

The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day

CSC. SchreiberMPM. PannellaDED. ElbazMBM. BétherminHIH. Inami

Centre National de la Recherche Scientifique · Université Paris Cité · +24 more institutions

Indexed inarxivcrossrefdoaj

Abstract

We present an analysis of the deepest Herschel images in four major extragalactic fields GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel and CANDELS–Herschel key programs. The star formation picture provided by a total of 10 497 individual far-infrared detections is supplemented by the stacking analysis of a mass complete sample of 62 361 star-forming galaxies from the Hubble Space Telescope (HST) H band-selected catalogs of the CANDELS survey and from two deep ground-based Ks band-selected catalogs in the GOODS–North and the COSMOS-wide field to obtain one of the most accurate and unbiased understanding to date of the stellar mass growth over the cosmic history. We show, for the…

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Authors

23

CS
C. SchreiberCorresponding
Centre National de la Recherche Scientifique, Université Paris Cité, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Astrophysique, Instrumentation et Modélisation, CEA Paris-Saclay
MP
M. Pannella
Centre National de la Recherche Scientifique, Université Paris Cité, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Institut d'Astrophysique de Paris, Sorbonne Université, Astrophysique, Instrumentation et Modélisation, CEA Paris-Saclay
DE
D. Elbaz
Centre National de la Recherche Scientifique, Université Paris Cité, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Astrophysique, Instrumentation et Modélisation, CEA Paris-Saclay
MB
M. Béthermin
Centre National de la Recherche Scientifique, Université Paris Cité, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Astrophysique, Instrumentation et Modélisation, CEA Paris-Saclay
HI
H. Inami
Kitt Peak National Observatory

Topics & keywords

Topics

Keywords

Galaxy
Redshift
Flattening
Stellar mass
Star formation
Hubble Ultra-Deep Field
Galaxy formation and evolution
Luminosity

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