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The Early Early Type: Discovery of a Passive Galaxy at $_{Zspec}$ $\sim$ 3

Authors :
Masato Onodera
Alessandro Cimatti
Mark Dickinson
Marcella Carollo
Matthieu Béthermin
Raphael Gobat
Emanuele Daddi
Alvio Renzini
V. Strazzullo
Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112))
Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)
Institute for Astronomy [Zürich]
Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology in Zürich [Zürich] (ETH Zürich)
INAF - Osservatorio Astronomico di Padova (OAPD)
Istituto Nazionale di Astrofisica (INAF)
National Optical Astronomy Observatory (NOAO)
Dipartimento di Astronomia
Università di Bologna [Bologna] (UNIBO)
UPGAL
European Project: 240039,EC:FP7:ERC,ERC-2009-StG,UPGAL(2009)
Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich)
Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)
Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Gobat R.
Strazzullo V.
Daddi E.
Onodera M.
Renzini A.
Béthermin M.
Dickinson M.
Carollo M.
Cimatti A.
Source :
Astrophysical Journal Letters, Astrophysical Journal Letters, 2012, 759 (2), pp.L44. ⟨10.1088/2041-8205/759/2/L44⟩, The Astrophysical journal letters, The Astrophysical journal letters, Bristol : IOP Publishing, 2012, 759 (2), pp.L44. ⟨10.1088/2041-8205/759/2/L44⟩, The Astrophysical journal letters, 2012, 759 (2), pp.L44. ⟨10.1088/2041-8205/759/2/L44⟩
Publication Year :
2012
Publisher :
HAL CCSD, 2012.

Abstract

We present the discovery of a massive, quiescent galaxy at z=2.99. We have obtained a HST/WFC3 spectrum of this object and measured its redshift from the detection of a deep 4000A break consistent with an old population and a high metallicity. By stellar population modeling of both its grism spectrum and broad-band photometry, we derive an age of ~0.7 Gyr, implying a formation redshift of z>4, and a mass >10^11 Msun. Although this passive galaxy is the most distant confirmed so far, we find that it is slightly less compact than other z>2 early-types of similar mass, being overall more analogous to those z~1.6 field early-type galaxies. The discovery of this object shows that early-type galaxies are detectable to at least z=3 and suggests that the diversity of structural properties found in z=1.4-2 ellipticals to earlier epochs could have its origin in a variety of formation histories among their progenitors.<br />6 pages, 4 figures, 1 table. Accepted for publication in The Astrophysical Journal Letters

Details

Language :
English
ISSN :
20418205 and 20418213
Database :
OpenAIRE
Journal :
Astrophysical Journal Letters, Astrophysical Journal Letters, 2012, 759 (2), pp.L44. ⟨10.1088/2041-8205/759/2/L44⟩, The Astrophysical journal letters, The Astrophysical journal letters, Bristol : IOP Publishing, 2012, 759 (2), pp.L44. ⟨10.1088/2041-8205/759/2/L44⟩, The Astrophysical journal letters, 2012, 759 (2), pp.L44. ⟨10.1088/2041-8205/759/2/L44⟩
Accession number :
edsair.doi.dedup.....e79f2a158fa3c4da6203e37e5f11c0e3
Full Text :
https://doi.org/10.1088/2041-8205/759/2/L44⟩