The intense starburst HDF 850.1 in a galaxy overdensity at z ≈ 5.2 in the Hubble Deep Field

Fabian Walter (), Roberto Decarli, Chris Carilli, Frank Bertoldi, Pierre Cox, Elisabete Da Cunha, Emanuele Daddi, Mark Dickinson, Dennis Downes, David Elbaz, Richard Ellis, Jacqueline Hodge, Roberto Neri, Dominik A. Riechers, Axel Weiss, Eric Bell, Helmut Dannerbauer, Melanie Krips, Mark Krumholz, Lindley Lentati, Roberto Maiolino, Karl Menten, Hans-Walter Rix, Brant Robertson, Hyron Spinrad, Dan P. Stark and Daniel Stern
Additional contact information
Fabian Walter: Max-Planck Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany
Roberto Decarli: Max-Planck Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany
Chris Carilli: National Radio Astronomy Observatory, Pete V. Domenici Array Science Center, PO Box O, Socorro, New Mexico 87801, USA
Frank Bertoldi: Argelander Institute for Astronomy, University of Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
Pierre Cox: IRAM, 300 rue de la Piscine, F-38406 Saint-Martin d'Hères, France
Elisabete Da Cunha: Max-Planck Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany
Emanuele Daddi: Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, Irfu/Service d’Astrophysique, CEA Saclay, Orme des Merisiers, 91191 Gif-sur-Yvette cedex, France
Mark Dickinson: National Optical Astronomy Observatory, 950 North Cherry Avenue
Dennis Downes: IRAM, 300 rue de la Piscine, F-38406 Saint-Martin d'Hères, France
David Elbaz: Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, Irfu/Service d’Astrophysique, CEA Saclay, Orme des Merisiers, 91191 Gif-sur-Yvette cedex, France
Richard Ellis: California Institute of Technology, MC105-24, Pasadena, California 91125, USA
Jacqueline Hodge: Max-Planck Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany
Roberto Neri: IRAM, 300 rue de la Piscine, F-38406 Saint-Martin d'Hères, France
Dominik A. Riechers: California Institute of Technology, MC105-24, Pasadena, California 91125, USA
Axel Weiss: Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
Eric Bell: University of Michigan, 500 Church Street, Ann Arbor, Michigan 48109, USA
Helmut Dannerbauer: Universität Wien, Institut für Astronomie, Türkenschanzstraße 17, 1080 Wien, Austria
Melanie Krips: IRAM, 300 rue de la Piscine, F-38406 Saint-Martin d'Hères, France
Mark Krumholz: University of California
Lindley Lentati: Cavendish Laboratory, University of Cambridge, 19 J J Thomson Avenue, Cambridge CB3 0HE, UK
Roberto Maiolino: Cavendish Laboratory, University of Cambridge, 19 J J Thomson Avenue, Cambridge CB3 0HE, UK
Karl Menten: Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
Hans-Walter Rix: Max-Planck Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany
Brant Robertson: University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721, USA
Hyron Spinrad: University of California at Berkeley
Dan P. Stark: University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721, USA
Daniel Stern: Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA

Nature, 2012, vol. 486, issue 7402, 233-236

Abstract: Using a millimetre-wave molecular line scan, a redshift has finally been determined for the extremely active star-forming galaxy HDF 850.1 in the Hubble Deep Field, which makes it younger than thought at 1.1 billion years after the Big Bang.

Date: 2012
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DOI: 10.1038/nature11073

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