A massive, quiescent galaxy at a redshift of 3.717
Karl Glazebrook (),
Corentin Schreiber,
Ivo Labbé,
Themiya Nanayakkara,
Glenn G. Kacprzak,
Pascal A. Oesch,
Casey Papovich,
Lee R Spitler,
Caroline M. S. Straatman,
Kim-Vy H. Tran and
Tiantian Yuan
Additional contact information
Karl Glazebrook: Centre for Astrophysics and Supercomputing, Swinburne University of Technology
Corentin Schreiber: Leiden Observatory, Leiden University
Ivo Labbé: Leiden Observatory, Leiden University
Themiya Nanayakkara: Centre for Astrophysics and Supercomputing, Swinburne University of Technology
Glenn G. Kacprzak: Centre for Astrophysics and Supercomputing, Swinburne University of Technology
Pascal A. Oesch: Geneva Observatory, University of Geneva
Casey Papovich: George P. and Cynthia W. Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station
Lee R Spitler: Macquarie Research Centre for Astronomy, Astrophysics and Astrophotonics, Macquarie University
Caroline M. S. Straatman: Max Planck Institute for Astronomy
Kim-Vy H. Tran: George P. and Cynthia W. Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station
Tiantian Yuan: Research School of Astronomy and Astrophysics, The Australian National University
Nature, 2017, vol. 544, issue 7648, 71-74
Abstract:
A massive ancient galaxy with minimal star formation is observed spectroscopically at an epoch when the Universe is less than 2 billion years old, posing a challenge to theories.
Date: 2017
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Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:544:y:2017:i:7648:d:10.1038_nature21680
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DOI: 10.1038/nature21680
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