Author
Listed:
- D. P. Marrone
(Steward Observatory, University of Arizona)
- J. S. Spilker
(Steward Observatory, University of Arizona)
- C. C. Hayward
(Center for Computational Astrophysics, Flatiron Institute
Harvard-Smithsonian Center for Astrophysics)
- J. D. Vieira
(University of Illinois)
- M. Aravena
(Núcleo de Astronomía, Facultad de Ingeniería, Universidad Diego Portales)
- M. L. N. Ashby
(Harvard-Smithsonian Center for Astrophysics)
- M. B. Bayliss
(Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology)
- M. Béthermin
(Aix Marseille Université, CNRS, LAM, Laboratoire d’Astrophysique de Marseille)
- M. Brodwin
(University of Missouri)
- M. S. Bothwell
(Cavendish Laboratory, University of Cambridge
Kavli Institute for Cosmology, University of Cambridge)
- J. E. Carlstrom
(Kavli Institute for Cosmological Physics, University of Chicago
University of Chicago
Enrico Fermi Institute, University of Chicago
University of Chicago)
- S. C. Chapman
(Dalhousie University)
- Chian-Chou Chen
(European Southern Observatory, Karl Schwarzschild Straße 2)
- T. M. Crawford
(Kavli Institute for Cosmological Physics, University of Chicago
University of Chicago)
- D. J. M. Cunningham
(Dalhousie University
Saint Mary’s University)
- C. De Breuck
(European Southern Observatory, Karl Schwarzschild Straße 2)
- C. D. Fassnacht
(University of California)
- A. H. Gonzalez
(University of Florida, Bryant Space Sciences Center)
- T. R. Greve
(University College London)
- Y. D. Hezaveh
(Kavli Institute for Particle Astrophysics and Cosmology, Stanford University)
- K. Lacaille
(McMaster University)
- K. C. Litke
(Steward Observatory, University of Arizona)
- S. Lower
(University of Illinois)
- J. Ma
(University of Florida, Bryant Space Sciences Center)
- M. Malkan
(University of California)
- T. B. Miller
(Dalhousie University)
- W. R. Morningstar
(Kavli Institute for Particle Astrophysics and Cosmology, Stanford University)
- E. J. Murphy
(National Radio Astronomy Observatory)
- D. Narayanan
(University of Florida, Bryant Space Sciences Center)
- K. A. Phadke
(University of Illinois)
- K. M. Rotermund
(Dalhousie University)
- J. Sreevani
(University of Illinois)
- B. Stalder
(Large Synoptic Survey Telescope)
- A. A. Stark
(Harvard-Smithsonian Center for Astrophysics)
- M. L. Strandet
(Max-Planck-Institut für Radioastronomie
International Max Planck Research School (IMPRS) for Astronomy and Astrophysics, Universities of Bonn and Cologne)
- M. Tang
(Steward Observatory, University of Arizona)
- A. Weiß
(Max-Planck-Institut für Radioastronomie)
Abstract
Two extremely massive galaxies are seen 800 million years after the Big Bang, showing the rapid growth of early structure and marking the most massive halo known in that era.
Suggested Citation
D. P. Marrone & J. S. Spilker & C. C. Hayward & J. D. Vieira & M. Aravena & M. L. N. Ashby & M. B. Bayliss & M. Béthermin & M. Brodwin & M. S. Bothwell & J. E. Carlstrom & S. C. Chapman & Chian-Chou C, 2018.
"Galaxy growth in a massive halo in the first billion years of cosmic history,"
Nature, Nature, vol. 553(7686), pages 51-54, January.
Handle:
RePEc:nat:nature:v:553:y:2018:i:7686:d:10.1038_nature24629
DOI: 10.1038/nature24629
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