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Title: An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5

Journal Article · · Nature (London)
DOI:https://doi.org/10.1038/nature25180· OSTI ID:1543732
 [1];  [2];  [2];  [2];  [2];  [3];  [4];  [5];  [6];  [7];  [7];  [8];  [9];  [2];  [3];  [1];  [1];  [10]
  1. The Observatories of the Carnegie Inst. for Science, Pasadena, CA (United States)
  2. Max Planck Inst. für Astronomie, Heidelberg (Germany)
  3. Peking Univ., Beijing (China)
  4. Max Planck Inst. für Astronomie, Heidelberg (Germany); Istituto Nazionale di Astrofisica (INAF), Bologna (Italy)
  5. California Inst. of Technology (CalTech), La Canada Flintridge, CA (United States). Jet Propulsion Lab.
  6. Univ. of Arizona, Tucson, AZ (United States)
  7. Univ. of California, Santa Barbara, CA (United States)
  8. MIT-Kavli Center for Astrophysics and Space Research, Cambridge, MA (United States)
  9. MIT-Kavli Center for Astrophysics and Space Research, Cambridge, MA (United States); Las Cumbres Observatory, Goleta, CA (United States)
  10. Inst. de Radioastronomie Millimétrique (IRAM), Saint Martin d’Hères (France)

Quasars are the most luminous non-transient objects known and as a result they enable studies of the Universe at the earliest cosmic epochs. Despite extensive efforts, however, the quasar ULAS J1120 + 0641 at redshift z = 7.09 has remained the only one known at z > 7 for more than half a decade. Here we report observations of the quasar ULAS J134208.10 + 092838.61 (hereafter J1342 + 0928) at redshift z = 7.54. This quasar has a bolometric luminosity of 4 × 1013 times the luminosity of the Sun and a black-hole mass of 8 × 108 solar masses. The existence of this supermassive black hole when the Universe was only 690 million years old—just five per cent of its current age—reinforces models of early black-hole growth that allow black holes with initial masses of more than about 104 solar masses or episodic hyper-Eddington accretion. We see strong evidence of absorption of the spectrum of the quasar redwards of the Lyman α emission line (the Gunn–Peterson damping wing), as would be expected if a significant amount (more than 10 per cent) of the hydrogen in the intergalactic medium surrounding J1342 + 0928 is neutral. We derive such a significant fraction of neutral hydrogen, although the exact fraction depends on the modelling. However, even in our most conservative analysis we find a fraction of more than 0.33 (0.11) at 68 per cent (95 per cent) probability, indicating that we are probing well within the reionization epoch of the Universe.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Sponsoring Organization:
USDOE
OSTI ID:
1543732
Journal Information:
Nature (London), Vol. 553, Issue 7689; ISSN 0028-0836
Publisher:
Nature Publishing GroupCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 596 works
Citation information provided by
Web of Science

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