The formation of supermassive black holes from Population III.1 seeds. I. Cosmic formation histories and clustering properties

Journal Article · Thu Dec 06 00:00:00 EST 2018 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/sty3298· OSTI ID:1488992

Banik, Nilanjan  ^[1]; Tan, Jonathan C. ^[2]; Monaco, Pierluigi ^[3]

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1. Department of Physics, University of Florida, Gainesville, FL 32611, USA, Fermi National Accelerator Laboratory, Batavia, IL 60510-0500, USA, GRAPPA Institute, Institute for Theoretical Physics Amsterdam and Delta Institute for Theoretical Physics, University of Amsterdam, Science Park 904, NL-1098 XH Amsterdam, the Netherlands, Lorentz Institute, Leiden University, Niels Bohrweg 2, Leiden, NL-2333 CA, the Netherlands
2. Department of Space, Earth and Environment, Chalmers University of Technology, SE-412 93 Gothenburg, Sweden, Department of Astronomy, University of Virginia, 530 McCormick Road, Charlottesville, VA 22904-4325, USA
3. Dipartimento di Fisica, Sezione di Astronomia, Università di Trieste, via Tiepolo 11, I-34143 Trieste, Italy, INAF – Osservatorio Astronomico di Trieste, via Tiepolo 11, I-34143 Trieste, Italy, INFN, via Valerio 2, I-34127 Trieste, Italy

• Sponsoring Organization: USDOE
• Grant/Contract Number: AC02-07CH11359
• OSTI ID: 1488992
• Journal Information: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Vol. 483 Journal Issue: 3; ISSN 0035-8711
• Publisher: Oxford University Press
• Country of Publication: United Kingdom
• Language: English