Early black holes in cosmological simulations: luminosity functions and clustering behaviour

Author:

DeGraf Colin1,Di Matteo Tiziana1,Khandai Nishikanta1,Croft Rupert1,Lopez Julio2,Springel Volker

Affiliation:

1. McWilliams Center for Cosmology; Carnegie Mellon University; 5000 Forbes Avenue; Pittsburgh; PA; 15213; USA

2. Computer Science Department; Carnegie Mellon University; 5000 Forbes Avenue; Pittsburgh; PA; 15213; USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 24 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Hungry or Not: How Stellar-Mass Black Holes Grow (or Don’t) in Dark Matter Mini-Haloes at High-Resolution;Monthly Notices of the Royal Astronomical Society;2024-02-22

2. Revisiting the extreme clustering of z ≈ 4 quasars with large volume cosmological simulations;Monthly Notices of the Royal Astronomical Society;2024-02-01

3. The low-end of the black hole mass function at cosmic dawn;Monthly Notices of the Royal Astronomical Society;2022-01-13

4. The host galaxies of z = 7 quasars: predictions from the BlueTides simulation;Monthly Notices of the Royal Astronomical Society;2020-10-05

5. Black Holes Across Cosmic History: A Journey Through 13.8 Billion Years;Black Hole Formation and Growth;2019

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