Slowing down of cosmic growth of supermassive black holes: theoretical prediction of the Eddington ratio distribution-Reference-Cited by-同舟云学术

Slowing down of cosmic growth of supermassive black holes: theoretical prediction of the Eddington ratio distribution

Published:2019-05-14 Issue:1 Volume:487 Page:409-419
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Shirakata Hikari¹²,Kawaguchi Toshihiro³,Oogi Taira⁴,Okamoto Takashi¹,Nagashima Masahiro⁵

Affiliation:

1. Department of Cosmosciences, Graduate School of Science, Hokkaido University, N10 W8, Kitaku, Sapporo 060-0810, Japan

2. Advanced Technology Research Center, Tadano Ltd., 2217-13, Hayashi-Cho, Takamatsu, Kagawa 761-0301, Japan

3. Department of Economics, Management and Information Science, Onomichi City University, 1600-2, Hisayamada, Onomichi, Hiroshima 722-8506, Japan

4. Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, the University of Tokyo, 5-1-5, Kashiwanoha, Kashiwa, 277-8583 Japan

5. Faculty of Education, Bunkyo University, 3337, Minami-ogishima, Koshigaya, Saitama 343-8511, Japan

Funder

Japan Science Society

Japan Society for the Promotion of Science

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/487/1/409/28701757/stz1282.pdf

Reference49 articles.

1. Slim accretion disks

2. X-rays across the galaxy population – II. The distribution of AGN accretion rates as a function of stellar mass and redshift

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

4. Evidence for a mass-dependent AGN Eddington ratio distribution via the flat relationship between SFR and AGN luminosity

Cited by 13 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. Connecting low-redshift LISA massive black hole mergers to the nHz stochastic gravitational wave background;Astronomy & Astrophysics;2024-06

2. The evolution of supermassive black hole mass–bulge mass relation by a semi-analytical model, ν2GC;Monthly Notices of the Royal Astronomical Society;2024-05-13

3. Steep-spectrum AGN in eROSITA Final Equatorial-Depth Survey (eFEDS): Their host galaxies and multi-wavelength properties;Astronomy & Astrophysics;2024-04

4. Black Hole Mass and Eddington-ratio Distributions of Less-luminous Quasars at z ∼ 4 in the Subaru Hyper Suprime-Cam Wide Field;The Astrophysical Journal;2024-02-01

5. Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVII. Black Hole Mass Distribution at z ∼ 6 Estimated via Spectral Comparison with Low-z Quasars;The Astrophysical Journal;2024-01-01