A new model of quasar mass evolution-Reference-Cited by-同舟云学术

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A new model of quasar mass evolution

Published:2022-08 Issue:8 Volume:367 Page:
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Li Zheng^ORCID,Zhang Ming,Peng Qiu-He,Liu Xiang

Funder

National Natural Science Foundation of China

West Light Foundation of the Chinese Academy of Sciences

Regional Collaborative Innovation Project of Xinjiang Uyghur Autonomous Region

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://link.springer.com/content/pdf/10.1007/s10509-022-04101-1.pdf

Reference60 articles.

1. Abazajian, K.N., Adelman-McCarthy, J.K., Agüeros, M.A., et al.: The seventh data release of the Sloan Digital Sky Survey. Astrophys. J. Suppl. Ser. 182(2), 543–558 (2009)

2. Abel, T., Bryan, G.L., Norman, M.L.: The formation of the first star in the Universe. Science 295, 93–98 (2002)

3. Avni, Y., Soltan, A., Tananbaum, H., Zamorani, G.: A method for determining luminosity functions incorporating both flux measurements and flux upper limits, with applications to the average X-ray to optical luminosity ratio for quasars. Astrophys. J. 238, 800–807 (1980)

4. Baganoff, F.K., Maeda, Y., Morris, M., et al.: Chandra X-ray spectroscopic imaging of Sagittarius A* and the central parsec of the galaxy. Astrophys. J. 591(2), 891–915 (2003)

5. Bañados, E., Venemans, B.P., Mazzucchelli, C., et al.: An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5. Nature 553, 473–476 (2018)

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