The Faint End of the Quasar Luminosity Function at z ∼ 5 from the Subaru Hyper Suprime-Cam Survey-Reference-Cited by-同舟云学术

The Faint End of the Quasar Luminosity Function at z ∼ 5 from the Subaru Hyper Suprime-Cam Survey

Published:2020-11-24 Issue:2 Volume:904 Page:89
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Niida Mana,Nagao Tohru^ORCID,Ikeda Hiroyuki^ORCID,Akiyama Masayuki^ORCID,Matsuoka Yoshiki,He Wanqiu,Matsuoka Kenta^ORCID,Toba Yoshiki^ORCID,Onoue Masafusa^ORCID,Kobayashi Masakazu A. R.^ORCID,Taniguchi Yoshiaki^ORCID,Furusawa Hisanori^ORCID,Harikane Yuichi^ORCID,Imanishi Masatoshi^ORCID,Kashikawa Nobunari^ORCID,Kawaguchi Toshihiro^ORCID,Komiyama Yutaka,Shirakata Hikari,Terashima Yuichi^ORCID,Ueda Yoshihiro^ORCID

Funder

JSPS

the Mitsubishi Foundation

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abbe11/pdf

Reference95 articles.

1. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY

2. The rest-frame UV luminosity function at z ≃ 4: a significant contribution of AGNs to the bright end of the galaxy population