The Evolving AGN Duty Cycle in Galaxies Since z ∼ 3 as Encoded in the X-Ray Luminosity Function-Reference-Cited by-同舟云学术

The Evolving AGN Duty Cycle in Galaxies Since z ∼ 3 as Encoded in the X-Ray Luminosity Function

Published:2020-03-23 Issue:1 Volume:892 Page:17
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Delvecchio I.^ORCID,Daddi E.^ORCID,Aird J.^ORCID,Mullaney J. R.^ORCID,Bernhard E.,Grimmett L. P.,Carraro R.,Cimatti A.^ORCID,Zamorani G.^ORCID,Caplar N.^ORCID,Vito F.^ORCID,Elbaz D.,Rodighiero G.^ORCID

Funder

European Union’s Horizon 2020 - Marie Curie grant

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab789c/pdf

Reference137 articles.

1. THENuSTAREXTRAGALACTIC SURVEY: FIRST DIRECT MEASUREMENTS OF THE ≳10 keV X-RAY LUMINOSITY FUNCTION FOR ACTIVE GALACTIC NUCLEI ATz> 0.1

2. X-rays across the galaxy population – I. Tracing the main sequence of star formation

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

4. X-rays across the galaxy population – III. The incidence of AGN as a function of star formation rate

5. PRIMUS: THE DEPENDENCE OF AGN ACCRETION ON HOST STELLAR MASS AND COLOR

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