Relativistic reflection from accretion disks in the population of Active Galactic Nuclei at z=0.5–4

Author:

Baronchelli L1,Nandra K1,Buchner J2ORCID

Affiliation:

1. Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching bei München, Germany

2. Instituto de Astrofisica, Facultad de Fisica, Pontificia Universidad Catolica de Chile, Casilla 306, Santiago 22, Chile

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 12 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. Statistical Aspects of X-ray Spectral Analysis;Handbook of X-ray and Gamma-ray Astrophysics;2024

2. Statistical Aspects of X-ray Spectral Analysis;Handbook of X-ray and Gamma-ray Astrophysics;2023-09-20

3. Are Compton-thin AGNs Globally Compton Thin?;The Astrophysical Journal;2021-11-01

4. Testing horizon topology with electromagnetic observations;Physical Review D;2020-11-12

5. Relativistic accretion disc reflection in AGN X-ray spectra at z = 0.5–4: a study of four Chandra Deep Fields;Monthly Notices of the Royal Astronomical Society;2020-09-07

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