X-Ray Bolometric Corrections for Compton-thick Active Galactic Nuclei-Reference-Cited by-同舟云学术

X-Ray Bolometric Corrections for Compton-thick Active Galactic Nuclei

Published:2017-07-17 Issue:1 Volume:844 Page:10
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Brightman M.,Baloković M.,Ballantyne D. R.^ORCID,Bauer F. E.^ORCID,Boorman P.^ORCID,Buchner J.^ORCID,Brandt W. N.^ORCID,Comastri A.^ORCID,Moro A. Del,Farrah D.^ORCID,Gandhi P.^ORCID,Harrison F. A.^ORCID,Koss M.^ORCID,Lanz L.^ORCID,Masini A.^ORCID,Ricci C.^ORCID,Stern D.^ORCID,Vasudevan R.,Walton D. J.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/844/i=1/a=10/pdf

Reference82 articles.

1. The evolution of the X-ray luminosity functions of unabsorbed and absorbed AGNs out to z∼ 5

2. Compton-thick AGN in the 70-monthSwift-BAT All-Sky Hard X-ray Survey: A Bayesian approach

3. TORUS AND ACTIVE GALACTIC NUCLEUS PROPERTIES OF NEARBY SEYFERT GALAXIES: RESULTS FROM FITTING INFRARED SPECTRAL ENERGY DISTRIBUTIONS AND SPECTROSCOPY

4. NuSTAROBSERVATIONS OF THE COMPTON-THICK ACTIVE GALACTIC NUCLEUS AND ULTRALUMINOUS X-RAY SOURCE CANDIDATE IN NGC 5643

5. Unified Models for Active Galactic Nuclei and Quasars

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