DETERMINING THE COVERING FACTOR OF COMPTON-THICK ACTIVE GALACTIC NUCLEI WITHNuSTAR-Reference-Cited by-同舟云学术

DETERMINING THE COVERING FACTOR OF COMPTON-THICK ACTIVE GALACTIC NUCLEI WITHNuSTAR

Published:2015-05-19 Issue:1 Volume:805 Page:41
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Brightman M.,Baloković M.,Stern D.^ORCID,Arévalo P.,Ballantyne D. R.,Bauer F. E.,Boggs S. E.,Craig W. W.,Christensen F. E.,Comastri A.,Fuerst F.,Gandhi P.,Hailey C. J.,Harrison F. A.,Hickox R. C.,Koss M.,LaMassa S.,Puccetti S.^ORCID,Rivers E.,Vasudevan R.,Walton D. J.,Zhang W. W.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/805/i=1/a=41/pdf

Reference73 articles.

1. XMM-Newton observations of Seyfert galaxies from the Palomar spectroscopic survey: the X-ray absorption distribution

2. XMM-Newton and Chandra measurements of the AGN intrinsic absorption: dependence on luminosity and redshift

3. Abundances of the elements: Meteoritic and solar

4. THE 2-79 keV X-RAY SPECTRUM OF THE CIRCINUS GALAXY WITHNuSTAR,XMM-Newton, ANDCHANDRA: A FULLY COMPTON-THICK ACTIVE GALACTIC NUCLEUS

5. MID-INFRARED SELECTION OF ACTIVE GALACTIC NUCLEI WITH THEWIDE-FIELD INFRARED SURVEY EXPLORER. II. PROPERTIES OFWISE-SELECTED ACTIVE GALACTIC NUCLEI IN THE NDWFS BOÖTES FIELD

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