Can we reproduce the X-ray background spectral shape using local active galactic nuclei?

Astrophysical Journal Letters

Volumn 770, Issue 2, 2013, Pages

  Vasudevan, Ranjan V ^a   Mushotzky, Richard F ^a   Gandhi, Poshak ^b,c  

^a University of Maryland   (United States)

^b JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^c DURHAM UNIVERSITY   (United Kingdom)

Author keywords

black hole physics; galaxies: active; galaxies: evolution; X rays: diffuse background

Indexed keywords

EID: 84879110201     PISSN: 20418205     EISSN: 20418213     Source Type: Journal    
DOI: 10.1088/2041-8205/770/2/L37     Document Type: Article

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