Bolometric correction factors for active galactic nuclei
نویسندگان
چکیده
منابع مشابه
Piecing Together the X-ray Background: Bolometric Corrections for Active Galactic Nuclei
The X-ray background can be used to constrain the accretion history of Supermassive Black Holes (SMBHs) in Active Galactic Nuclei (AGN), with the SMBH mass density related to the energy density due to accretion. A knowledge of the hard X-ray bolometric correction, κ2−10keV is a vital input into these studies, as it allows us to constrain the parameters of the accretion responsible for SMBH grow...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2019
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/stz2016