The Hard X-Ray Spectral Slope as an Accretion Rate Indicator in Radio-Quiet Active Galactic Nuclei

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This article presents XMM-Newton observations of two luminous and high accretion rate radio-quiet active galactic nuclei at z ~ 2.

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4 p.

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Shemmer, Ohad; Brandt, William Nielsen; Netzer, Hagai; Maiolino, Roberto & Kaspi, Shai June 14, 2006.

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This article presents XMM-Newton observations of two luminous and high accretion rate radio-quiet active galactic nuclei at z ~ 2.

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4 p.

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  • The Astrophysical Journal, 2006. Washington, DC: The American Astronomical Society

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  • Publication Title: The Astrophysical Journal
  • Volume: 646
  • Page Start: 29
  • Page End: 32

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  • June 14, 2006

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  • Aug. 17, 2016, 10:44 p.m.

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  • Aug. 19, 2016, 10:55 a.m.

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Shemmer, Ohad; Brandt, William Nielsen; Netzer, Hagai; Maiolino, Roberto & Kaspi, Shai. The Hard X-Ray Spectral Slope as an Accretion Rate Indicator in Radio-Quiet Active Galactic Nuclei, article, June 14, 2006; Washington, DC. (digital.library.unt.edu/ark:/67531/metadc861705/: accessed September 21, 2017), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT College of Arts and Sciences.