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Cited article:

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AChandraLook at Five of the Broadest Double‐Peaked Balmer Line Emitters

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XMM-Newtonobservations of 4 luminous radio-quiet AGN, and the soft X-ray excess problem

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A broad-line region origin for the iron Kα line in NGC 7213

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Observational Constraints on the Dependence of Radio‐Quiet Quasar X‐Ray Emission on Black Hole Mass and Accretion Rate

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Can photo-ionisation explain the decreasing fraction of X-ray obscured AGN with luminosity?

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The X‐Ray Properties of the Most Luminous Quasars from the Sloan Digital Sky Survey

D. W. Just, W. N. Brandt, O. Shemmer, et al.
The Astrophysical Journal 665 (2) 1004 (2007)
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