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BAT AGN Spectroscopic Survey XII The relation between coronal properties of active galactic nuclei and the Eddington ratio

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Figure 1. Histogram of the cut-off energy of unobscured (N H < 10 22 cm −2 ) sources from the Swift/BAT AGN catalogue of Ricci et al
Figure 2. Left-hand panel: Cut-off energy versus the 14–150 keV intrinsic luminosity (in erg s −1 ) for the sources in our sample
Figure 5. Median values of the cut-off energy for different intervals of Eddington ratio considering different 2–10 keV bolometric corrections: the λ Edd -dependent bolometric corrections of Vasudevan & Fabian (2007)  (or-ange dot–dot–dashed line) and
Figure 6. Cut-off energy versus the luminosity for two ranges of black hole mass (left-hand panel, in units of M  ) and of Eddington ratio (right-hand panel).
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