In a hard-X-ray-selected sample of 236 nearby unobscured AGN, the 2-10 keV X-ray bolometric correction is primarily set by Eddington ratio, with the luminosity dependence vanishing below λEdd ≈ 0.01.
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BASS LIII: The Eddington Ratio as the Primary Regulator of the Fraction of X-ray Emission in Active Galactic Nuclei
In a hard-X-ray-selected sample of 236 nearby unobscured AGN, the 2-10 keV X-ray bolometric correction is primarily set by Eddington ratio, with the luminosity dependence vanishing below λEdd ≈ 0.01.