Abstract: X-ray data for quasar 4C 74.26 have previously been modeled with a broad Fe Ka emission line and re?ection continuum originating in the inner part of the accretion disk around the central supermassive black hole (SMBH), i.e., the strong-gravity regime. We modeled broadband X-ray spectra from Suzaku and NuSTAR with MYTORUS, self-consistently accounting for Fe Ka line emission, as well as direct and re?ected continuum emission, from matter with a ?nite column density. A narrow Fe Ka emission li...

Source: Broadband X-Ray Constraints on the Accreting Black Hole in Quasar 4C 74.26