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Modeling Fermi Large Area Telescope and Multiwavelength Data from Blazars
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Blazars are active galactic nuclei with relativistic jets pointed at the Earth, making them extremely bright at essentially all wavelengths, from radio to gamma rays. I review the modeling of this broadband spectral energy distributions of these objects, and what we have learned, with a focus on gamma rays.
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The High-redshift Blazar MG3 J163554+3629: Physical Properties and the Enigma of Its Unexpected Supermassive Black Hole Growth
A one-zone SED fit for the z=3.65 blazar gives MBH≈1.1e9 Msun and eta=0.083, but the claimed Eddington-growth failure is an artifact of an inverted efficiency factor in Eq. (3).
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