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The Radio to TeV Synchrotron and Inverse Compton Emission from Extragalactic Relativistic Jets

Markos Georganopoulos, Department of Physics
Amanda Dotson, Department of Physics

We are developing state of the art models for the steady-state and time-dependent emission from extragalactic jets of non-thermal plasma. The codes we are developing will be used for modeling current and upcoming observations, with emphasis on the Gamma ray results from Fermi, NASA’s new Gamma Ray orbiting observatory.