UMBC High Performance Computing Facility
Please note that this page is under construction. We are documenting the
240-node cluster maya that will be available in Spring 2014. Currently,
the cluster tara is still available. Please see the 2013 Resources Pages
under the Resources tab.
The Radio to TeV Synchrotron and Inverse Compton Emission from Extragalactic Relativistic Jets
Markos Georganopoulos and 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.