Speaker
Peter Marinos
(University of Adelaide)
Description
We have simulated the diffuse cosmic-ray sea and gamma-ray emission with GALPROP using a time-dependent solution to the transport equation to ensure the IC emissions are computed accurately. Our predictions are compared to the diffuse emission estimated by the H.E.S.S. telescope array, and the future prospects for detections with CTA will be discussed.
Primary author
Peter Marinos
(University of Adelaide)
