Speaker
Peter Marinos
(University of Adelaide)
Description
We use the simulation software "GALPROP" to model the Milky Way's diffuse TeV gamma-ray emission and how the diffuse emission will vary over time. We compare GALPROP's predictions to observational data, investigating how the emission will impact the forthcoming CTA Observatory's Galactic plane survey.
Primary author
Peter Marinos
(University of Adelaide)
