The \(\gamma\)-ray Milky Way above 10 GeV:
Distinguishing Sources from Diffuse Emission

Abstract

One of the most prominent features of the gamma-ray sky is the emission from our own galaxy. The Galactic plane has been observed by Fermi/LAT in GeV and H.E.S.S. in TeV light. Fermi has modeled the Galactic emission as the sum of a c