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Detecting Galactic diffuse emission in the Very High Energy domain
Blanc – Accords bilatéraux 2013 - SIMI 5 - Physique subatomique et théories associées, astrophysique, astronomie et planétologie
2013
Diffuse emission is the most prominent observational signature from the sky at Gigaelectronvolt (GeV) energies. Galactic diffuse emission was established before individual gamma-ray sources started to emerge and constitute a prime source of knowledge about cosmic-ray particle interactions and radiat
