2017/08/17 by M. L. Ahnen, MAGIC Collaboration, Ahnen, M. L. +242
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Radiation Detection and Scintillator Technologies
paper · pdf · doi:10.48550/arxiv.1708.05153
openalex publication_date 2017/08/17 · openalex created_date 2022/10/03 · openalex updated_date 2026/07/28
MAGIC (Major Atmospheric Gamma Imaging Cherenkov) is a system of two 17 m diameter, F/1.03 Imaging Atmospheric Cherenkov Telescopes (IACT). They are dedicated to the observation of gamma rays from galactic and extragalactic sources in the very high energy range (VHE, 30 GeV to 100 TeV). This submission contains links to the proceedings for the 35th International Cosmic Ray Conference (ICRC2017), held in Bexco, Busan, Korea from the 12th to the 17th of July, 2017.