MAGIC observations of the diffuse γ-ray emission in the vicinity of the Galactic center
Aims: In the presence of a sufficient amount of target material, γ-rays can be used as a tracer in the search for sources of Galactic cosmic rays (CRs). Here we present deep observations of the Galactic center (GC) region with the MAGIC telescopes and use them to infer the underlying CR distribution and to study the alleged PeV proton accelerator
MAGIC Collaboration et al.
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10
2020