MAGIC very large zenith angle observations of the Crab Nebula up to 100 TeV
Aims: We measure the Crab Nebula γ-ray spectral energy distribution in the ~100 TeV energy domain and test the validity of existing leptonic emission models at these high energies. Methods: We used the novel very large zenith angle observations with the MAGIC telescope system to increase the collection area above 10 TeV. We also developed an
MAGIC Collaboration et al.
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2020