
doi: 10.1063/1.2757375
Pulsars were detected by EGRET up to energies below 20 GeV. Observations at higher energies with ground‐based experiments, including MAGIC, so far failed to detect pulsars, indicating a sharp cutoff of the pulsed emission. Here we present, in particular, the results of the search for very high γ‐ray emission from the pulsar PSR B1951+32.
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