Pulsar observations with the MAGIC Telescope

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.