  We report on the observations of the Crab pulsar with the MAGIC telesopes.
Data were taken both in the mono-mode ($>25$ GeV) and in the stereo-mode ($>50$
GeV). Clear signals from the two peaks were detected with both modes and the
phase resolved energy spectra were calculated. By comparing with the
measurements done by Fermi-LAT, we found that the energy spectra of the Crab
pulsar does not follow a power law with an exponential cutoff, but that it
extends as a power law after the break at around 5 GeV. This suggests that the
emission above 25 GeV is not dominated by the curvatura radiation, which is
inconsistent with the standard prediction of the OG and SG models.
