The MAGIC telescope has detected for the first time pulsed gamma-rays from the Crab pulsar in the VHE domain [ 1 ] .
The observations were performed with a newly developed trigger system that allows us to lower the energy threshold of the telescope from 55 GeV to 25 GeV .
We present a comparison of light curves measured by our experiment with the one measured by space detectors .
A strong energy dependent decrease of the first peak with respect to the second peak P1/P2 could be observed .
Finally , fitting our measured data and previous measurements from EGRET we determine a turnover of the energy spectrum at 17.7 +- 2.8 ( stat . )
+- 5.0 ( syst . )
GeV , assuming an exponential cutoff .
This rules out the scenario in which the gamma rays are produced in vicinity of the polar caps of the neutron star .