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During the last 4 years the MAGIC collaboration has searched for high-energygamma-ray emission of some of the most promising pulsar candidates. The lowenergy threshold of MAGIC offered the opportunity for a high sensitivity searchjust above 50-100 GeV (since 2008 a new trigger system has decreased the energythreshold to 25 GeV), an energy region up to now not reachable to ground basedinstruments and past satellite borne detectors. No pulsed gamma-ray emissionhas been detected from any pulsar observed during the observation campaigns of2005-2006. Here we present the upper limits obtained for tow canonical pulsars(PSR J0205+6449 and PSR J2229+6114) and their host nebulae (3C 58 andBoomerang, respectively) and the millisecond pulsar PSR J0218+4232. Physicsimplications will be discussed.

Upper limits for pulsars with MAGIC (2005/2006 observations)