Bonn 2010 – scientific programme
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T: Fachverband Teilchenphysik
T 93: Gammaastronomie II
T 93.3: Talk
Tuesday, March 16, 2010, 17:20–17:35, HG XVII
MAGIC observations of the Crab pulsar — •Takayuki Saito1, Nepomuk Otte2, Michael Rissi3, Thomas Schweizer1, and Maxim Shayduk1 — 1Max-Planck-Institut fuer Physik, Muenchen, Germany — 2Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, USA — 3ETH, Zurich, Switzerland
MAGIC detected pulsed gamma-rays above 25 GeV from the Crab pulsar in winter 2007-2008 and follow-up observation was done in winter 2008-2009. Here we will present the datailed analysis results including phase resolved energy spectra, energy dependence of P1/P2 ratio and peak phases. These results will be compared with the Fermi-LAT results from 100 MeV to 20 GeV.