Observations of the Crab Pulsar between 25 and 100 GeV with the MAGIC I Telescope
We report on the observation of γ-rays above 25 GeV from the Crab pulsar (PSR B0532+21) using the MAGIC I telescope. Two data sets from observations during the winter period 2007/2008 and 2008/2009 are used. In order to discuss the spectral shape from 100 MeV to 100 GeV, one year of public Fermi Large Area Telescope (Fermi-LAT) data are also
Aleksić, J. et al.
Fecha de publicación:
11
2011