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Fig. 2

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NGC 1275 spectral energy distribution measured by MAGIC between 70 GeV and 500 GeV (filled squares), together with the results above 100 MeV achieved from the first year (filled circles, Kataoka et al. 2010), and from the first two years (open circles, Brown & Adams 2011) of the Fermi-LAT all-sky-survey observations. The power-law fits to the Fermi-LAT data (extrapolated up to 1 TeV) are also shown, together with the exponential power-law fit provided in Kataoka et al. (2010).

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