Fig. 3
Light curves of the Geminga pulsar obtained with MAGIC for different energy bins. From top to bottom: above 50 GeV, 50–100 GeV and 100–200 GeV. Two cycles are plotted for clarity. The bin width corresponds to ~10.8 ms (1/22 of the Geminga rotational period). The shaded brown areas show the positions of P1 (main pulse) and P2 (interpulse). The gray area shows the off-region. The dashed red line represents the averaged number of events in the background region.
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