Fig. 7
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Spectral energy distribution of the γ-ray emission within 1° radius of the Geminga pulsar. Spectra from two HAWC analyses of Geminga are shown for comparison (Abeysekara et al. 2017a,b), with flux normalisation scaled to match the sub-region from which the H.E.S.S. spectrum is extracted. Error bands include systematic uncertainties for H.E.S.S. but are statistical only for HAWC.
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