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Fig. 7
Spectral energy distribution of the emission from PSR B1259–63/LS 2883 obtained with the Fermi-LAT and H.E.S.S. in CT5 mono mode during the HE gamma-ray flare in 2014, based on observations taken between tp + 44.2 d and tp + 52.2 d). Power laws are assumed for both data sets.
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