Fig. B.1
Differential energy spectra of the Crab nebula from Aharonian et al. (2006, red-dashed line with red-diamond markers) and from this work (TBS; blue-circle markers and blue line indicating the best-fit spectrum). The spectrum above 10 TeV could not be shown and therefore the spectra were truncated at this energy. See text in Sect. 4 and Appendix B for further information.
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