Fig. 2

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CRe spectra in the Magellanic Clouds. The curves are the secondary spectra (dashed), primary spectra (dotted), and the primaries’ local PL representations (solid). In each panel the normalization of the primary CRe spectrum to its PL counterpart is chosen such that they nearly overlap. The primary CRe injection indices, qi, are 2.28 (SMC) and 2.23 (LMC). The two LMC CRe spectra panels refer, respectively, to the T+17 and A+16 Fermi/LAT datasets, as secondary spectra are derived from the pionic fits to the γ-ray data.
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