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Fig. 3.

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SEDs of interesting candidates detected at GeV energies, namely M31 (upper panel), or on the verge of GeV detection, namely M33 (mid panel) and M83 (lower panel). The line and color codes match those of Fig. 2. The solid black line with arrows represents the upper bound on the expected γ-ray emission of each galaxy including the absorption on the EBL at multi-TeV energies.

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