Fig. 2.
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Left: Inner galaxy gamma-ray SEDs as a function of the energy for the DGE + cocoons contributions (golden band) and for the cocoons only (blue line). We rescale the predicted SEDs in order to account for the LHAASO mask in the galactic disc. Right: Same as left panel, but for the outer galaxy. In both panels, the gamma-ray SEDs are compared with Fermi-LAT and LHAASO data reported by LHAASO Collaboration (2025).
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