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Fig. 2.

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Average spectrum of the γ-ray diffuse emission along the galactic plane (|b|< 5°) compared with Fermi-LAT data in three longitude intervals. The “Sources” component comprises the sources included in the 4FGL Fermi Catalog as well as unresolved sources and the interstellar galactic background light (IGB) component comprises the extra-galactic background light and Fermi’s instrumental background.

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