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Fig. 3


Photon yields arising in the γ-ray model for the best-fit to the data in the 0.25–63 GeV band on a 0. °25 grid, from the H I and CO phases of the North Rim (EriN), South Loop (EriS), East Shell (EriE), West Rim (EriW), MBM 20, Cetus and Taurus, Eridu cirrus, Main Taurus and Galactic disc clouds, from the DNM gas column density, from the Hα template (HII), from the γ-ray point sources, from the Sun and Moon emissions (SM), from the isotropic background (iso) and from the Galactic IC emission.

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