Fig. E.1.
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Comparison of the γ-ray transmissivities of the diffuse emission for a uniform CR density model and the distribution according to Eq. (7). The Galactic latitude and longitude range is the same as in Fig. 5, with Galactic longitudes 25° ≤l ≤ 100° and Galactic latitudes with |b|≤5°, and the ISM density model is the one from Ferrière (1998) and Ferrière et al. (2007).
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