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Fig. 3


Top: γ-ray counts of gaseous origin recorded in the 0.4–100 GeV energy band in a 0. °125 pixel grid. γ-ray emissions other than due to cosmic-ray interactions in the gas have been subtracted. The map has been smoothed with a Gaussian kernel of 0. °14 dispersion for display. Bottom: stellar reddening by dust displayed at the Fermi-LAT angular resolution for comparison.

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