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Fig. 2


Top: γ-ray counts of gaseous origin recorded in the 0.25-63 GeV band in a 0. °25 pixel grid. γ-ray emissions other than due to CR interactions with the gas were subtracted. Middle: dust optical depth measured at 353 GHz and displayed at the Fermi -LAT angular resolution for comparison. Bottom: dust optical depth measured at 353 GHz at its original resolution of 5′.

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