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tokens: We thank A. Strong and T. Porter for advice regarding the details of the GALPROP ISRF model used in this paper. We also thank A. M. Stutz, Y. L. Shirley, J. Steinacker, and E. Keto for helpful discussions and comments on the paper draft. The work of J.K. and S.E.R. was supported by the Deutsche Forschungsgemeinschaft priority program 1573 (“Physics of the Interstellar Medium”). H.L. and M.N. were funded by the Deutsches Zentrum für Luft- und Raumfahrt (DLR). PACS has been developed by a consortium of institutes led by MPE (Germany), including UVIE (Austria); KU Leuven, CSL, IMEC (Belgium); CEA, LAM (France); MPIA (Germany); INAF-IFSI/OAA/OAP/OAT, LENS, SISSA (Italy); IAC (Spain). This development has been supported by the funding agencies BMVIT (Austria), ESA-PRODEX (Belgium), CEA/CNES (France), DLR (Germany), ASI/INAF (Italy), and CICYT/MCYT (Spain).