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Fig. 1


New TS map in the region of SNR Kes 41 generated in the 0.5–400 GeV energy band according to the last update on this source analysed in this work. Contours delineate the radio emission at 843 MHz from SUMSS at levels 0.09, 0.3, 0.5, and 0.7 Jy beam−1. Labels correspond to Kes 41 and the neighbouring HII regions (1:G337.711 −0.056; 2:G337.711+0.089; 3:G337.622−0.067; 4:G337.667−0.167; 5:G337.978−0.144; 6:G338.011+0.022; 7:G337.686+0.137; 8:G338.114 −0.193; Jones & Dickey 2012). The ellipse E1 is the area employed in Supan et al. (2018) to derive the properties of the interstellar medium, used to place constraints on the spectral fitting procedure presented in this work. Further details of the Kes 41 environment are presented in Supan et al. (2018).

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