Fig. 9.

SED of HESS J1832−093: radio upper limits (yellow) (Condon et al. 1998; Helfand et al. 2006), IR (magenta) (Skrutskie et al. 2006), UV (green), X-rays (cian), HE (red), and VHE (blue) γ-rays (H.E.S.S. Collaboration 2015). In grey, SED from HESS J0632+057 is shown for comparison, including radio (Moldón et al. 2011), IR re-scaled a factor 10−3 (Skrutskie et al. 2006), X-ray (Hinton et al. 2009), and γ-rays (Li et al. 2017; Aharonian et al. 2007). In black, synchrotron and IC emission models for HESS J0632+057 with Emin of 1 GeV (solid), 10 GeV (dashed) and 100 GeV (dotted) (Hinton et al. 2009).
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