Fig. 4
Energy flux (1σ statistical error bars) for HESS J1801−204 and multiwavelength comparisons. Included is the Fermi-LAT GeV emission (Acero et al. 2015), VLA radio emission for G10.0−0.3 (Kulkarni et al. 1994), SGR 1806−20 X-ray unpulsed emission (powerlaw fits: 1. Beppo-SAX 21 Mar. 1999; 2. XMM-Newton 3 Apr. 2002; 3. XMM-Newton 6 Oct. 2004; and 4. INTEGRAL IBIS 2006/2007 from Esposito et al. 2007), and X-ray upper limit for LBV 1806−20 (Nazé et al. 2012).
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