Comparison between the LS 5039 model (Fig. 11) and the observed lightcurves. The model 10−30 MeV and 1−10 keV lightcurves were multiplied by a factor 10 and 2, respectively, to match the observations in Takahashi et al. (2009), Collmar & Zhang (2014). The grey lightcurve in the 0.1−10 GeV and 10−30 MeV panels represents the contribution from the relativistic Maxwellian component. The VHE and HE gamma-ray lightcurves are taken from Aharonian et al. (2006) and Abdo et al. (2009), respectively.
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