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Fig. 8


Spectral energy distributions and lightcurves depending on inclination for our reference model. Top panels: thick black line is the average spectrum, thick coloured lines are the average INFC (dark blue) and SUPC (light blue) spectra (Sect. 4.4), thick dashed line shows the contribution of the back shock region to the average spectrum, thin grey lines show the spectral evolution with orbital phase. Bottom panels: VHE gamma-ray and X-ray lightcurves (thick solid lines). Again, the dashed line shows the back shock contribution. The thin grey line in the middle panels is the unabsorbed VHE flux.

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