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Fig. 7


Spectral evolution (43.2 min snapshots) during the imposed flaring scenario by setting xe = 2.5 in the leptonic case of 1 ES 1011+496 (intrinsic spectrum). The SSC limit shows the simple flaring behaviour as expected, without spectral evolution in the VHE and orphan flares do not occur. The inset shows the corresponding lightcurves in the X-rays and gamma rays exhibiting a slight delay caused by the IC upscattering of the enhanced synchrotron photons.

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