Fig. 6

Spectral evolution (18.5 min snapshots) during the imposed flaring scenario of 1 ES 1011+496 (intrinsic spectrum). The VHE peak rises with the synchrotron peak because of the enhanced seed photons for hadronic interactions and the redistribution via γγ → e±. The inset shows the second, orphan flare in the gamma rays (see also Fig. 5) due to enhanced proton synchrotron radiation occurring with a delay, since the protons need time to accelerate to high energies.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.