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Photohadronic scenario in interpreting the February-March 2014 flare of 1ES 1011+496
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Photohadronic scenario in interpreting the February-March 2014 flare of 1ES 1011+496
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The extraordinary multi-TeV flare from 1ES 1011 +496 during February-March 2014 was observed by MAGIC telescopes for 17 nights and the average spectrum of the whole period has a non-trivial shape. We have used the photohadronic model and a template EBL model to explain the average spectrum which fits well to the flare data. The spectral index $\alpha$ is the only free parameter in our model. We have also shown that the non-trivial nature of the spectrum is due to the change in the behavior of the optical depth above $\sim 600$ GeV $\gamma$-ray energy accompanied with the high SSC flux.
Forward citations
Cited by 1 Pith paper
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Multi-TeV flaring in nearby High Energy Blazars: A photohadronic scenario
Review applies the photohadronic model with EBL corrections to explain multi-TeV flaring in three nearby blazars.
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