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The extraordinary multi-TeV flare from 1ES 1011 +496 during February-March2014 was observed by MAGIC telescopes for 17 nights and the average spectrum ofthe whole period has a non-trivial shape. We have used the photohadronic modeland a template EBL model to explain the average spectrum which fits well to theflare data. The spectral index $\alpha$ is the only free parameter in ourmodel. We have also shown that the non-trivial nature of the spectrum is due tothe change in the behavior of the optical depth above $\sim 600$ GeV$\gamma$-ray energy accompanied with the high SSC flux.

Photohadronic scenario in interpreting the February-March 2014 flare of 1ES 1011+496