HAWC data extend the VHE gamma-ray spectrum of gamma Cygni SNR to higher energies, tightening constraints on the maximum particle acceleration energy.
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Modeling the non-thermal emission of the gamma Cygni Supernova Remnant up to the highest energies
HAWC data extend the VHE gamma-ray spectrum of gamma Cygni SNR to higher energies, tightening constraints on the maximum particle acceleration energy.