HAWC survey of Galactic supernova remnants provides TeV gamma-ray data to constrain cosmic-ray acceleration energies and emission mechanisms.
The 2HWC HAWC Observatory Gamma-Ray Catalog
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HAWC data extend the VHE gamma-ray spectrum of gamma Cygni SNR to higher energies, tightening constraints on the maximum particle acceleration energy.
citing papers explorer
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A Survey of TeV emission from Galactic Supernova Remnants with HAWC
HAWC survey of Galactic supernova remnants provides TeV gamma-ray data to constrain cosmic-ray acceleration energies and emission mechanisms.
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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.