HAWC survey of Galactic supernova remnants provides TeV gamma-ray data to constrain cosmic-ray acceleration energies and emission mechanisms.
Discovery of very high energy gamma-ray emission coincident with molecular clouds in the W 28 (G6.4-0.1) field
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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.