"PeVatrons" refer to astrophysical sources capable of accelerating particles to energies $\\sim$PeV and higher, potentially contributing to the cosmic r...
Galactic PeVatrons are astrophysical sources accelerating particles up to a few PeV ($\\sim$10$^{15}$ eV) energies. The primary signature of 100 TeV $\\...
<italic>Context.</italic> Recently, HAWC, AS<italic>γ</italic>, and LHAASO experiments have reported the gamma-ray spectrum of supernova remnant (SNR) ...
We suggest a concept fora novel wide-angle imaging detector for gamma-rays with energies inthe largely unexplored range between 10 TeV and several PeV...
We present the first catalog of gamma-ray sources emitting above 56 and 100 TeV with data from the High Altitude Water Cherenkov Observatory, a wide field-of-view observatory capable of detecting gamma rays up to a few hundred TeV. Ni...
Remarkable improvements inthe sensitivity and image resolution ofγ-ray sky surveys provided by the current generation of ground-based particle detecti...
Several gamma-ray observatories have discovered photons of cosmic origin with energies inthe PeV (1015eV) range. Photons at these energies might be pro...
We present the detection of VHE gamma-ray emission above 100 TeV from HAWCJ2227+610 with theHAWC observatory. Combining our observations with previous...