Ground-level particle detection is now a well-established approach to TeV γ-ray astronomy.
Detection of Cherenkov light produced in water-filled detection units is a proven and cost …

The presence of a spectral softening, occurring at∼ 3 PeV energies, seen in the local
cosmic-ray energy spectrum provides an evidence that our Galaxy hosts astrophysical …

The direct detection of primary gamma-rays is only possible with space-based detectors,
such as Fermi-LAT. However, the size and sensitivity limitations of satellite-borne detectors …

Dark matter is thought to make up most of the matter density of the Universe, yet its true
nature remains uncertain. Among dark matter theories, Weakly Interacting Massive Particles …

Ground-based γ-ray astronomy is a powerful tool to study cosmic-ray physics, providing a
diagnostic of the high-energy processes at work in the most extreme astrophysical …

Currently, one of the most profound mysteries in physics is the nature of dark matter
particles. Its existence is inferred through the gravitational effects it has on visible matter, but …

The Southern Wide-field Gamma-ray Observatory (SWGO) is the project to build a new
extensive air shower particle detector for the observation of very-high-energy gamma-rays in …

A new generation of high-energy gamma-ray detectors is being developed by the Southern
Wide-field Gamma-ray Observatory (SWGO)[1], which will operate in the energy range of …