Non-thermal particles and high-energy radiation can play a role in the dynamical processes
in star-forming regions and provide an important piece of the multiwavelength observational …

We present the results of the most comprehensive survey of the Galactic plane in very high-
energy (VHE) γ-rays, including a public release of Galactic sky maps, a catalog of VHE …

We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA)
to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray …

During the last 20 years, TeV astronomy has turned from a fledgling field, with only a handful
of sources, into a fully-developed astronomy discipline, broadening our knowledge on a …

We present the results of the most comprehensive survey of the Galactic plane in very high-
energy (VHE) gamma-rays, including a public release of Galactic sky maps, a catalog of …

Abstract The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project led by
the Italian National Institute for Astrophysics (INAF) is developing and will deploy at the …

Thermal Higgsino dark matter (DM), with a mass near 1.1 TeV, is one of the most well-
motivated and untested DM candidates. Leveraging recent hydrodynamic cosmological …

Aims. The identification of PeVatrons, hadronic particle accelerators reaching the knee of the
cosmic ray spectrum (few× 10 15 eV), is crucial to understand the origin of cosmic rays in the …

The observation of the diffuse Galactic gamma-ray flux is the most powerful tool to study
cosmic rays in different regions of the Galaxy, because the energy and angular distributions …

Aims. In the presence of a sufficient amount of target material, γ-rays can be used as a tracer
in the search for sources of Galactic cosmic rays (CRs). Here we present deep observations …