For nearly a century, more mass has been measured in galaxies than is contained in the
luminous stars and gas. Through continual advances in observations and theory, it has …

Weakly interacting massive particles (WIMPs) remain a prime candidate for the cosmological
dark matter (DM), even in the absence of current collider signals that would unambiguously …

INTRODUCTION Neutrinos are tracers of cosmic-ray acceleration: electrically neutral and
traveling at nearly the speed of light, they can escape the densest environments and may be …

We present the first catalog of TeV gamma-ray sources realized with data from the newly
completed High Altitude Water Cherenkov Observatory (HAWC). It is the most sensitive wide …

Ground-based gamma-ray astronomy has had a major breakthrough with the impressive
results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground …

Composition and spectra of Galactic cosmic rays (CRs) are vital for studies of high-energy
processes in a variety of environments and on different scales, for interpretation of γ-ray and …

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

We present constraints on the annihilation cross section of weakly interacting massive
particles dark matter based on the joint statistical analysis of four dwarf galaxies with …

We report the detection of pulsed gamma rays from the Crab pulsar at energies above 100
giga–electron volts (GeV) with the Very Energetic Radiation Imaging Telescope Array …

The high demands of modern experiments in fast waveform digitizing led to the development
of a whole family of switched capacitor arrays (SCA), called the Domino Ring Sampler …