The indirect detection of dark matter annihilation and decay using observations of photons,
charged cosmic rays and neutrinos offers a promising means of identifying the particle …

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 …

We present the first joint analysis of gamma-ray data from the MAGIC Cherenkov telescopes
and the Fermi Large Area Telescope (LAT) to search for gamma-ray signals from dark matter …

The dwarf spheroidal satellite galaxies of the Milky Way are some of the most dark-matter-
dominated objects known. Due to their proximity, high dark matter content, and lack of …

Gamma-ray searches for dark matter annihilation and decay in dwarf galaxies rely on an
understanding of the dark matter density profiles of these systems. Conversely, uncertainties …

Utilizing the Fermi measurement of the γ-ray spectrum toward the Inner Galaxy, we derive
some of the strongest constraints to date on the dark matter (DM) lifetime in the mass range …

The majority of the matter in the universe is still unidentified and under investigation by both
direct and indirect means. Many experiments searching for the recoil of dark-matter particles …

The current standard model of cosmology (SMoC) requires The Dual Dwarf Galaxy Theorem
to be true according to which two types of dwarf galaxies must exist: primordial dark-matter …

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 …

Abstract The High Altitude Water Cherenkov (HAWC) observatory is an array of large water
Cherenkov detectors sensitive to gamma rays and hadronic cosmic rays in the energy band …