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 …

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting
views and insights from all disciplines involved—cosmology, astrophysics, nuclear, and …

The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark
matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs …

MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located in the
Canary island of La Palma, Spain. During summer 2011 and 2012 it underwent a series of …

The inner region of the Milky Way halo harbors a large amount of dark matter (DM). Given its
proximity, it is one of the most promising targets to look for DM. We report on a search for the …

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 …

Spectral lines are among the most powerful signatures for dark matter (DM) annihilation
searches in very-high-energy γ rays. The central region of the Milky Way halo is one of the …

The origin of the extragalactic γ-ray background (EGB) has been debated for some time. The
EGB comprises the γ-ray emission from resolved and unresolved extragalactic sources …

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 …

Dwarf spheroidal (dSph) galaxies are prime targets for present and future γ-ray telescopes
hunting for indirect signals of particle dark matter. The interpretation of the data requires …