D. Malyshev

TL;DR: In this article, the authors report on γ-ray observations of the Milky-Way satellite galaxies (dSphs) based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis.

TL;DR: The Fermi Large Area Telescope (LAT) has provided the most detailed view to date of the emission toward the Galactic center (GC) in high-energy gamma-rays as mentioned in this paper.

TL;DR: In this article, the authors analyzed 50 months of Fermi Large Area Telescope (LAT) data between 100 MeV and 500 GeV above 10 deg in Galactic latitude to derive the spectrum and morphology of two large structures in the gamma-ray sky extending to 55 deg below the Galactic center.

TL;DR: In this paper, the authors argue that the change in pulsed γ-ray emission is due to a change in emission beaming and speculate that it is precipitated by a shift in the magnetic field structure, leading to either effective magnetic inclination or effective current.

TL;DR: In this article, the authors used the substructure of the dark matter halo of a galaxy cluster and the cross sections for DM anniature signals to search for dark matter annihilation signals.