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David Maurin

Researcher at University of Grenoble

Publications -  232
Citations -  19193

David Maurin is an academic researcher from University of Grenoble. The author has contributed to research in topics: Cosmic ray & Dark matter. The author has an hindex of 68, co-authored 215 publications receiving 17295 citations. Previous affiliations of David Maurin include Centre national de la recherche scientifique & Joseph Fourier University.

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Search for Dark Matter Annihilation Signals from the Fornax Galaxy Cluster with H.E.S.S

A. Abramowski, +196 more
TL;DR: In this paper, the authors derived upper limits on the velocity-weighted annihilation cross-section as a function of the dark matter particle mass for different DM particle models, such as those arising from Kaluza-Klein and supersymmetric models.
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A search for a dark matter annihilation signal toward the Canis Major overdensity with H.E.S.S.

Felix Aharonian, +160 more
TL;DR: In this article, a search for a dark matter (DM) annihilation signal into $\gamma$-rays toward the direction of the Canis Major (CMa) overdensity is presented.
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Dark matter in the classical dwarf spheroidal galaxies: a robust constraint on the astrophysical factor for gamma-ray flux calculations

TL;DR: A new analysis of the relative detectability of dark matter annihilation in the Milky Way's eight classical dwarf spheroidal (dSph) satellite galaxies is presented, using Markov-Chain Monte Carlo techniques to fit dark matter halo parameters to empirical velocity dispersion profiles via the spherical Jeans equation.
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γ -rays from annihilating dark matter in galaxy clusters: stacking versus single source analysis

TL;DR: In this article, the authors derived a new data-driven limit for the extra-galactic DM annihilation background Jextra-gal>JGal/5 and considered a source-stacking approach.
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CLUMPY v3: γ-ray and ν signals from dark matter at all scales

TL;DR: This version of the CLUMPY code includes the mean extragalactic signal with several pre-defined options and keywords related to cosmological parameters, mass functions for the dark matter structures, and γ -ray absorption up to high redshift.