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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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Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with the Alpha Magnetic Spectrometer on the International Space Station

M. Aguilar, +253 more
TL;DR: The detailed rigidity dependence of the nitrogen flux spectral index is presented for the first time and it is found the spectral index rapidly hardens at high rigidities and becomes identical to the spectral indices of primary He, C, and O cosmic rays above ∼700 GV.
Posted Content

Les Houches 2011: Physics at TeV Colliders New Physics Working Group Report

Gustaaf Brooijmans, +143 more
TL;DR: The activities of the "New Physics" working group for the "Physics at TeV Colliders" workshop (Les Houches, France, 30 May-17 June, 2011) are described in this paper.
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Discovery of extended VHE γ-ray emission from the vicinity of the young massive stellar cluster Westerlund 1

A. Abramowski, +208 more
TL;DR: In this article, the detection of the degree-scale extended VHE gamma-ray source HESS J1646-458 was reported based on 45 hours of H.E.S. observations performed between 2004 and 2008.
Posted Content

A database of charged cosmic rays

TL;DR: A new online database and associated online tools ( data selection, data export, plots, etc.) for charged cosmic-ray measurements are given and new data can be submitted, providing the community with a collaborative tool to archive past and future cosmic-rays measurements.
Journal ArticleDOI

Discovery of Gamma-Ray emission from the shell-type supernova remnant RCW 86 with HESS

Felix Aharonian, +160 more
TL;DR: The shell-type supernova remnant (SNR RCW 86) was detected with a statistical significance of 8.5 sigma and is significantly more extended than the H.E.S. point spread function.