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E. Brion

Researcher at DSM

Publications -  49
Citations -  4844

E. Brion is an academic researcher from DSM. The author has contributed to research in topics: High Energy Stereoscopic System & Supernova remnant. The author has an hindex of 30, co-authored 40 publications receiving 4611 citations.

Papers
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An Exceptional Very High Energy Gamma-Ray Flare of PKS 2155-304

Felix Aharonian, +125 more
TL;DR: In this paper, the average flux observed during an extreme gamma-ray outburst is I(>200 GeV) = (1.72$\pm$$0.05_{\rm stat}
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Energy Spectrum of Cosmic-Ray Electrons at TeV Energies

Felix Aharonian, +155 more
TL;DR: In this measurement, the first of this type, the High Energy Stereoscopic System is able to extend the measurement of the electron spectrum beyond the range accessible to direct measurements, finding evidence for a substantial steepening in the energy spectrum above 600 GeV compared to lower energies.
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Primary particle acceleration above 100 TeV in the shell-type supernova remnant RX J1713.7-3946 with deep HESS observations

Felix Aharonian, +124 more
TL;DR: The combined gamma-ray image of the 2004 and 2005 data reveals the morphology of RX J1713.7-3946 with unprecedented precision, as well as significantly increased statistics and energy coverage as compared to earlier 2003 & 2004 results.
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Discovery of very high energy gamma-ray emission coincident with molecular clouds in the W 28 (G6.4-0.1) field

Felix Aharonian, +140 more
TL;DR: The W28 field was observed at Very High Energy (VHE) gamma-ray energies (E>0.1 TeV) with the H.E.S. Cherenkov telescopes to indicate a hadronic origin for HESSJ1801-233 and HessJ1800-240, and several cloud components in projection may contribute to the VHE emission.
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New constraints on the mid-IR EBL from the HESS discovery of VHE gamma-rays from 1ES 0229+200

Felix Aharonian, +143 more
TL;DR: In this paper, a very high energy (VHE: >100 GeV) γ-ray emission from the high-frequency peaked BL Lac 1ES 0229+200 was detected at the 6.6σ level in the HESS observations (41.8 h live time).