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B. Degrange

Researcher at École Polytechnique

Publications -  269
Citations -  23601

B. Degrange is an academic researcher from École Polytechnique. The author has contributed to research in topics: High Energy Stereoscopic System & Blazar. The author has an hindex of 76, co-authored 268 publications receiving 22350 citations. Previous affiliations of B. Degrange include Centre national de la recherche scientifique & Purdue University.

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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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Observations of the Crab nebula with HESS

Felix Aharonian, +106 more
TL;DR: In this paper, the Crab nebula was observed with the H.E.S. stereoscopic Cherenkov-telescope array between 2003 and 2005 for a total of 22.9 hours (after data quality selection).
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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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A low level of extragalactic background light as revealed by gamma-rays from blazars.

Felix Aharonian, +102 more
- 20 Apr 2006 - 
TL;DR: In this paper, an alternative approach is proposed based on the detection and identification of EBL absorption features in high-energy spectra of objects of known redshift, which provides the most stringent upper limit to date on the EBL in the Opt-NIR band, which appears significantly lower than expected from the current direct estimates and very close to the absolute lower limit represented by the integrated light of resolved galaxies.
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The H.E.S.S. Survey of the Inner Galaxy in Very High Energy Gamma Rays

Felix Aharonian, +103 more
TL;DR: The distribution in Galactic latitude of the detected sources appears to be consistent with a scale height in the Galactic disk for the parent population smaller than 100 pc, consistent with expectations for supernova remnants and/or pulsar wind nebulae.