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J. P. Tavernet

Researcher at Pierre-and-Marie-Curie University

Publications -  25
Citations -  4617

J. P. Tavernet is an academic researcher from Pierre-and-Marie-Curie University. The author has contributed to research in topics: Cosmic ray & Meson. The author has an hindex of 15, co-authored 25 publications receiving 4352 citations.

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Design concepts for the Cherenkov Telescope Array CTA: An advanced facility for ground-based high-energy gamma-ray astronomy

Marcos Daniel Actis, +685 more
TL;DR: The ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes as mentioned in this paper, which is an international initiative to build the next generation instrument, with a factor of 5-10 improvement in sensitivity in the 100 GeV-10 TeV range and the extension to energies well below 100GeV and above 100 TeV.
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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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Search for neutral heavy leptons produced in Z decays

P. Abreu, +587 more
TL;DR: Weak isosinglet neutral heavy leptons (m) have been searched for using data collected by the DELPHI detector corresponding to 3:3 106 hadronic Z0 decays at LEP1.
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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.