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A. Jacholkowska

Researcher at University of Montpellier

Publications -  178
Citations -  15181

A. Jacholkowska is an academic researcher from University of Montpellier. The author has contributed to research in topics: High Energy Stereoscopic System & Pulsar. The author has an hindex of 51, co-authored 176 publications receiving 14030 citations.

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The LHCb detector at the LHC

A. A. Alves, +889 more
TL;DR: The LHCb experiment is dedicated to precision measurements of CP violation and rare decays of B hadrons at the Large Hadron Collider (LHC) at CERN (Geneva).
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First result from the Alpha Magnetic Spectrometer on the International Space Station: precision measurement of the positron fraction in primary cosmic rays of 0.5-350 GeV.

M. Aguilar, +347 more
TL;DR: The very accurate data show that the positron fraction is steadily increasing from 10 to ∼ 250 GeV, but, from 20 to 250 GeV, the slope decreases by an order of magnitude, showing the existence of new physical phenomena.
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Electroweak measurements in electron positron collisions at W-boson-pair energies at LEP

S. Schael, +1675 more
- 30 Nov 2013 - 
TL;DR: In this paper, the results of the four LEP experiments were combined to determine fundamental properties of the W boson and the electroweak theory, including the branching fraction of W and the trilinear gauge-boson self-couplings.
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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.