activity
20132026
most citedA very-high-energy component deep in the Gamma-ray Burst afterglow

274 citations · 2.5k across the 118 of their papers we have counts for

collaborators
Showing 2017Show all

6 papers · 1 filter

astro-ph.HE2017★ 64 cited

TeV gamma-ray observations of the binary neutron star merger GW170817 with H.E.S.S

H. E. S. S. Collaboration, :, H. Abdalla +250

We search for high-energy gamma-ray emission from the binary neutron star merger GW170817 with the H.E.S.S. Imaging Air Cherenkov Telescopes. The observations presented here have b…

astro-ph.HE2017★ 3 cited

Cherenkov Telescope Array Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

F. Acero, B. S. Acharya, V. Acín Portella +1137

List of contributions from the Cherenkov Telescope Array Consortium presented at the 35th International Cosmic Ray Conference, July 12-20 2017, Busan, Korea.

astro-ph.HE2017★ 3 cited

Observations of the Pulsar Wind Nebula HESS J1825-137 with H.E.S.S. II

A. M. W. Mitchell, S. Caroff, R. D. Parsons +3

We present a new and deep analysis of the pulsar wind nebula (PWN) HESS\,J1825--137 with a comprehensive data set of almost 400 hours taken with the H.E.S.S. array between 2004 and…

astro-ph.HE2017★ 3 cited

The Vela X pulsar wind nebula through the eyes of H.E.S.S. and Suzaku

L. Tibaldo, F. Aharonian, P. Bordas +5

Pulsar wind nebulae (PWNe) are among the most extreme particle accelerators in galaxies, are recognized as multi-TeV electron/positron sources, and are one of the dominant classes…

astro-ph.HE2017★ 108 cited

Indications for a high-rigidity break in the cosmic-ray diffusion coefficient

Yoann Genolini, Pasquale D. Serpico, Mathieu Boudaud +9

Using cosmic-ray boron to carbon ratio (B/C) data recently released by the AMS-02 experiment, we find tantalizing indications ({\it decisive evidence}, in Bayesian terms) in favor…

astro-ph.HE2017★ 12 cited

Precision measurement of the (e + e) flux in primary cosmic rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station

Manuela Vecchi

We present a precise measurement of the combined electron plus positron flux from 0.5 GeV to 1 TeV, based on the analysis of the data collected by the Alpha Magnetic Spectrometer d…