activity
20012015
most citedAn Exceptional VHE Gamma-Ray Flare of PKS 2155-304

816 citations · 6.9k across the 54 of their papers we have counts for

collaborators

53 papers

astro-ph.HE2015★ 17 cited

Observations of the Crab Nebula with H.E.S.S. Phase II

M. Holler, D. Berge, C. van Eldik +7

The High Energy Stereoscopic System (H.E.S.S.) phase I instrument was an array of four mirror area Imaging Atmospheric Cherenkov Telescopes (IACTs) that has ver…

astro-ph.HE2014★ 7 cited

The Contribution of Millisecond Pulsars to the Galactic Cosmic-Ray Lepton Spectrum

C. Venter, A. Kopp, P. L. Gonthier +2

Pulsars are believed to be sources of relativistic electrons and positrons. The abundance of detections of gamma-ray millisecond pulsars by Fermi Large Area Telescope coupled with…

astro-ph.HE2013

The Discrepancy in Modelling of Galactic Cosmic Ray Primaries and Secondaries

D. Bisschoff, I. Büsching, M. S. Potgieter

Given that the bulk of the galactic cosmic rays (CRs) originates from transient point-like sources, such as supernova remnants, the flux of the CR primary component measured at Ear…

astro-ph.HE2012★ 64 cited

Anisotropic diffusion of galactic cosmic ray protons and their steady-state azimuthal distribution

Frederic Effenberger, Horst Fichtner, Klaus Scherer +1

Galactic transport models for cosmic rays involve the diffusive motion of these particles in the interstellar medium. Due to the large-scale structured galactic magnetic field this…

astro-ph.HE2012★ 84 cited

Spectral analysis and interpretation of the γ-ray emission from the Starburst galaxy NGC 253

H. E. S. S. Collaboration, A. Abramowski, F. Acero +192

Very-high-energy (VHE; E >100 GeV) and high-energy (HE; 100 MeV < E < 100 GeV) data from γ-ray observations performed with the H.E.S.S. telescope array and the Fermi-LAT instrument…

astro-ph.HE2012★ 85 cited

Search for Dark Matter Annihilation Signals from the Fornax Galaxy Cluster with H.E.S.S

HESS Collaboration, A. Abramowski, F. Acero +195

The Fornax galaxy cluster was observed with the High Energy Stereoscopic System (H.E.S.S.) for a total live time of 14.5 hours, searching for very-high-energy (VHE, E>100 GeV) gamm…