863 citations
- S. Funk4 profiles26 · h 89
- B. Giebels4 profiles24 · h 83
- C. Venter3 profiles24 · h 65
- G. Dubus2 profiles24 · h 64
- C. Boisson4 profiles23 · h 64
- D. Emmanoulopoulos4 profiles23 · h 37
- H. Sol4 profiles23 · h 62
- I. Büsching5 profiles23 · h 32
- M. Punch2 profiles23 · h 61
- M. Raue4 profiles23 · h 50
- R. Terrier2 profiles23 · h 68
- S. Pita4 profiles23 · h 60
- Max Planck Institute for Nuclear PhysicsDE25 papers
- Centre National de la Recherche ScientifiqueFR24 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR24 papers
- Laboratoire AstroParticule et CosmologieFR24 papers
- CEA Paris-SaclayFR23 papers
- École PolytechniqueFR23 papers
- Humboldt-Universität zu BerlinDE23 papers
- Institut de Planétologie et d'Astrophysique de GrenobleFR23 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR23 papers
- Laboratoire de Physique Nucléaire et de Hautes ÉnergiesFR23 papers
- Laboratoire de Physique ThéoriqueFR23 papers
- Laboratoire Leprince-RinguetFR23 papers
4 papers · 1 filter
Detection of Gamma Rays From a Starburst Galaxy
The HESS Collaboration, F. Acero
Starburst galaxies exhibit in their central regions a highly increased rate of supernovae, the remnants of which are thought to accelerate energetic cosmic rays up to energies of ~…
Unidentified Gamma-Ray Sources as Ancient Pulsar Wind Nebulae
O. C. de Jager, S. E. S. Ferreira, A. Djannati-Ataï +6
In this paper we explore the evolution of a PWN while the pulsar is spinning down. An MHD approach is used to simulate the evolution of a composite remnant. Particular attention is…
Simultaneous observations of PKS 2155-304 with H.E.S.S., Fermi, RXTE and ATOM: spectral energy distributions and variability in a low state
H. E. S. S., Fermi-LAT collaborations
We report on the first simultaneous observations that cover the optical, X-ray, and high energy gamma-ray bands of the BL Lac object PKS 2155-304. The gamma-ray bands were observed…
H.E.S.S. observations of gamma-ray bursts in 2003-2007
F. Aharonian
Very-high-energy (VHE; >~100 GeV) gamma-rays are expected from gamma-ray bursts (GRBs) in some scenarios. Exploring this photon energy regime is necessary for understanding the ene…