863 citations
- S. Funk4 profiles26 · h 89
- B. Giebels4 profiles25 · h 83
- C. Venter3 profiles25 · h 65
- G. Dubus2 profiles25 · h 64
- C. Boisson4 profiles24 · h 64
- H. Sol4 profiles24 · h 62
- M. Punch2 profiles24 · h 61
- M. Raue4 profiles24 · h 50
- R. Terrier2 profiles24 · h 68
- S. Pita4 profiles24 · h 60
- U. Schwanke7 profiles24 · h 63
- B. Degrange5 profiles23 · h 52
- Max Planck Institute for Nuclear PhysicsDE27 papers
- Centre National de la Recherche ScientifiqueFR26 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR26 papers
- Laboratoire AstroParticule et CosmologieFR26 papers
- CEA Paris-SaclayFR25 papers
- École PolytechniqueFR25 papers
- Humboldt-Universität zu BerlinDE25 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR25 papers
- Laboratoire de Physique Nucléaire et de Hautes ÉnergiesFR25 papers
- Laboratoire de Physique ThéoriqueFR25 papers
- Laboratoire Leprince-RinguetFR25 papers
- A. Alikhanyan National LaboratoryAM24 papers
10 papers · 2 filters
H.E.S.S. observations of the supernova remnant RX J0852.0-4622: shell-type morphology and spectrum of a widely extended VHE gamma-ray source
HESS Collaboration, F. A. Aharonian
The shell-type supernova remnant RX J0852.0-4622 was observed with the High Energy Stereoscopic System (H.E.S.S.) of Atmospheric Cherenkov Telescopes between December 2004 and May…
Primary particle acceleration above 100 TeV in the shell-type Supernova Remnant RX J1713.7-3946 with deep H.E.S.S. observations
The HESS Collaboration, F. Aharonian
We present deep H.E.S.S. observations of the supernova remnant (SNR) RX J1713.7-3946. Combining data of three years - from 2003 to 2005 - we obtain significantly increased statisti…
Discovery of Very High Energy Gamma-Ray Emission from the BL Lac Object H2356-309 with the H.E.S.S. Cherenkov Telescopes
Aharonian et al.
The extreme synchrotron BL Lac object H2356-309, located at a redshift of z = 0.165, was observed from June to December 2004 with a total exposure of approx. 40 h live-time with th…
Energy dependent gamma-ray morphology in the Pulsar wind nebula HESSJ1825-137
F. Aharonian
Detailed morphological and spatially resolved spectral studies reveal the very high-energy (VHE) gamma-ray aspects of this object with unprecedented precision. We confirm previous…
Observations of the Crab Nebula with H.E.S.S
The HESS Collaboration, F. Aharonian
The Crab nebula was observed with the H.E.S.S. stereoscopic Cherenkov-telescope array between October 2003 and January 2005 for a total of 22.9 hours (after data quality selection)…
Periodic Modulations in an X-ray Flare from Sagittarius A*
Guillaume Belanger, Regis Terrier, Okkie De Jager +2
We present the highly significant detection of a quasi-periodic flux modulation with a period of 22.2 min seen in the X-ray data of the Sgr A* flare of 2004 August 31. This flaring…