output
20032011
most citedObservations of the Crab Nebula with H.E.S.S

863 citations

Showing 2006Show all

59 papers · 1 filter

astro-ph2006189 cited

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…

hep-ph2006

Double spin azimuthal asymmetries A_{LT} and A_{LL} in semi-inclusive DIS

A. Kotzinian

Within the LO QCD parton model of SIDIS with unintegrated quark distribution and fragmentation functions we study the transverse momentum and azimuthal dependencies of the double s…

astro-ph200693 cited

MAGIC upper limits on the very high energy emission from GRBs

J. Albert, E. Aliu, H. Anderhub +57

The fast repositioning system of the MAGIC Telescope has allowed during its first data cycle, between 2005 and the beginning of year 2006, observing nine different GRBs as possible…

astro-ph2006342 cited

Fast variability of TeV gamma-rays from the radio galaxy M 87

HESS Collaboration, F. A. Aharonian

The detection of fast variations of the TeV (10^12 eV) gamma-ray flux, on time-scales of days, from the nearby radio galaxy M 87 is reported. These variations are ~10 times faster…

astro-ph20062 cited

Study on Cosmic Ray Background Rejection with a 30 m Stand-Alone IACT using Non-parametric Multivariate Methods in a sub-100 GeV Energy Range

A. Konopelko, A. Chilingarian, A. Reimers

During the last decade ground-based very high-energy gamma-ray astronomy achieved a remarkable advancement in the development of the observational technique for the registration an…

astro-ph2006328 cited

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…