activity
20062009
most citedObservations of the Crab Nebula with H.E.S.S

863 citations · 2.1k across the 11 of their papers we have counts for

collaborators
Showing astro-phShow all

9 papers · 1 filter

astro-ph200880 cited

Exploring a SNR/Molecular Cloud Association Within HESS J1745-303

HESS Collaboration, F. Aharonian

HESS J1745-303 is an extended, unidentified VHE (very high energy) gamma-ray source discovered using HESS in the Galactic Plane Survey. Since no obvious counterpart has previously…

astro-ph2007212 cited

HESS VHE Gamma-Ray Sources Without Identified Counterparts

HESS Collaboration, F. Aharonian

The detection of gamma rays in the very-high-energy (VHE) energy range (100 GeV--100 TeV) provides a direct view of the parent population of ultra-relativistic particles found in a…

astro-ph2007114 cited

Detection of extended very-high-energy gamma-ray emission towards the young stellar cluster Westerlund 2

HESS Collaboration, F. Aharonian

Results from gamma-ray observations by the H.E.S.S. telescope array in the direction of the young stellar cluster Westerlund 2 are presented. Stereoscopic imaging of Cherenkov ligh…

astro-ph200764 cited

First ground based measurement of atmospheric Cherenkov light from cosmic rays

HESS Collaboration, F. A. Aharonian

A recently proposed novel technique for the detection of cosmic rays with arrays of Imaging Atmospheric Cherenkov Telescopes is applied to data from the High Energy Stereoscopic Sy…

astro-ph200666 cited

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…

astro-ph2006188 cited

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…