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

863 citations · 1.5k across the 6 of their papers we have counts for

collaborators

6 papers

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…

astro-ph2006863 cited

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)…

astro-ph2006197 cited

First detection of a VHE gamma-ray spectral maximum from a Cosmic source: H.E.S.S. discovery of the Vela X nebula

Aharonian et al.

The Vela supernova remnant (SNR) is a complex region containing a number of sources of non-thermal radiation. The inner section of this SNR, within 2 degrees of the pulsar PSR B083…