activity
20012010
most citedObservations of the Crab Nebula with H.E.S.S

863 citations · 1.4k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2010★ 40 cited

Discovery of VHE -ray emission from the SNR G54.1+0.3

V. A. Acciari, E. Aliu, T. Arlen +79

We report the discovery of very high energy gamma-ray emission from the direction of the SNR G54.1+0.3 using the VERITAS ground-based gamma-ray observatory. The TeV signal has an o…

astro-ph2008

Galactic Compact Objects Section of the White Paper on the Status and Future of Ground-based TeV Gamma-ray Astronomy

P. Kaaret, A. A. Abdo, J. Arons +22

This is a report on the findings of the Galactic compact objects working group for the white paper on the status and future of TeV gamma-ray astronomy. The white paper is an APS co…

astro-ph2007★ 64 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-ph2006★ 66 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-ph2006★ 188 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-ph2006★ 863 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)…