activity
20042009
most citedAn Exceptional VHE Gamma-Ray Flare of PKS 2155-304

816 citations · 5.1k across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.GA2009★ 132 cited

Spectrum and variability of the Galactic Center VHE gamma-ray source HESS J1745-290

H. E. S. S. collaboration, :, F. Aharonian

A detailed study of the spectrum and variability of the source HESS J1745-290 in the Galactic Center (GC) region using new data from the H.E.S.S. array of Cherenkov telescopes is p…

astro-ph2008★ 24 cited

Discovery of very-high-energy gamma-ray emission from the vicinity of PSR J1913+1011 with H.E.S.S

HESS Collaboration, F. Aharonian

The H.E.S.S. experiment, an array of four Imaging Atmospheric Cherenkov Telescopes with high sensitivity and large field-of-view, has been used to search for emitters of very-high-…

astro-ph2008★ 279 cited

Discovery of very high energy gamma-ray emission coincident with molecular clouds in the W28 (G6.4-0.1) field

HESS Collaboration, F Aharonian

We observed the W28 field (for ~40 h) at Very High Energy (VHE) gamma-ray energies (E>0.1 TeV) with the H.E.S.S. Cherenkov telescopes. A reanalysis of EGRET E>100 MeV data was also…

astro-ph2007★ 98 cited

Observations of the Sagittarius Dwarf galaxy by the H.E.S.S. experiment and search for a Dark Matter signal

HESS Collaboration, F. Aharonian

Observations of the Sagittarius dwarf spheroidal (Sgr dSph) galaxy were carried out with the H.E.S.S. array of four imaging air Cherenkov telescopes in June 2006. A total of 11 hou…

astro-ph2007★ 187 cited

HESS Observations and VLT Spectroscopy of PG 1553+113

HESS Collaboration, F. Aharonian

AIMS: The properties of the very high energy (VHE; E>100 GeV) gamma-ray emission from the high-frequency peaked BL Lac PG 1553+113 are investigated. An attempt is made to measure t…

astro-ph2007

H.E.S.S. observations of the supernova remnant RX J0852.0-4622

H. E. S. S. Collaboration, :, M. Lemoine-Goumard +4

The shell-type supernova remnant RX J0852.0-4622 was detected in 2004 and re-observed between December 2004 and May 2005 with the High Energy Stereoscopic System (H.E.S.S.), an arr…