activity
20042026
most citedAn Exceptional VHE Gamma-Ray Flare of PKS 2155-304

816 citations · 12.3k across the 168 of their papers we have counts for

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35 papers · 1 filter

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★ 14 cited

Discovery of an X-ray nebula around PSR J1718-3825 and implications for the nature of the gamma-ray source HESS J1718-385

J. A. Hinton, S. Funk, S. Carrigan +5

Combined X-ray synchrotron and inverse-Compton gamma-ray observations of pulsar wind nebulae (PWN) may help to elucidate the processes of acceleration and energy loss in these syst…

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…