activity
19982018
most citedAn Exceptional VHE Gamma-Ray Flare of PKS 2155-304

816 citations · 4.4k across the 39 of their papers we have counts for

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Showing 2008Show all

6 papers · 1 filter

astro-ph2008★ 62 cited

Very high energy gamma-ray observations of the galaxy clusters Abell 496 and Abell 85 with H.E.S.S

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

Aims: The nearby galaxy clusters Abell 496 and Abell 85 are studied in the very high energy (VHE, E > 100 GeV) band to investigate VHE cosmic rays (CRs) in this class of objects wh…

astro-ph2008★ 112 cited

Discovery of gamma-ray emission from the shell-type supernova remnant RCW 86 with H.E.S.S

HESS Collaboration, F. Aharonian

The shell-type supernova remnant (SNR) RCW 86, possibly associated with the historical supernova SN 185, with its relatively large size (about 40' in diameter) and the presence of…

astro-ph2008★ 34 cited

H.E.S.S. Observations of the Prompt and Afterglow Phases of GRB 060602B

HESS Collaboration, F. Aharonian

We report on the first completely simultaneous observation of a gamma-ray burst (GRB) using an array of Imaging Atmospheric Cherenkov Telescopes which is sensitive to photons in th…

astro-ph2008★ 33 cited

H.E.S.S. upper limits for Kepler's supernova remnant

HESS Collaboration, F. Aharonian

Observations of Kepler's supernova remnant (G4.5+6.8) with the H.E.S.S. telescope array in 2004 and 2005 with a total live time of 13 h are presented. Stereoscopic imaging of Chere…

astro-ph2008★ 46 cited

Chandra and H.E.S.S. observations of the Supernova Remnant CTB 37B

HESS Collaboration, F. Aharonian

The >100 GeV gamma-ray source, HESS J1713-381, apparently associated with the shell-type supernova remnant (SNR) CTB 37B, was discovered using H.E.S.S. in 2006. X-ray follow-up obs…

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…