activity
20042024
most citedH.E.S.S. Observations of PKS 2155-304

153 citations · 692 across the 9 of their papers we have counts for

collaborators
Showing 2005Show all

6 papers · 1 filter

astro-ph2005★ 71 cited

Observations of Selected AGN with H.E.S.S

F. Aharonian et al.

A sample of selected active galactic nuclei (AGN) was observed in 2003 and 2004 with the High Energy Stereoscopic System (H.E.S.S.), an array of imaging atmospheric-Cherenkov teles…

astro-ph2005★ 101 cited

Multi-wavelength observations of PKS 2155-304 with H.E.S.S

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

The High Energy Stereoscopic System (H.E.S.S.) has observed the high-frequency peaked BL Lac object PKS2155-304 in 2003 between October 19 and November 26 in Very High Energy (VHE)…

astro-ph2005★ 72 cited

Serendipitous discovery of the unidentified extended TeV gamma-ray source HESS J1303-631

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

The serendipitous discovery of an unidentified extended TeVgamma-ray source close to the galactic plane named HESS J1303-631 at a significance of 21 standard deviations is reported…

astro-ph2005★ 138 cited

Discovery of extended VHE gamma-ray emission from the asymmetric pulsar wind nebula in MSH 15-52 with H.E.S.S

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

The Supernova Remnant MSH 15-52 has been observed in very high energy (VHE) gamma-rays using the H.E.S.S. 4-telescope array located in Namibia. A gamma-ray signal is detected at th…

astro-ph2005★ 15 cited

Search for TeV emission from the region around PSR B1706-44 with the H.E.S.S. experiment

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

The region around PSR B1706-44 has been observed with the H.E.S.S. imaging atmospheric Cherenkov telescopes in 2003. No evidence for gamma-ray emission in the TeV range was found a…

astro-ph2005★ 139 cited

Very high energy gamma rays from the composite SNR G0.9+0.1

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

Very high energy (> 100 GeV) gamma-ray emission has been detected for the first time from the composite supernova remnant G0.9+0.1 using the H.E.S.S. instrument. The source is dete…