activity
20062009
most citedObservations of the Crab Nebula with H.E.S.S

863 citations · 2.4k across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2009★ 59 cited

H.E.S.S. observations of gamma-ray bursts in 2003-2007

F. Aharonian

Very-high-energy (VHE; >~100 GeV) gamma-rays are expected from gamma-ray bursts (GRBs) in some scenarios. Exploring this photon energy regime is necessary for understanding the ene…

astro-ph2008★ 30 cited

Search for Gamma-rays from Dark Matter annihilations around Intermediate Mass Black Holes with the H.E.S.S. experiment

HESS Collaboration, F Aharonian, G. Bertone

The H.E.S.S. array of Cherenkov telescopes has performed, from 2004 to 2007, a survey of the inner Galactic plane at photon energies above 100 GeV. About 400 hours of data have bee…

astro-ph2008★ 80 cited

Exploring a SNR/Molecular Cloud Association Within HESS J1745-303

HESS Collaboration, F. Aharonian

HESS J1745-303 is an extended, unidentified VHE (very high energy) gamma-ray source discovered using HESS in the Galactic Plane Survey. Since no obvious counterpart has previously…

astro-ph2008★ 65 cited

Discovery of VHE gamma-rays from the high-frequency-peaked BL Lac object RGB J0152+017

HESS Collaboration, F. Aharonian

Aims: The BL Lac object RGB J0152+017 (z=0.080) was predicted to be a very high-energy (VHE; > 100 GeV) gamma-ray source, due to its high X-ray and radio fluxes. Our aim is to unde…

astro-ph2007★ 212 cited

HESS VHE Gamma-Ray Sources Without Identified Counterparts

HESS Collaboration, F. Aharonian

The detection of gamma rays in the very-high-energy (VHE) energy range (100 GeV--100 TeV) provides a direct view of the parent population of ultra-relativistic particles found in a…

astro-ph2007★ 40 cited

Upper Limits from HESS AGN Observations in 2005-2007

HESS Collaboration, F. Aharonian

AIMS: Very high energy (VHE; E>100 GeV) gamma-ray studies were performed for 18 active galactic nuclei (AGN) from a variety of AGN classes. METHODS: VHE observations of a sample of…