activity
20162026
most citedA very-high-energy component deep in the Gamma-ray Burst afterglow

274 citations · 2.1k across the 67 of their papers we have counts for

collaborators
Showing 2017Show all

7 papers · 1 filter

astro-ph.HE2017★ 64 cited

TeV gamma-ray observations of the binary neutron star merger GW170817 with H.E.S.S

H. E. S. S. Collaboration, :, H. Abdalla +250

We search for high-energy gamma-ray emission from the binary neutron star merger GW170817 with the H.E.S.S. Imaging Air Cherenkov Telescopes. The observations presented here have b…

astro-ph.HE2017★ 10 cited

Contributions of the High Energy Stereoscopic System (H.E.S.S.) to the 35th International Cosmic Ray Conference (ICRC), Busan, Korea

H. E. S. S. Collaboration, :, H. Abdalla +256

Index of H.E.S.S. conference proceedings to the 35th ICRC, Busan, Korea

astro-ph.HE2017★ 2 cited

Target of Opportunity Observations of Blazars with H.E.S.S

F. Schüssler, M. Seglar-Arroyo, M. Arrieta +13

The very-high-energy (VHE, E>100 GeV) extragalactic sky is dominated by blazars, a class of active galactic nuclei which show rapid variability at all wavelengths. Target of Opport…

astro-ph.HE2017★ 2 cited

H.E.S.S. observations following multi-messenger alerts in real-time

Fabian Schüssler, M. Backes, A. Balzer +12

The H.E.S.S. Imaging Air Cherenkov Telescope system is, due to its fast reaction time and its comparably low energy threshold, very well suited to perform follow-up observations of…

astro-ph.HE2017★ 74 cited

Characterising the VHE diffuse emission in the central 200 parsecs of our Galaxy with H.E.S.S

H. E. S. S. Collaboration, :, H. Abdalla +256

The diffuse very high-energy (VHE, > 100 GeV) gamma-ray emission observed in the central 200 pc of the Milky Way by H.E.S.S. was found to follow the dense matter distribution in th…

astro-ph.IM2017★ 5 cited

Gravitational wave alert follow-up strategy in the H.E.S.S. multi-messenger framework

M. Seglar-Arroyo, F. Schüssler

The H.E.S.S. high-energy gamma-ray observatory is member of the Virgo/LIGO electromagnetic follow-up effort since early 2014. Its capability for transient follow-up studies benefit…