activity
20072025
most citedThe energy spectrum of cosmic-ray electrons at TeV energies

638 citations · 12.1k across the 215 of their papers we have counts for

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Showing 2017 · astro-ph.HEShow all

10 papers · 2 filters

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★ 14 cited

On the expected -ray emission from nearby flaring stars

Stefan Ohm, Clemens Hoischen

Stellar flares have been extensively studied in soft X-rays (SXR) by basically every X-ray mission. Hard X-ray (HXR) emission from stellar superflares, however, have only been dete…

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★ 7 cited

First Results of Eta Car Observations with H.E.S.S.II

E. Leser, S. Ohm, M. Füßling +7

Eta Carinae (or Eta Car) is a colliding-wind binary that shows non-thermal emission from hard X-rays to high-energy -rays. The -ray spectrum exhibits two spectral components,…

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…