activity
19972026
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 14.2k across the 232 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.HEShow all

9 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★ 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

The modeling of the Vela pulsar pulses - from optical to hard gamma-ray energy

Bronisław Rudak, Jarosław Dyks

The pulsed radiation from PSR B0833-45 (Vela) has a phased-averaged spectral energy distribution (SED) of an apparently simple structure across a wide energy range, from optical li…

astro-ph.HE2017★ 20 cited

The first detection of a pulsar with ALMA

Roberto P. Mignani, Rosita Paladino, Bronek Rudak +8

Pulsars are neutron stars, stellar corpses left over after supernova explosions of stars about ten times as massive as our Sun, with densities comparable to the atomic nucleus', sp…

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.HE2017★ 82 cited

A polarized fast radio burst at low Galactic latitude

E. Petroff, S. Burke-Spolaor, E. F. Keane +35

We report on the discovery of a new fast radio burst, FRB 150215, with the Parkes radio telescope on 2015 February 15. The burst was detected in real time with a dispersion measure…