activity
20022020
most citedCharacterising the VHE diffuse emission in the central 200 parsecs of our Galaxy with H.E.S.S

74 citations · 380 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2020★ 50 cited

Monitoring of the radio galaxy M87 during a low emission state from 2012 to 2015 with MAGIC

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +188

M87 is one of the closest (z=0.00436) extragalactic sources emitting at very-high-energies (VHE, E > 100 GeV). The aim of this work is to locate the region of the VHE gamma-ray emi…

astro-ph.HE2018★ 5 cited

Decomposing blazar spectra into lepto-hadronic emission components

A. Gokus, S. Richter, F. Spanier +4

Recently reported coincidences between high-energy neutrino events and major blazar outbursts reinforce the relevance of lepto-hadronic emission models for blazars. We study the in…

astro-ph.HE2018

AGN Neutrino flux estimates for a realistic hybrid model

S. Richter, F. Spanier

Recent reports of possible correlations between high energy neutrinos observed by IceCube and Active Galactic Nuclei (AGN) activity sparked a burst of publications that attempt to…

astro-ph.HE2018★ 49 cited

A search for new supernova remnant shells in the Galactic plane with H.E.S.S

H. E. S. S. Collaboration, :, H. Abdalla +263

A search for new supernova remnants (SNRs) has been conducted using TeV gamma-ray data from the H.E.S.S. Galactic plane survey. As an identification criterion, shell morphologies t…

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★ 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…