activity
20162021
most citedContributions of the High Energy Stereoscopic System (H.E.S.S.) to the 35th International Cosmic Ray Conference (ICRC), Busan, Korea

10 citations · 14 across the 2 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

5 papers · 1 filter

astro-ph.HE2021★ 4 cited

HESS J1858+020: A GeV-TeV source possibly powered by CRs from SNR G35.6-0.4

Y. Cui, Y. Xin, S. Liu +3

Context: The supernova remnant (SNR) G35.6-0.4 shows a non-thermal radio shell, however, no γ-ray or X-ray counterparts have been found for it thus far. One TeV source, HESS J1858+…

astro-ph.HE2019

X-Ray spectral evolution of PSR~J2032+4127 during the 2017 periastron passage

Partha Sarathi Pal, P. H. Thomas Tam, Yudong Cui +3

We report X-ray data analysis results obtained from Chandra, XMM-Newton, NuSTAR and Swift observations of PSR J2032+4127 taken before, during, and after the periastron on 2017 Nove…

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.HE2016

A young SNR illuminating nearby Molecular Clouds with cosmic rays

Y. Cui, G. Pühlhofer, A. Santangelo

The Supernova Remnant (SNR) HESS J1731-347 displays strong non-thermal TeV gamma-ray and X-ray emission, thus the object is at present time accelerating particles to very high ener…

astro-ph.HE2016

Acceleration of petaelectronvolt protons in the Galactic Centre

H. E. S. S. collaboration, :, A. Abramowski +229

Galactic cosmic rays reach energies of at least a few Peta-electronvolts (1 PeV = electron volts). This implies our Galaxy contains PeV accelerators (PeVatrons), bu…