activity
20112022
most citedTeV gamma-ray observations of the binary neutron star merger GW170817 with H.E.S.S

64 citations · 408 across the 16 of their papers we have counts for

collaborators

38 papers

astro-ph.HE2022

A PeVatron Candidate: Modelling the Boomerang Nebula in X-ray Band

Xuan-Han Liang, Chao-Ming Li, Qi-Zuo Wu +2

Pulsar wind nebula (PWN) Boomerang and the associated supernova remnant (SNR) G106.3+2.7 are among candidates for the ultra-high-energy (UHE) gamma-ray counterparts published by LH…

astro-ph.HE2022

A semi-analytical solution to the forward-reverse shock hydrodynamics of the gamma-ray burst afterglow

Ze-Lin Zhang, Ruo-Yu Liu, Jin-Jun Geng +2

We extend the standard model of forward-reverse shock (FS-RS) for gamma-ray burst (GRB) afterglow to more general cases. On one hand, we derive the analytical solution to the hydro…

astro-ph.HE20222 cited

Constraining the baryon loading factor of AGN jets: implication from the gamma-ray emission of the Coma cluster

Xin-Yue Shi, Yi Zhang, Ruo-Yu Liu +1

High-energy cosmic rays (CRs) can be accelerated in the relativistic jets of Active Galactic Nuclei (AGNs) powered by supermassive black holes. The baryon loading efficiency onto r…

astro-ph.HE202129 cited

Origin of Galactic sub-PeV diffuse gamma-ray emission: Constraints from high-energy neutrino observations

Ruo-Yu Liu, Xiang-Yu Wang

Very recently, diffuse gamma rays with have been discovered from the Galactic disk by the Tibet air shower array and muon detector array (Tibet AS+M…

astro-ph.HE202121 cited

Particle acceleration in shearing flows: the case for large-scale jets

Jie-Shuang Wang, Brian Reville, Ruo-Yu Liu +2

X-ray observations of kilo-parsec scale jets indicate that a synchrotron origin of the sustained non-thermal emission is likely. This requires distributed acceleration of electrons…

astro-ph.HE2021

Investigating the nature of MGRO J1908+06 with multiwavelength observations

Jian Li, Ruo-Yu Liu, Emma de Ona Wilhelmi +7

The unidentified TeV source MGRO J1908+06, with emission extending from hundreds of GeV to beyond 100TeV, is one of the most intriguing sources in the Galactic plane. MGRO J1908+06…