collaborators

6 papers

astro-ph.HE2026

Gamma-Ray Emission from the Crab Pulsar: A 17-Year Fermi-LAT Reanalysis

Liancheng Zhou, Yun-Lu Gong, Jun Fang +1

We present a reanalysis of 17 years of Fermi Large Area Telescope (LAT) observations of the Crab pulsar obtained between 2008 August and 2025 August. Using monthly Jodrell Bank rad…

astro-ph.HE2025

A Giant Peanut-shaped Ultra-High-Energy Gamma-Ray Emitter Off the Galactic Plane

Zhen Cao, Felix Aharonian, Yunxiang Bai +312

Ultra-high-energy (UHE), exceeding 100 TeV (10^12 electronvolts), γ-rays manifests extreme particle acceleration in astrophysical sources. Recent observations by γ-ray telescopes…

astro-ph.HE2025

Kinetic Simulations of Particle Acceleration in Relativistic Perpendicular Electron-positron Shocks with Proton Admixture

Huan Yu, Qi Xia, Jun Fang

Particle acceleration in relativistic shocks of electron-positron plasmas with proton admixture is investigated through two-dimensional (2D) particle-in-cell (PIC) simulations. The…

astro-ph.HE2025

Particle Acceleration along Magnetic Fields as the Origin of Ear-like Structures in Supernova Remnants

Huan Yu, Jun Fang

The origin of ear-like structures with two opposite lobes extending from the shell of supernova remnants (SNRs) remains a subject of active debate, with proposed mechanisms ranging…

astro-ph.HE2025

Detection of the Extended -ray Emission around TeV source 1LHAASO J0249+6022 with Fermi-LAT

Gong Yunlu, Zhou Liancheng, Xia Qi +3

1LHAASO J0249+6022 is an extended very-high-energy gamma-ray source discovered by the Large High-Altitude Air Shower Observatory. Based on nearly 16.1 years of data from the Fermi…

astro-ph.HE2025

Multiband Nonthermal Radiative Properties of the Pulsar Wind Nebula CTB 87

Gong Yunlu, Zhou Liancheng, Xia Qi +3

The pulsar wind nebula CTB 87 (G74.9+1.2) is one of the sources emitting -rays with energies higher than 10 TeV, as measured by the Very Energetic Radiation Imaging Telescope A…