activity
20232026
most citedThe origin of very-high-energy gamma-rays from GRB 221009A: implications for reverse shock proton synchrotron emission

15 citations · 16 across the 10 of their papers we have counts for

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astro-ph.HE2026

Constraining Cosmic-Ray Acceleration and Escape in Middle-Aged Supernova Remnants with GeV-TeV Gamma-Ray Observations

Siyu Chen, Bing Theodore Zhang, Yi Xing +2

In this work, we perform a systematic, time-dependent study of the gamma-ray emission from four representative middle-aged SNRs (W51C, IC~443, W44, W28), incorporating both CRs wit…

astro-ph.HE2026

On the Physical Origins of Long Period Radio Transients

Yuanhong Qu, Bing Zhang

Long-period radio transients (LPRTs) are a rapidly growing class of coherent radio sources with periods ranging from minutes to hours, whose central engines and emission mechanisms…

astro-ph.HE2026

Resolving the 2024 Outburst of Magnetar 1E 1841-045 from its host Supernova Remnant with EP-FXT

Yu-Cong Fu, Lin Lin, Yu-Jia Zheng +11

The magnetar 1E 1841-045 exhibited a new active episode starting on August 20, 2024, marked by X-ray bursts and enhanced persistent emission. Using data from the Einstein Probe (EP…

astro-ph.HE2026

A Minimal Interpretation of the Galactic Cosmic-Ray Proton and Helium Spectra from GeV to PeV Energies

Felix Aharonian, Bing Theodore Zhang

High-precision measurements of the cosmic-ray (CR) proton and helium spectra have revealed significant deviations from a simple power law, characterized by multiple spectral featur…

astro-ph.HE2026

Physical origin of very-high-energy gamma rays from the low-luminosity active galactic nucleus NGC 4278 and implications for neutrino observations

Shilong Chen, Abhishek Das, B. Theodore Zhang +3

Relativistic jets in active galactic nuclei (AGNs) are known to accelerate particles to extreme energies, yet the physical origin of very-high-energy (VHE) emission from low-lumino…