activity
20242026
collaborators

10 papers

astro-ph.HE2026

Magnetic rigidity reveals the PeVatron acceleration region in SS 433

Jie Liao, Wancheng Xu, Lang Cui +10

PeVatrons are cosmic accelerators capable of driving particles to petaelectronvolt (PeV) energies. Recently, microquasar jets have emerged as compelling Galactic PeVatron candidate…

astro-ph.HE2026

FAST Discovery of Jy Radio Pulsations from PSR J2238+5903, Providing a DM Distance Anchor for the Candidate TeV Halo 1LHAASO J2238+5900

Jianli Zhang, Hui Zhu, Guanhong Lin +10

We report the first detection of radio pulsations from PSR J2238+5903, a gamma-ray pulsar spatially coincident with the extended TeV source 1LHAASO J2238+5900. Our 3000 s FAST L-ba…

astro-ph.HE2026

Searching for Spider-Like Pulsars from TESS Ellipsoidal Lightcurves with X-ray counterparts

Xiaoqing Liang, Partha Sarathi Pal, P. H. Thomas Tam +2

We present a search for new spider pulsar candidates through multi-wavelength cross-matching, including -ray, X-ray, and optical data. A search for sinusoidal-like optical modu…

astro-ph.HE2025

Ultrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems

The LHAASO Collaboration, Zhen Cao, Felix Aharonian +315

Black holes (BH), one of the most intriguing objects in the universe, can manifest themselves through electromagnetic radiation initiated by the accretion flow. Some stellar-mass B…

astro-ph.HE2025

Unsupervised machine learning classification of gamma-ray bursts based on the rest-frame prompt emission parameters

Si-Yuan Zhu, Lang Shao, Pak-Hin Thomas Tam +1

Gamma-ray bursts (GRBs) are generally believed to originate from two distinct progenitors, compact binary mergers and massive collapsars. Traditional and some recent machine learni…

astro-ph.HE2025

Identifying Merger-Driven Long Gamma-Ray Bursts based on Machine Learning

Si-Yuan Zhu, Hui-Ying Deng, Fu-Wen Zhang +2

Gamma-ray bursts (GRBs) are classified as Type I GRBs originated from compact binary mergers and Type II GRBs originated from massive collapsars. While Type I GRBs are typically sh…