collaborators

6 papers

astro-ph.CO2026

From Cosmic Web to Supernova Remnants: Modeling FRB DM to Trace Baryons across Multiple Scales

Zhao Joseph Zhang

Fast radio bursts (FRBs) provide a powerful probe of ionized baryons through their dispersion measures (DMs), but the observed signal contains contributions from the intergalactic…

astro-ph.HE2026

Radio Emission from Fast Blue Optical Transients Powered by Trans-relativistic Shocks in Confined Circumstellar Material

Liang-Duan Liu, Jia-Sen Zhang, Zhao-Sheng Zhang +1

Fast blue optical transients (FBOTs) are luminous, rapidly evolving explosions whose radio emission provides a sensitive probe of shock interaction and the circumstellar material (…

astro-ph.HE2026

Utilizing Dispersion Measure of Fast Radio Bursts to Probe the Intergalactic Medium Turbulence

Rui-Nan Li, Zhao Joseph Zhang, Kentaro Nagamine +3

Extragalactic fast radio bursts (FRBs) have emerged as powerful probes of turbulence within the intergalactic medium (IGM), a phenomenon that plays a crucial role in various cosmol…

astro-ph.CO2026

Probing the Cosmic Baryon Distribution and the Impact of Active Galactic Nuclei Feedback with Fast Radio Bursts in CROCODILE Simulation

Zhao Joseph Zhang, Kentaro Nagamine, Yuri Oku +6

We investigate the Missing Baryon problem using Fast Radio Bursts (FRBs) to trace cosmic baryons. Our CROCODILE simulations, performed with the GADGET3/4-OSAKA smoothed particle hy…

astro-ph.GA2025

Magnetic fields in galactic environments probed by Fast Radio Bursts

Ilya S. Khrykin, Nicolas Tejos, J. Xavier Prochaska +7

FRBs constitute a unique probe of various astrophysical and cosmological environments via their characteristic dispersion and rotation (RM) measures that encode information about t…

astro-ph.HE2025

Signature of a magnetar central engine with precession motion in the X-ray emission of GRB 220711B

Ying-Ze Shan, Xing Yang, Hou-Jun Lü +6

The -ray light curve of long-duration GRB 220711B, is characterized by a multi-peaked structure with a duration lasting 105 seconds. More interestingly, the X-ray aftergl…