collaborators

7 papers

astro-ph.HE2026

The Very Late Time Afterglow of GW170817 Favors a Wobbling Jet

Hao Wang, Ore Gottlieb, Aman Katira +4

GW170817 remains the only binary neutron star merger detected through multimessenger emission. Its afterglow has been monitored for nearly a decade, offering an unprecedented oppor…

astro-ph.HE2025

{\tt RapidGBM}: An Efficient Tool for Fermi-GBM Visibility Checking and Data Analysis with a Case Study of EP240617a

Yun Wang, Jia Ren, Lu-Yao Jiang +15

We have developed a lightweight tool, {\tt RapidGBM}, featuring a web-based interface and capabilities of rapid calculation of Fermi Gamma-ray Burst Monitor (GBM) visibilities and…

astro-ph.HE2025

GRB 240825A: Early Reverse Shock and Its Physical Implications

Chao Wu, Yun Wang, Hua-Li Li +84

Early multiwavelength observations offer crucial insights into the nature of the relativistic jets responsible for gamma-ray bursts and their interaction with the surrounding mediu…

astro-ph.HE2025

Forward and Reverse Shock Emission from Relativistic Jets with Arbitrary Angular and Stratified Radial Profiles

Hao Wang, Hao Zhou, Yi-Zhong Fan +1

Gamma-ray bursts are expected to be generated by structured jets, whose profiles significantly impact their afterglow emission. Previously, we developed a numerical code jetsimpy,…

astro-ph.HE2025

A period-increasing oscillation signal in a long gamma-ray burst

Tian-Ci Zheng, Stefano Covino, Yun Wang +3

Gamma-ray bursts (GRBs), the brightest electromagnetic bursts in the universe, are believed to originate from ultra-relativistic jets launched by the rapidly rotating central engin…

astro-ph.HE2025

Leptohadronic Multimessenger Modeling of Two High-redshift (z 1) Neutrino Emission Blazar Candidates

Xiong Jiang, Neng-Hui Liao, Xue Rui +2

The blazars are one of the leading candidate sources of high-energy neutrinos. Recently, two blazars have been found to be temporally and spatially correlated with some IceCube hig…