activity
20232026
most citedMultiwavelength Afterglow Analysis of GRB 221009A: Unveiling the Evolution of a Cooling Break in a Wind-like Medium

5 citations · 7 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2026

Einstein Probe Fast X-ray Transients Extend the Physical Parameter Space of Relativistic Jets

Connery Chen, Yihan Wang, Bing Zhang

Fast X-ray Transients (FXTs) detected by the Einstein Probe (EP) mission possess exceptionally low spectral peak energies compared to typical long (Type II) GRBs. Some of these ext…

astro-ph.HE2026

Early results from the SVOM Observatory Science program

A. Coleiro, L. Tao, F. Cangemi +44

We present the organisation and early results from the Observatory Science program of the Space-based multi-band astronomical Variable Objects Monitor (SVOM), based on data collect…

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

VegasAfterglow: A High-Performance Framework for Gamma-Ray Burst Afterglows

Yihan Wang, Connery Chen, Bing Zhang

Gamma-ray bursts (GRBs) are the most luminous astrophysical transients, known to be associated with core collapse of massive stars or mergers of two compact objects such as two neu…

astro-ph.HE2024★ 5 cited

Multiwavelength Afterglow Analysis of GRB 221009A: Unveiling the Evolution of a Cooling Break in a Wind-like Medium

Donggeun Tak, Z. Lucas Uhm, Gregory S. H. Paek +8

Gamma-ray bursts (GRBs) are the most energetic explosions in the universe, and their afterglow emission provides an opportunity to probe the physics of relativistic shock waves in…

astro-ph.HE2023★ 2 cited

Evidence of Hadronic Emission from the brightest-of-all-time GRB 221009A

Kai Wang, Qing-Wen Tang, Yan-Qiu Zhang +4

Acceleration of hadrons in relativistic shocks has been long expected and invoked to model GRB high-energy photon and neutrino emissions. However, so far there has been no direct o…