activity
20032026
most citedOptical Flashes and Very Early Afterglows in Wind Environments

110 citations · 443 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2026

FAST Polarization Catalog of FRB 20240114A

Tian-Cong Wang, Jun-Shuo Zhang, Xiao-Hui Liu +60

Polarization measurements of fast radio bursts (FRBs) probe the magnetized plasma surrounding their central engines. FRB~20240114A is an exceptionally active repeating source, with…

astro-ph.HE2024★ 34 cited

Triggering the Untriggered: The First Einstein Probe-Detected Gamma-Ray Burst 240219A and Its Implications

Yi-Han Iris Yin, Bin-Bin Zhang, Jun Yang +49

The Einstein Probe (EP) achieved its first detection and localization of a bright X-ray flare, EP240219a, on 2024 February 19, during its commissioning phase. Subsequent targeted s…

astro-ph2005★ 3 cited

X-ray flares: late internal and late external shocks

X. F. Wu, Z. G. Dai, X. Y. Wang +3

We analyze several recently detected gamma-ray bursts (GRBs) with late X-ray flares in the context of late internal shock and late external shock models. We find that the X-ray fla…

astro-ph2005★ 10 cited

A Two-Component Explosion Model for the Giant Flare and Radio Afterglow from SGR1806-20

Z. G. Dai, X. F. Wu, X. Y. Wang +2

The brightest giant flare from the soft -ray repeater (SGR) 1806-20 was detected on 2004 December 27. The isotropic-equivalent energy release of this burst is at least one order…

astro-ph2005★ 24 cited

An energetic blast wave from the December 27 giant flare of the soft gamma-ray repeater 1806-20

X. Y. Wang, X. F. Wu, Y. Z. Fan +2

Recent follow-up observations of the December 27 giant flare of SGR 1806-20 have detected a multiple-frequency radio afterglow from 240 MHz to 8.46 GHz, extending in time from a we…

astro-ph2004★ 43 cited

Gamma-Ray Bursts: Polarization of Afterglows from Two-Component Jets

X. F. Wu, Z. G. Dai, Y. F. Huang +1

Polarization behaviors of optical afterglows from two-component gamma-ray burst jets are investigated, assuming various configurations for the two components. In most cases, the ob…