activity
19982026
most citedThe optical flare and afterglow light curve of GRB 050904 at redshift z=6.29

55 citations · 140 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026

Diverse properties of electron Forbush decreases revealed by the Dark Matter Particle Explorer

F. Alemanno, Q. An, P. Azzarello +147

The Forbush decrease (FD) of cosmic rays is an important probe of the interplanetary environment disturbed by solar activities. In this work, we study the properties of 8 FDs elect…

astro-ph.HE2026

First Detection of -Ray Emission from the Compact Symmetric Object JVAS J1311+1658

Xiong Jiang, Yang-Ji Li, Hai Lei +1

We report the first detection of -ray emission from the young radio galaxy JVAS~J1311+1658, classified as a compact symmetric object (CSO). This detection is characterized by a…

astro-ph.HE2025

GRB 241030A: a prompt thermal X-ray emission component and diverse origin of the very early UVOT WHITE and U band emission

Qiu-Li Wang, Hao Zhou, Yun Wang +17

We present a detailed analysis of the long-duration GRB 241030A detected by {\it Swift}. Thanks to the rapid response of XRT and UVOT, the strongest part of the prompt emission of…

astro-ph.HE2023★ 1 cited

A two-component jet model for the optical plateau in the afterglow of GRB 191221B

Yi-Ming Zhu, Yun Wang, Hao Zhou +5

The long gamma-ray burst GRB 191221B has abundant observations in X-ray, optical and radio bands. In the literature, the observed optical light curve of GRB 191221B displays a plat…

astro-ph2005★ 55 cited

The optical flare and afterglow light curve of GRB 050904 at redshift z=6.29

D. M. Wei, T. Yan, Y. Z. Fan

GRB050904 is very interesting since it is by far the most distant GRB event known to date(). It was reported that during the prompt high energy emission phase, a very brigh…

astro-ph2003★ 40 cited

The afterglow of GRB021211: Another case of reverse shock emission

D. M. Wei

GRB021211 was first detected by HETE II and its early afterglow has been observed. There is a break in its afterglow light curve at about 12 minutes after the bursts, before the br…