activity
20082025
most citedDiscovery of the radio and X-ray counterpart of TeV Gamma-ray source HESS J1731-347

95 citations · 291 across the 7 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2025★ 1 cited

An Intermediate-mass Black Hole Lurking in A Galactic Halo Caught Alive during Outburst

C. -C. Jin, D. -Y. Li, N. Jiang +137

Stellar-mass and supermassive black holes abound in the Universe, whereas intermediate-mass black holes (IMBHs) of ~10^2-10^5 solar masses in between are largely missing observatio…

astro-ph.HE2024★ 30 cited

A fast X-ray transient from a weak relativistic jet associated with a type Ic-BL supernova

H. Sun, W. -X. Li, L. -D. Liu +163

Massive stars end their lives as core-collapse supernovae, amongst which some extremes are broad-lined type Ic supernovae from Wolf-Rayet stars associated with long-duration gamma-…

astro-ph.HE2024★ 2 cited

Soft X-ray prompt emission from a high-redshift gamma-ray burst EP240315a

Y. Liu, H. Sun, D. Xu +191

Long gamma-ray bursts (GRBs) are believed to originate from core collapse of massive stars. High-redshift GRBs can probe the star formation and reionization history of the early un…

astro-ph.HE2022★ 53 cited

First wide field-of-view X-ray observations by a lobster eye focusing telescope in orbit

C. Zhang, Z. X. Ling, X. J. Sun +75

As a novel X-ray focusing technology, lobster eye micro-pore optics (MPO) feature both a wide observing field of view and true imaging capability, promising sky monitoring with sig…

astro-ph.SR2018★ 15 cited

Two Types of Long-duration Quasi-static Evolution of Solar Filaments

Chen Xing, Haochuan Li, Bei Jiang +2

In this Letter, we investigate the long-duration quasi-static evolution of 12 pre-eruptive filaments (4 active region and 8 quiescent filaments), mainly focusing on the evolution o…

astro-ph2008★ 95 cited

Discovery of the radio and X-ray counterpart of TeV Gamma-ray source HESS J1731-347

W. W. Tian, D. A. Leahy, M. Haverkorn +1

We discover a faint shell-type radio and X-ray source, G353.6-0.7, associated with HESS J1731-347. G353.6-0.7 is likely an old supernova remnant (SNR), based on radio (0.8 GHz, 1.4…