activity
20122024
most citedObservation of spectral lines in the exceptional GRB 221009A

40 citations · 288 across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.HE2024★ 16 cited

Relation between the keV-MeV and TeV emission of GRB 221009A and its implications

Yan-Qiu Zhang, Hao-Xiang Lin, Shao-Lin Xiong +13

Gamma-ray bursts (GRBs) are believed to launch relativistic jets, which generate prompt emission by internal processes, and produce long-lasting afterglows by driving external shoc…

astro-ph.HE2024★ 40 cited

Observation of spectral lines in the exceptional GRB 221009A

Yan-Qiu Zhang, Shao-Lin Xiong, Ji-Rong Mao +21

As the brightest gamma-ray burst ever observed, GRB 221009A provided a precious opportunity to explore spectral line features. In this paper, we performed a comprehensive spectrosc…

astro-ph.HE2023

Observation of GRB 221009A early afterglow in X/-ray energy band

Chao Zheng, Yan-Qiu Zhang, Shao-Lin Xiong +45

The early afterglow of a Gamma-ray burst (GRB) can provide critical information on the jet and progenitor of the GRB. The extreme brightness of GRB 221009A allows us to probe its e…

astro-ph.HE2023

Revisiting the Properties of GW190814 and Its Formation History

F. Lyu, L. Yuan, D. H. Wu +9

GW190814 was reported during LIGO's and Virgo's third observing run with the most asymmetric component masses (a black hole and a compac…

astro-ph.HE2023

Individual and Averaged Power Density Spectra of X-ray bursts from SGR J1935+2154: Quasiperiodic Oscillation Search and Slopes

Shuo Xiao, Xiao-Bo Li, Wang-Chen Xue +29

The study of quasi-periodic oscillations (QPOs) and power density spectra (PDS) continuum properties can help shed light on the still illusive emission physics of magnetars and as…

astro-ph.HE2023

The Minimum Variation Timescales of X-ray bursts from SGR J1935+2154

Shuo Xiao, Jiao-Jiao Yang, Xi-Hong Luo +34

The minimum variation timescale (MVT) of soft gamma-ray repeaters can be an important probe to estimate the emission region in pulsar-like models, as well as the Lorentz factor and…