activity
20052025
most citedSpectral lags caused by the Doppler effect of fireballs

55 citations · 283 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2025

Towards Understanding the Origin of Swift Gamma-Ray Bursts Driven by Magnetars

C. T. Hao, J. H. Jing, X. L. Han +7

We analyze a sample of\textit{ Swift} gamma-ray bursts (GRBs) with extended emissions in -rays and/or X-ray plateaus that may be driven by magnetars. Multi-wavelength data and m…

astro-ph.HE2024★ 8 cited

Revisiting the energy distribution and formation rate of CHIME fast radio bursts

K. J. Zhang, Z. B. Zhang, A. E. Rodin +9

Based on the first CHIME/FRB catalogue, three volume-limited samples of fast radio bursts (FRBs) are built, with samples 1, 2, and 3 corresponding to a fluence cut of 5, 3, and 1,…

astro-ph.HE2023★ 18 cited

Properties of Gamma-Ray Bursts Associated with Supernovae and Kilonovae

Q. M. Li, Z. B. Zhang, X. L. Han +3

We systematically compare the temporal and spectral properties of 53 Supernova (SN)-associated and 15 Kilonova (KN)-associated Gamma-Ray Bursts (GRBs). We find that the spectral pa…

astro-ph.HE2023★ 1 cited

The origin of low-redshift event rate excess as revealed by the low-luminosity GRBs

X. F. Dong, Z. B. Zhang, Q. M. Li +2

The relation between the event rate of long Gamma-Ray Bursts at low redshift and the star formation rate is still controversial, especially in the low-redshift end. Dong et al. con…

astro-ph.HE2021★ 8 cited

Overall Spectral Properties of Prompt Emissions with Diverse Segments in Swift/BAT Short Gamma-ray Bursts

X. J. Li, Z. B. Zhang, K. Zhang

Owing to lack of multiple components of prompt -ray emissions in short gamma-ray bursts (sGRBs), how these distinct components are correlated still keeps unclear. In this paper,…

astro-ph.HE2021★ 19 cited

Long and Short Fast Radio Bursts are Different from Repeating and Non-repeating Transients

X. J. Li, X. F. Dong, Z. B. Zhang +1

We collect 133 Fast Radio Bursts (FRBs), including 110 non-repeating and 23 repeating ones, and systematically investigate their observational properties. To check the frequency de…