most citedSynchrotron Radiation Dominates the Extremely Bright GRB 221009A

43 citations · 105 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2024

A new subclass of gamma-ray burst originating from compact binary merger

Chen-Wei Wang, Wen-Jun Tan, Shao-Lin Xiong +15

Type I gamma-ray bursts (GRBs) are believed to originate from compact binary merger usually with duration less than 2 seconds for the main emission. However, recent observations of…

astro-ph.HE20232 cited

Evidence of Hadronic Emission from the brightest-of-all-time GRB 221009A

Kai Wang, Qing-Wen Tang, Yan-Qiu Zhang +4

Acceleration of hadrons in relativistic shocks has been long expected and invoked to model GRB high-energy photon and neutrino emissions. However, so far there has been no direct o…

astro-ph.IM2023

Calibration of the Timing Performance of GECAM-C

Shuo Xiao, Ya-Qing Liu, Ke Gong +35

As a new member of the Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) after GECAM-A and GECAM-B, GECAM-C (originally called HEBS), which was lau…

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…

astro-ph.HE202343 cited

Synchrotron Radiation Dominates the Extremely Bright GRB 221009A

Jun Yang, Xiao-Hong Zhao, Zhenyu Yan +30

The brightest Gamma-ray burst, GRB 221009A, has spurred numerous theoretical investigations, with particular attention paid to the origins of ultra-high energy TeV photons during t…