activity
20222026
most citedInsight-HXMT dedicated 33-day observation of SGR J1935+2154 I. Burst Catalog

36 citations · 48 across the 15 of their papers we have counts for

collaborators

18 papers

astro-ph.IM2026

ELISA: A Bayesian X/-ray Spectral Analysis Toolkit

Wang-Chen Xue, Sheng-Lun Xie, Chao Zheng +11

Forward-folded X/-ray spectral fitting increasingly benefits from Bayesian workflows to better capture counting statistics, background uncertainties, and complex parameter degen…

astro-ph.HE2026

Magnetar X-ray flares as elementary reconnection events in a self-organized critical magnetosphere

Sheng-Lun Xie, Yi Zhao, Wen-Long Zhang +3

Magnetar bursts are commonly attributed to magnetic energy release, yet the physically relevant dissipation unit has remained uncertain. Here we argue that this unit is not the bur…

astro-ph.HE2026

Evidence of self-organized criticality in the prompt emission of a bright gamma-ray burst

Wen-Long Zhang, Wen-Jun Tan, Hao-Tian Lan +18

Gamma-ray bursts (GRBs) are the most energetic explosive events in the Universe, yet the physical mechanism of their prompt emission remains a mystery. Especially, it is unclear wh…

astro-ph.HE2026

GRB 250706B/C: Insight-HXMT Discovery of a High-Luminosity Burst as a Candidate for Fallback-Regulated Accretion in the Prompt Emission

Chen-Wei Wang, R. Moradi, Shao-Lin Xiong +15

Fallback accretion in collapsar models is often associated with underluminous gamma-ray bursts (GRBs), leading to the widespread view that fallback-fed engines may be intrinsically…

astro-ph.HE2026

Spectral Evidence of Heavy Nuclei from the Neutron Star Crust in Magnetar Bursts

Sheng-Lun Xie, Yun-Wei Yu, Shao-Lin Xiong +1

The crust of a neutron star (NS) provides a unique laboratory for studying matter under extreme density and magnetic field conditions that cannot be realized in terrestrial experim…

astro-ph.HE2026★ 4 cited

Brightest GRB flare observed in GRB 221009A: bridge the last gap between flare and prompt emission in GRB

Zheng-Hang Yu, Chen-Wei Wang, Shao-Lin Xiong +46

Flares are usually observed during the afterglow phase of Gamma-Ray Bursts (GRBs) in soft X-ray, optical and radio bands, but rarely in gamma-ray band. Despite the extraordinary br…

astro-ph.IM2025

LUNCH: A Lightweight Unified Deep-Learning Framework for General Transients Classification in High-Energy Time-Domain Astronomy

Peng Zhang, Chen-Wei Wang, Zheng-Hang Yu +19

The increasing data volume of high-energy space monitors necessitates real-time, automated transient classification for multi-messenger follow-up. Conventional methods rely on empi…

astro-ph.IM2025

BREAKFAST: A Framework for general joint BA duty and follow-up guidance of multiple -ray monitors

Chen-Wei Wang, Peng Zhang, Shao-Lin Xiong +30

With the growing number of gamma-ray monitors in operation, several research teams have adopted a strategy of joint operation and scientific duty to improve efficiency. A successfu…

astro-ph.HE2025★ 5 cited

Unveil A Peculiar Light Curve Pattern of Magnetar Burst with GECAM observations of SGR J1935+2154

Yue Wang, Chen-Wei Wang, Shaolin Xiong +28

Magnetar X-ray Burst (MXB) is usually composed of a single pulse or multiple pulses with rapid rise and brief duration mostly observed in hard X-ray (soft gamma-ray) band. Previous…

astro-ph.HE2025★ 2 cited

Eclipsed X-ray Bursts from Magnetar SGR J1935+2154 and the Fireball Measurements

Sheng-Lun Xie, Aming Chen, Yun-Wei Yu +17

In theory, burst activity of the magnetar can lead to the formation of fireballs trapped by the magnetic field and corotating with the star. However, the smoking-gun observational…

astro-ph.HE2025

On the Ultra-Long Gamma-Ray Transient GRB 250702B/EP250702

Jin-Peng Zhang, Chen-Wei Wang, Zheng-Hang Yu +20

GRB 250702B/EP250702a is an interesting long-duration gamma-ray transient whose nature is in debate. To obtain a full picture in gamma-ray band, we implement a comprehensive target…

astro-ph.HE2025

Multi-Instrument Search for Gamma-Ray Counterpart of X-ray Transients detected by EP/WXT

Yan-Qiu Zhang, Wang-Chen Xue, Jin-Peng Zhang +25

As a soft X-ray imager with unprecedentedly large field of view, EP/WXT has detected many (fast) X-ray transients, whose nature is very intriguing. Whether there is gamma-ray count…

astro-ph.HE2025

GECAM Discovery of Peculiar Oscillating Particle Precipitation Events

Chenwei Wang, Shaolin Xiong, Yi Zhao +52

Charged particle precipitation typically manifests as a gradual increase and decrease of flux observed by space detectors. Cases with rapidly flux variation are very rare. Periodic…

astro-ph.IM2025

Pitch Angle Measurement Method based on Detector Counts Distribution. -I. Basic conception

Chenwei Wang, Shaolin Xiong, Hongbo Xue +36

As an X-ray and gamma-ray all-sky monitor aiming for high energy astrophysical transients, Gravitational-wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) has al…

astro-ph.HE2025

Search for Type IL Gamma-ray Bursts: Criterion, Results, Verification and Physical Implication

Wen-Jun Tan, Chen-Wei Wang, Peng Zhang +11

As an interesting subclass of gamma-ray burst (GRB), Type IL GRB (such as GRB 211211A and GRB 230307A) features a long-duration prompt emission but originating from compact binary…

astro-ph.HE2025

Evolution of the Three Spectral Components in the Prompt Emission of GRB 240825A

Chen-Wei Wang, Wen-Jun Tan, Shao-Lin Xiong +17

The prompt emission of Gamma-Ray Bursts (GRBs) could be composed of different spectral components, such as a dominant non-thermal Band component in the keV-MeV range, a subdominant…

astro-ph.HE2022★ 1 cited

A Localization Method of High Energy Transients for All-Sky Gamma-Ray Monitor

Yi Zhao, Wangchen Xue, Shaolin Xiong +62

Fast and reliable localization of high-energy transients is crucial for characterizing the burst properties and guiding the follow-up observations. Localization based on the relati…

astro-ph.HE2022★ 36 cited

Insight-HXMT dedicated 33-day observation of SGR J1935+2154 I. Burst Catalog

Ce Cai, Wangchen Xue, Chengkui Li +21

Magnetars are neutron stars with extreme magnetic field and sometimes manifest as soft gamma-ray repeaters (SGRs). SGR J1935+2154 is one of the most prolific bursters and the first…