activity
20142023
most citedMeasurement of the strong phase difference in

50 citations · 187 across the 12 of their papers we have counts for

collaborators

12 papers

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…

astro-ph.IM20237 cited

Pulsar and Magnetar Navigation with Fermi/GBM and GECAM

Xi-Hong Luo, Shuo Xiao, Shi-Jie Zheng +29

The determination of the absolute and relative position of a spacecraft is critical for its operation, observations, data analysis, scientific studies, as well as deep space explor…

astro-ph.HE202317 cited

Discovery of the linear energy-dependence of the spectral lag of X-ray bursts from SGR J1935+2154

Shuo Xiao, You-Li Tuo, Shuang-Nan Zhang +31

Spectral lag of the low-energy photons with respect to the high-energy ones is a common astrophysical phenomenon (such as Gamma-ray bursts and the Crab pulsar) and may serve as a k…

astro-ph.IM20231 cited

The performance of SiPM-based gamma-ray detector (GRD) of GECAM-C

Dali Zhang, Chao Zheng, Jiacong Liu +42

As a new member of GECAM mission, the GECAM-C (also called High Energy Burst Searcher, HEBS) is a gamma-ray all-sky monitor onboard SATech-01 satellite, which was launched on July…

astro-ph.HE202333 cited

Insight-HXMT and GECAM-C observations of the brightest-of-all-time GRB 221009A

Zheng-Hua An, S. Antier, Xing-Zi Bi +174

GRB 221009A is the brightest gamma-ray burst ever detected since the discovery of this kind of energetic explosions. However, an accurate measurement of the prompt emission propert…

astro-ph.IM20234 cited

Cross calibration of gamma-ray detectors (GRD) of GECAM-C

Yan-Qiu Zhang, Shao-Lin Xiong, Rui Qiao +42

The gamma-ray detectors (GRDs) of GECAM-C onborad SATech-01 satellite is designed to monitor gamma-ray transients all over the sky from 6 keV to 6 MeV. The energy response matrix i…