Zobrazeno 1 - 10
of 148
pro vyhledávání: '"Li‐Xin Qiao"'
Autor:
Feng, Pei-Yi, An, Zheng-Hua, Li, Yu-Hui, Le, Qi, Zhang, Da-Li, Li, Xin-Qiao, Xiong, Shao-Lin, Liu, Cong-Zhan, Liu, Wei-Bin, Wang, Jian-Li, Deng, Bing-Lin, Xu, He, Lu, Hong
The Gamma-Ray Transient Monitor (GTM) is an all-sky monitor onboard the Distant Retrograde Orbit-A (DRO-A) satellite, with the scientific objective of detecting gamma-ray bursts in the energy range of 20 keV to 1 MeV. The GTM is equipped with five Ga
Externí odkaz:
http://arxiv.org/abs/2411.18988
Autor:
Zhang, Yan-Qiu, Xiong, Shao-Lin, Mao, Ji-Rong, Zhang, Shuang-Nan, Xue, Wang-Chen, Zheng, Chao, Liu, Jia-Cong, Zhang, Zhen, Wang, Xi-Lu, Ge, Ming-Yu, Yi, Shu-Xu, Song, Li-Ming, An, Zheng-Hua, Cai, Ce, Li, Xin-Qiao, Peng, Wen-Xi, Tan, Wen-Jun, Wang, Chen-Wei, Wen, Xiang-Yang, Wang, Yue, Xiao, Shuo, Zhang, Fan, Zhang, Peng, Zheng, Shi-Jie
Publikováno v:
Observation of spectral lines in the exceptional GRB 221009A. Sci. China-Phys. Mech. Astron. 67, 289511 (2024)
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 spectroscopy analysis of GRB 221009A jointly with GECAM-C and Fermi/GBM data to
Externí odkaz:
http://arxiv.org/abs/2403.12851
Autor:
Feng, Pei-Yi, An, Zheng-Hua, Zhang, Da-Li, Wang, Chen-Wei, Zheng, Chao, Yang, Sheng, Xiong, Shao-Lin, Liu, Jia-Cong, Li, Xin-Qiao, Gong, Ke, Liu, Xiao-Jing, Gao, Min, Wen, Xiang-Yang, liu, Ya-Qing, Zhao, Xiao-Yun, Zhang, Fan, Sun, Xi-Lei, Lu, Hong
Publikováno v:
Sci. China-Phys. Mech. Astron. 67, 111013 (2024)
Gamma-ray Transient Monitor (GTM) is an all-sky monitor onboard the Distant Retrograde Orbit-A (DRO-A) satellite with the scientific objective of detecting gamma-ray transients ranging from 20 keV to 1 MeV. GTM is equipped with 5 Gamma-ray Transient
Externí odkaz:
http://arxiv.org/abs/2401.07513
Autor:
Feng, Pei-Yi, Sun, Xi-Lei, Wang, Cheng-Er, Deng, Yong, An, Zheng-Hua, Zhang, Da-Li, Zheng, Chao, Li, Xin-Qiao, Xiong, Shao-Lin, Lu, Hong
The intrinsic resolution is the primary limitation on the total energy resolution of LaBr$_3$(Ce) crystal. This intrinsic resolution arises from two effects: fluctuations occurring in the process of energy transfer to luminescent centers within the L
Externí odkaz:
http://arxiv.org/abs/2401.00226
Autor:
Feng, Pei-Yi, Sun, Xi-Lei, An, Zheng-Hua, Deng, Yong, Wang, Cheng-Er, Jiang, Huang, Li, Jun-Jie, Zhang, Da-Li, Li, Xin-Qiao, Xiong, Shao-Lin, Zheng, Chao, Gong, Ke, Yang, Sheng, Liu, Xiao-Jing, Gao, Min, Wen, Xiang-Yang, Liu, Ya-Qing, Xu, Yan-Bing, Zhao, Xiao-Yun, Liu, Jia-Cong, Zhang, Fan, Lu, Hong
The GECAM series of satellites utilize LaBr3(Ce), LaBr3(Ce,Sr), and NaI(Tl) crystals as sensitive materials for gamma-ray detectors (GRDs). To investigate the non-linearity in the detection of low-energy gamma rays and address errors in the E-C relat
Externí odkaz:
http://arxiv.org/abs/2312.16658
Autor:
Zheng, Chao, Zhang, Yan-Qiu, Xiong, Shao-Lin, Li, Cheng-Kui, Gao, He, Xue, Wang-Chen, Liu, Jia-Cong, Wang, Chen-Wei, Tan, Wen-Jun, Peng, Wen-Xi, An, Zheng-Hua, Cai, Ce, Ge, Ming-Yu, Guo, Dong-Ya, Huang, Yue, Li, Bing, Li, Ti-Pei, Li, Xiao-Bo, Li, Xin-Qiao, Li, Xu-Fang, Liao, Jin-Yuan, Liu, Cong-Zhan, Lu, Fang-Jun, Ma, Xiang, Qiao, Rui, Song, Li-Ming, Wang, Jin, Wang, Ping, Wang, Xi-Lu, Wang, Yue, Wen, Xiang-Yang, Xiao, Shuo, Xu, Yan-Bing, Xu, Yu-Peng, Yao, Zhi-Guo, Yi, Qi-Bing, Yi, Shu-Xu, You, Yuan, Zhang, Fan, Zhang, Jin-Peng, Zhang, Peng, Zhang, Shu, Zhang, Shuang-Nan, Zhang, Yan-Ting, Zhang, Zhen, Zhao, Xiao-Yun, Zhao, Yi, Zheng, Shi-Jie
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 early afterglow in unprecedented detail. In this letter, we report comp
Externí odkaz:
http://arxiv.org/abs/2310.10522
Autor:
Xiao, Shuo, Liu, Ya-Qing, Gong, Ke, An, Zheng-Hua, Xiong, Shao-Lin, Li, Xin-Qiao, Wen, Xiang-Yang, Peng, Wen-Xi, Zhang, Da-Li, Tuo, You-Li, Zheng, Shi-Jie, Song, Li-Ming, Wang, Ping, Zhao, Xiao-Yun, Huang, Yue, Ma, Xiang, Liu, Xiao-Jing, Qiao, Rui, Xu, Yan-Bing, Yang, Sheng, Zhang, Fan, Wang, Yue, Zhang, Yan-Qiu, Xue, Wang-Chen, Liu, Jia-Cong, Zheng, Chao, Wang, Chen-Wei, Tan, Wen-Jun, Cai, Ce, Yi, Qi-Bin, Zhang, Peng, Luo, Xi-Hong, Yang, Jiao-Jiao, Zhi, Qi-Jun, Dong, Ai-Jun, Dang, Shi-Jun, Shang, Lun-Hua, Zhang, Shuang-Nan
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 launched on board the SATech-01 satellite on July 27, 2022, aims to monit
Externí odkaz:
http://arxiv.org/abs/2308.11362
Autor:
Xiao, Shuo, Yang, Jiao-Jiao, Luo, Xi-Hong, Xiong, Shao-Lin, Qu, Yuan-Hong, Zhang, Shuang-Nan, Xue, Wang-Chen, Li, Xiao-Bo, Tuo, You-Li, Dong, Ai-Jun, Zhao, Ru-Shuang, Dang, Shi-Jun, Shang, Lun-Hua, Ma, Qing-Bo, Cai, Ce, Wang, Jin, Wang, Ping, Li, Cheng-Kui, Yi, Shu-Xu, Zhang, Zhen, Ge, Ming-Yu, Zheng, Shi-Jie, Song, Li-Ming, Peng, Wen-Xi, Wen, Xiang-Yang, Li, Xin-Qiao, An, Zheng-Hua, Xu, Xin, Wang, Yue, Zheng, Chao, Zhang, Yan-Qiu, Liu, Jia-Cong, Zhang, Bin, Xie, Wei, Feng, Jian-Chao, Wang, De-Hua, Zhi, Qi-Jun
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 radius of the possible relativistic jet in gamma-ray burst (GRB)-like
Externí odkaz:
http://arxiv.org/abs/2307.07079
Autor:
Xie, Sheng-Lun, Cai, Ce, Yu, Yun-Wei, Xiong, Shao-Lin, Lin, Lin, Zhao, Yi, Zhang, Shuang-Nan, Song, Li-Ming, Wang, Ping, Li, Xiao-Bo, Xue, Wang-Chen, Zhang, Peng, Zheng, Chao, Zhang, Yan-Qiu, Liu, Jia-Cong, Wang, Chen-Wei, Tan, Wen-Jun, Wang, Yue, Yu, Zheng-Hang, Feng, Pei-Yi, Zhang, Jin-Peng, Xiao, Shuo, Zhao, Hai-Sheng, Zhang, Wen-Long, Zhang, Yan-Ting, Huang, Yue, Zhao, Xiao-Yun, Ma, Xiang, Zheng, Shi-Jie, Li, Xin-Qiao, Wen, Xiang-Yang, Gong, Ke, An, Zheng-Hua, Zhang, Da-Li, Yang, Sheng, Liu, Xiao-Jing, Zhang, Fan
Magnetar is a neutron star with an ultrahigh magnetic field ($\sim 10^{14}-10^{15}$ G) which usually manifests as soft gamma-ray repeater (SGR) or anomalous X-ray pulsar (AXP). SGR J1935+2154 is not only one of the most active magnetar detected so fa
Externí odkaz:
http://arxiv.org/abs/2307.01010
Autor:
Luo, Xi-Hong, Xiao, Shuo, Zheng, Shi-Jie, Ge, Ming-Yu, Tuo, You-Li, Xiong, Shao-Lin, Zhang, Shuang-Nan, Lu, Fang-Jun, Huang, Yue, Yang, Cheng, Zhi, Qi-Jun, Song, Li-Ming, Peng, Wen-Xi, Wen, Xiang-Yang, Li, Xin-Qiao, An, Zheng-Hua, Wang, Jin, Wang, Ping, Cai, Ce, Li, Cheng-Kui, Li, Xiao-Bo, Zhang, Fan, Dong, Ai-Jun, Xie, Wei, Feng, Jian-Chao, Ma, Qing-Bo, Wang, De-Hua, Shang, Lun-Hua, Xu, Xin, Zhang, Meng-Xuan, Dong, Zi-Ping, Dang, Shi-Jun
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 exploration in general. A spacecraft that can determine its own absolute pos
Externí odkaz:
http://arxiv.org/abs/2303.14490