Zobrazeno 1 - 10
of 51
pro vyhledávání: '"Ce Cai"'
Autor:
Chao Zheng, Yan-Qiu Zhang, Shao-Lin Xiong, Cheng-Kui Li, He Gao, Wang-Chen Xue, Jia-Cong Liu, Chen-Wei Wang, Wen-Jun Tan, Wen-Xi Peng, Zheng-Hua An, Ce Cai, Ming-Yu Ge, Dong-Ya Guo, Yue Huang, Bing Li, Ti-Pei Li, Xiao-Bo Li, Xin-Qiao Li, Xu-Fang Li, Jin-Yuan Liao, Cong-Zhan Liu, Fang-Jun Lu, Xiang Ma, Rui Qiao, Li-Ming Song, Jin Wang, Ping Wang, Xi-Lu Wang, Yue Wang, Xiang-Yang Wen, Shuo Xiao, Yan-Bing Xu, Yu-Peng Xu, Zhi-Guo Yao, Qi-Bing Yi, Shu-Xu Yi, Yuan You, Fan Zhang, Jin-Peng Zhang, Peng Zhang, Shu Zhang, Shuang-Nan Zhang, Yan-Ting Zhang, Zhen Zhang, Xiao-Yun Zhao, Yi Zhao, Shi-Jie Zheng
Publikováno v:
The Astrophysical Journal Letters, Vol 962, Iss 1, p L2 (2024)
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:
https://doaj.org/article/9661393924584b919b41a300d6cb4c12
Autor:
Ruijing Tang, Dahai Yan, Haiyun Zhang, Qingchang Zhao, Lian Tao, Chengkui Li, Mingyu Ge, Xiaobo Li, Qianqing Yin, Ce Cai
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 1, p 26 (2024)
The Gaussian process method is employed to analyze the light curves of bursts detected by Insight-HXMT, Neutron Star Interior Composition Explorer (NICER), and Gravitational Wave High-energy Electromagnetic Counterpart All-sky Monitor from SGR 1935+2
Externí odkaz:
https://doaj.org/article/4ec555740b3941dd88877295d5a2ac2a
Autor:
Shuo Xiao, Yan-Qiu Zhang, Zi-Pei Zhu, Shao-Lin Xiong, He Gao, Dong Xu, Shuang-Nan Zhang, Wen-Xi Peng, Xiao-Bo Li, Peng Zhang, Fang-Jun Lu, Lin Lin, Liang-Duan Liu, Zhen Zhang, Ming-Yu Ge, You-Li Tuo, Wang-Chen Xue, Shao-Yu Fu, Xing Liu, Jin-Zhong Liu, An Li, Tian-Cong Wang, Chao Zheng, Yue Wang, Shuai-Qing Jiang, Jin-Da Li, Jia-Cong Liu, Zhou-Jian Cao, Xi-hong Luo, Jiao-jiao Yang, Shu-Xu Yi, Xi-Lu Wang, Ce Cai, Qi-Bin Yi, Yi Zhao, Sheng-Lun Xie, Cheng-Kui Li, Qi Luo, Li-Ming Song, Shu Zhang, Jin-Lu Qu, Cong-Zhan Liu, Xu-Fang Li, Yu-Peng Xu, Ti-Pei Li
Publikováno v:
The Astrophysical Journal, Vol 970, Iss 1, p 6 (2024)
The milestone discovery of GW170817-GRB 170817A-AT 2017gfo has shown that gravitational waves (GWs) could be produced during the merger of a neutron star–neutron star/black hole and that in electromagnetic (EM) waves, a gamma-ray burst (GRB) and a
Externí odkaz:
https://doaj.org/article/dcc9bc6c9fd0408ea6c7cbdebf860c7b
Autor:
Peng Zhang, Bing Li, Renzhou Gui, Shaolin Xiong, Ze-Cheng Zou, Xianggao Wang, Xiaobo Li, Ce Cai, Yi Zhao, Yanqiu Zhang, Wangchen Xue, Chao Zheng, Hongyu Zhao
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 272, Iss 1, p 4 (2024)
To investigate gamma-ray bursts (GRBs) in depth, it is crucial to develop an effective method for identifying GRBs accurately. Current criteria, e.g., onboard blind search, ground blind search, and target search, are limited by manually set threshold
Externí odkaz:
https://doaj.org/article/b9119e6d4dcd4876b998b659d92b676b
Autor:
Jun Yang, Xiao-Hong Zhao, Zhenyu Yan, Xiangyu Ivy Wang, Yan-Qiu Zhang, Zheng-Hua An, Ce Cai, Xin-Qiao Li, Zihan Li, Jia-Cong Liu, Zi-Ke Liu, Xiang Ma, Yan-Zhi Meng, Wen-Xi Peng, Rui Qiao, Lang Shao, Li-Ming Song, Wen-Jun Tan, Ping Wang, Chen-Wei Wang, Xiang-Yang Wen, Shuo Xiao, Wang-Chen Xue, Yu-Han Yang, Yi-Han Iris Yin, Bing Zhang, Fan Zhang, Shuai Zhang, Shuang-Nan Zhang, Chao Zheng, Shi-Jie Zheng, Shao-Lin Xiong, Bin-Bin Zhang
Publikováno v:
The Astrophysical Journal Letters, Vol 947, Iss 1, p L11 (2023)
The brightest gamma-ray burst, GRB 221009A, has spurred numerous theoretical investigations, with particular attention paid to the origins of ultrahigh-energy TeV photons during the prompt phase. However, analyzing the mechanism of radiation of photo
Externí odkaz:
https://doaj.org/article/ad8854cccfb34384849848cc57c5c25a
Autor:
Bei You, Yuoli Tuo, Chengzhe Li, Wei Wang, Shuang-Nan Zhang, Shu Zhang, Mingyu Ge, Chong Luo, Bifang Liu, Weimin Yuan, Zigao Dai, Jifeng Liu, Erlin Qiao, Chichuan Jin, Zhu Liu, Bozena Czerny, Qingwen Wu, Qingcui Bu, Ce Cai, Xuelei Cao, Zhi Chang, Gang Chen, Li Chen, Tianxiang Chen, Yibao Chen, Yong Chen, Yupeng Chen, Wei Cui, Weiwei Cui, Jingkang Deng, Yongwei Dong, Yuanyuan Du, Minxue Fu, Guanhua Gao, He Gao, Min Gao, Yudong Gu, Ju Guan, Chengcheng Guo, Dawei Han, Yue Huang, Jia Huo, Shumei Jia, Luhua Jiang, Weichun Jiang, Jing Jin, Yongjie Jin, Lingda Kong, Bing Li, Chengkui Li, Gang Li, Maoshun Li, Tipei Li, Wei Li, Xian Li, Xiaobo Li, Xufang Li, Yanguo Li, Zhengwei Li, Xiaohua Liang, Jinyuan Liao, Congzhan Liu, Guoqing Liu, Hongwei Liu, Xiaojing Liu, Yinong Liu, Bo Lu, Fangjun Lu, Xuefeng Lu, Qi Luo, Tao Luo, Xiang Ma, Bin Meng, Yi Nang, Jianyin Nie, Ge Ou, Jinlu Qu, Na Sai, Rencheng Shang, Liming Song, Xinying Song, Liang Sun, Ying Tan, Lian Tao, Chen Wang, Guofeng Wang, Juan Wang, Lingjun Wang, Wenshuai Wang, Yusa Wang, Xiangyang Wen, Baiyang Wu, Bobing Wu, Mei Wu, Guangcheng Xiao, Shuo Xiao, Shaolin Xiong, Yupeng Xu, Jiawei Yang, Sheng Yang, Yanji Yang, Qibin Yi, Qianqing Yin, Yuan You, Aimei Zhang, Chengmo Zhang, Fan Zhang, Hongmei Zhang, Juan Zhang, Tong Zhang, Wanchang Zhang, Wei Zhang, Wenzhao Zhang, Yi Zhang, Yifei Zhang, Yongjie Zhang, Yue Zhang, Zhao Zhang, Ziliang Zhang, Haisheng Zhao, Xiaofan Zhao, Shijie Zheng, Dengke Zhou, Jianfeng Zhou, Yuxuan Zhu, Yue Zhu
Publikováno v:
Nature Communications, Vol 12, Iss 1, Pp 1-11 (2021)
Evolution of accretion disk and corona during outbursts in black hole binary systems is still unclear. Here, the authors show spectral analysis of MAXI J1820+070 and propose a scenario of a dynamical corona to explain the evolution of the reflection
Externí odkaz:
https://doaj.org/article/08ba0f4a6ddf40c79819c077774b1898
Autor:
Shuo Xiao, Ya-Qing Liu, Ke Gong, Zheng-Hua An, Shao-Lin Xiong, Xin-Qiao Li, Xiang-Yang Wen, Wen-Xi Peng, Da-Li Zhang, You-Li Tuo, Shi-Jie Zheng, Li-Ming Song, Ping Wang, Xiao-Yun Zhao, Yue Huang, Xiang Ma, Xiao-Jing Liu, Rui Qiao, Yan-Bing Xu, Sheng Yang, Fan Zhang, Yue Wang, Yan-Qiu Zhang, Wang-Chen Xue, Jia-Cong Liu, Chao Zheng, Chen-Wei Wang, Wen-Jun Tan, Ce Cai, Qi-Bin Yi, Peng Zhang, Xi-Hong Luo, Jiao-Jiao Yang, Qi-Jun Zhi, Ai-Jun Dong, Shi-Jun Dang, Lun-Hua Shang, Shuang-Nan Zhang
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 270, Iss 1, p 3 (2023)
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 2022 July 27, aims to monito
Externí odkaz:
https://doaj.org/article/bd39e2fcf6ca4a3dae2f0ac83c7dfde5
Autor:
Shuo Xiao, Jiao-Jiao Yang, Xi-Hong Luo, Shao-Lin Xiong, Yuan-Hong Qu, Shuang-Nan Zhang, Wang-Chen Xue, Xiao-Bo Li, You-Li Tuo, Ai-Jun Dong, Ru-Shuang Zhao, Shi-Jun Dang, Lun-Hua Shang, Qing-Bo Ma, Ce Cai, Jin Wang, Ping Wang, Cheng-Kui Li, Shu-Xu Yi, Zhen Zhang, Ming-Yu Ge, Shi-Jie Zheng, Li-Ming Song, Wen-Xi Peng, Xiang-Yang Wen, Xin-Qiao Li, Zheng-Hua An, Xin Xu, Yue Wang, Chao Zheng, Yan-Qiu Zhang, Jia-Cong Liu, Bin Zhang, Wei Xie, Jian-Chao Feng, De-Hua Wang, Qi-Jun Zhi
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 268, Iss 1, p 5 (2023)
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)–li
Externí odkaz:
https://doaj.org/article/e860043c050448e4bca91a67fc480dcd
Autor:
Xi-Hong Luo, Shuo Xiao, Shi-Jie Zheng, Ming-Yu Ge, You-Li Tuo, Shao-Lin Xiong, Shuang-Nan Zhang, Fang-Jun Lu, Yue Huang, Cheng Yang, Qi-Jun Zhi, Li-Ming Song, Wen-Xi Peng, Xiang-Yang Wen, Xin-Qiao Li, Zheng-Hua An, Jin Wang, Ping Wang, Ce Cai, Cheng-Kui Li, Xiao-Bo Li, Fan Zhang, Ai-Jun Dong, Wei Xie, Jian-Chao Feng, Qing-Bo Ma, Hua Wang De, Lun-Hua Shang, Xin Xu, Meng-Xuan Zhang, Zi-Ping Dong, Shi-Jun Dang
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 266, Iss 1, p 16 (2023)
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:
https://doaj.org/article/6da9c7d6483342eeb1fa0c54d18881b4
Autor:
Yi Zhao, Wang-Chen Xue, Shao-Lin Xiong, Yuan-Hao Wang, Jia-Cong Liu, Qi Luo, Yan-Qiu Zhang, Jian-Chao Sun, Xiao-Yun Zhao, Ce Cai, Shuo Xiao, Yue Huang, Xiao-Bo Li, Zhen Zhang, Jin-Yuan Liao, Sheng Yang, Rui Qiao, Dong-Ya Guo, Chao Zheng, Qi-Bin Yi, Sheng-Lun Xie, Zhi-Wei Guo, Chao-Yang Li, Chen-Wei Wang, Wen-Jun Tan, Yue Wang, Wen-Xi Peng, Shi-Jie Zheng, Jian-Jian He, Ping Wang, Jin Wang, Xiang Ma, Xin-Ying Song, Hong-Mei Zhang, Bing Li, Peng Zhang, Hong Wu, Yan-Qi Du, Jing Liang, Guo-Ying Zhao, Xin-Qiao Li, Xiang-Yang Wen, Zheng-Hua An, Xi-Lei Sun, Yan-Bing Xu, Fan Zhang, Da-Li Zhang, Ke Gong, Ya-Qing Liu, Xiao-Hua Liang, Xiao-Jing Liu, Min Gao, Jin-Zhou Wang, Li-Ming Song, Gang Chen, Ke-Ke Zhang, Xing-Bo Han, Hai-Yan Wu, Tai Hu, Hao Geng, Fang-Jun Lu, Shu Zhang, Shuang-Nan Zhang, Gao-Peng Lu, Ming Zeng, Heng Yu
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 265, Iss 1, p 17 (2023)
The Gravitational Wave High-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is a pair of microsatellites (i.e., GECAM-A and GECAM-B) dedicated to monitoring gamma-ray transients including the high-energy electromagnetic counterparts of gra
Externí odkaz:
https://doaj.org/article/24f4bda62e2548709e374a4df532befa