Zobrazeno 1 - 10
of 1 458
pro vyhledávání: '"Li Ti"'
Autor:
Zhao Siyue, Li Caiwu, Li Guo, Yang Shengzhi, Zhou Yingming, He Yongguo, Wu Daifu, Zhou Yu, Zeng Wen, Li Ti, Qu Yuanyuan, Li Bei, Deng Wenwen, Jin Lei, Yu Xiumei, Huang Yan, Zhang Hemin, Zou Likou
Publikováno v:
Open Life Sciences, Vol 14, Iss 1, Pp 288-298 (2019)
The giant panda (GP) was the most endangered species in China, and gut microbiota plays a vital role in host health. To determine the differences of the gut microbiota among the male, female and pregnant GPs, a comparative analysis of gut microbiota
Externí odkaz:
https://doaj.org/article/23605cfe8dc144418f86ab5c7f55c061
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:
Yu, Wei, Bu, Qing-Cui, Liu, He-Xin, Huang, Yue, Zhang, Liang, Yang, Zi-Xu, Qu, Jin-Lu, Zhang, Shu, Song, Li-Ming, Zhang, Shuang-Nan, Jia, Shu-Mei, Ma, Xiang, Tao, Lian, Ge, Ming-Yu, Liu, Qing-Zhong, Yan, Jing-Zhi, Cao, Xue-Lei, Chang, Zhi, Chen, Li, Chen, Yong, Chen, Yu-Peng, Ding, Guo-Qiang, Guan, Ju, Jin, Jing, Kong, Ling-Da, Li, Bing, Li, Cheng-Kui, Li, Ti-Pei, Li, Xiao-Bo, Liao, Jin-Yuan, Liu, Bai-Sheng, Liu, Cong-Zhan, Lu, Fang-Jun, Ma, Rui-Can, Nie, Jian-Yin, Ren, Xiao-Qin, Sai, Na, Tan, Ying, Tuo, You-Li, Wang, Ling-Jun, Wang, Peng-Ju, Wu, Bai-Yang, Xiao, Guang-Cheng, Yin, Qian-Qing, You, Yuan, Zhang, Juan, Zhang, Peng, Zhang, Wei, Zhao, Hai-Sheng, Zheng, Shi-Jie, Zhou, Deng-Ke
We have performed a spectral-timing analysis on the black hole X-ray binary MAXI J1535--571 during its 2017 outburst, with the aim of exploring the evolution of the inner accretion flow geometry. X-ray reverberation lags are observed in the hard-inte
Externí odkaz:
http://arxiv.org/abs/2305.16716
Autor:
Xiao, Shuo, Tuo, You-Li, Zhang, Shuang-Nan, Xiong, Shao-Lin, Lin, Lin, Zhang, Yan-Qiu, Wang, Yue, Xue, Wang-Chen, Cai, Ce, Gao, He, Li, Cheng-Kui, Li, Xiao-Bo, Zheng, Chao, Liu, Jia-Cong, Wang, Ping, Wang, Jin, Peng, Wen-Xi, Liu, Cong Zhan, Li, Xin-Qiao, Wen, Xiang-Yang, An, Zheng-Hua, Song, Li-Ming, Zheng, Shi-Jie, Zhang, Fan, Dong, Ai-Jun, Xie, Wei, Feng, Jian-Chao, Ma, Qing-Bo, Wang, De-Hua, Luo, Xi-Hong, Dang, Shi-Jun, Shang, Lun-Hua, Zhi, Qi-Jun, Li, Ti-Pei
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 key probe to the underlying radiation mechanism. However, spectral lag
Externí odkaz:
http://arxiv.org/abs/2303.12542
Autor:
An, Zheng-Hua, Antier, S., Bi, Xing-Zi, Bu, Qing-Cui, Cai, Ce, Cao, Xue-Lei, Camisasca, Anna-Elisa, Chang, Zhi, Chen, Gang, Chen, Li, Chen, Tian-Xiang, Chen, Wen, Chen, Yi-Bao, Chen, Yong, Chen, Yu-Peng, Coughlin, Michael W., Cui, Wei-Wei, Dai, Zi-Gao, Hussenot-Desenonges, T., Du, Yan-Qi, Du, Yuan-Yuan, Du, Yun-Fei, Fan, Cheng-Cheng, Frontera, Filippo, Gao, He, Gao, Min, Ge, Ming-Yu, Gong, Ke, Gu, Yu-Dong, Guan, Ju, Guo, Dong-Ya, Guo, Zhi-Wei, Guidorzi, Cristiano, Han, Da-Wei, He, Jian-Jian, He, Jun-Wang, Hou, Dong-Jie, Huang, Yue, Huo, Jia, Ji, Zhen, Jia, Shu-Mei, Jiang, Wei-Chun, Kann, David Alexander, Klotz, A., Kong, Ling-Da, Lan, Lin, Li, An, Li, Bing, Li, Chao-Yang, Li, Cheng-Kui, Li, Gang, Li, Mao-Shun, Li, Ti-Pei, Li, Wei, Li, Xiao-Bo, Li, Xin-Qiao, Li, Xu-Fang, Li, Yan-Guo, Li, Zheng-Wei, Liang, Jing, Liang, Xiao-Hua, Liao, Jin-Yuan, Lin, Lin, Liu, Cong-Zhan, Liu, He-Xin, Liu, Hong-Wei, Liu, Jia-Cong, Liu, Xiao-Jing, Liu, Ya-Qing, Liu, Yu-Rong, Lu, Fang-Jun, Lu, Hong, Lu, Xue-Feng, Luo, Qi, Luo, Tao, Ma, Bin-Yuan, Ma, Fu-Li, Ma, Rui-Can, Ma, Xiang, Maccary, Romain, Mao, Ji-Rong, Meng, Bin, Nie, Jian-Yin, Orlandini, Mauro, Ou, Ge, Peng, Jing-Qiang, Peng, Wen-Xi, Qiao, Rui, Qu, Jin-Lu, Ren, Xiao-Qin, Shi, Jing-Yan, Shi, Qi, Song, Li-Ming, Song, Xin-Ying, Su, Ju, Sun, Gong-Xing, Sun, Liang, Sun, Xi-Lei, Tan, Wen-Jun, Tan, Ying, Tao, Lian, Tuo, You-Li, Turpin, Damien, Wang, Jin-Zhou, Wang, Chen, Wang, Chen-Wei, Wang, Hong-Jun, Wang, Hui, Wang, Jin, Wang, Ling-Jun, Wang, Peng-Ju, Wang, Ping, Wang, Wen-Shuai, Wang, Xiang-Yu, Wang, Xi-Lu, Wang, Yu-Sa, Wang, Yue, Wen, Xiang-Yang, Wu, Bo-Bing, Wu, Bai-Yang, Wu, Hong, Xiao, Sheng-Hui, Xiao, Shuo, Xiao, Yun-Xiang, Xie, Sheng-Lun, Xiong, Shao-Lin, Xiong, Sen-Lin, Xu, Dong, Xu, He, Xu, Yan-Jun, Xu, Yan-Bing, Xu, Ying-Chen, Xu, Yu-Peng, Xue, Wang-Chen, Yang, Sheng, Yang, Yan-Ji, Yang, Zi-Xu, Ye, Wen-Tao, Yi, Qi-Bin, Yi, Shu-Xu, Yin, Qian-Qing, You, Yuan, Yu, Yun-Wei, Yu, Wei, Yu, Wen-Hui, Zeng, Ming, Zhang, Bing, Zhang, Bin-Bin, Zhang, Da-Li, Zhang, Fan, Zhang, Hong-Mei, Zhang, Juan, Zhang, Liang, Zhang, Peng, Zhang, Shu, Zhang, Shuang-Nan, Zhang, Wan-Chang, Zhang, Xiao-Feng, Zhang, Xiao-Lu, Zhang, Yan-Qiu, Zhang, Yan-Ting, Zhang, Yi-Fei, Zhang, Yuan-Hang, Zhang, Zhen, Zhao, Guo-Ying, Zhao, Hai-Sheng, Zhao, Hong-Yu, Zhao, Qing-Xia, Zhao, Shu-Jie, Zhao, Xiao-Yun, Zhao, Xiao-Fan, Zhao, Yi, Zheng, Chao, Zheng, Shi-Jie, Zhou, Deng-Ke, Zhou, Xing, Zhu, Xiao-Cheng
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 properties of this burst is very challenging due to its exceptional brightnes
Externí odkaz:
http://arxiv.org/abs/2303.01203
Autor:
Xiao, Shuo, Peng, Wen-Xi, Zhang, Shuang-Nan, Xiong, Shao-Lin, Li, Xiao-Bo, Tuo, You-Li, Gao, He, Wang, Yue, Xue, Wang-Chen, Zheng, Chao, Zhang, Yan-Qiu, Liu, Jia-Cong, Li, Cheng-Kui, Yi, Shu-Xu, Wang, Xi-Lu, Zhang, Zhen, Cai, Ce, Dong, Ai-Jun, Xie, Wei, Feng, Jian-Chao, Ma, Qing-Bo, Wang, De-Hua, Luo, Xi-Hong, Zhi, Qi-Jun, Song, Li-Ming, Li, Ti-Pei
The precursors of short and long Gamma Ray Bursts (SGRBs and LGRBs) can serve as probes of their progenitors, as well as shedding light on the physical processes of mergers or core-collapse supernovae. Some models predict the possible existence of Qu
Externí odkaz:
http://arxiv.org/abs/2210.08491
Autor:
Li Ti
Publikováno v:
Open Physics, Vol 6, Iss 4, Pp 891-894 (2008)
Externí odkaz:
https://doaj.org/article/4e64eb3c7a0e42739cb9fd387b367b2d
Autor:
Kong, Ling-Da, Zhang, Shu, Zhang, Shuang-Nan, Ji, Long, Doroshenko, Victor, Santangelo, Andrea, Chen, Yu-Peng, Lu, Fang-Jun, Ge, Ming-Yu, Wang, Peng-Ju, Tao, Lian, Qu, Jin-Lu, Li, Ti-Pei, Liu, Cong-Zhan, Liao, Jin-Yuan, Chang, Zhi, Peng, Jing-Qiang, Shui, Qing-Cang
The detection of cyclotron resonance scattering features (CRSFs) is the only way to directly and reliably measure the magnetic field near the surface of a neutron star (NS). The broad energy coverage and large collection area of \emph{Insight}-HXMT i
Externí odkaz:
http://arxiv.org/abs/2206.04283
Autor:
Xiao, Shuo, Zhang, Yan-Qiu, Zhu, Zi-Pei, Xiong, Shao-Lin, Gao, He, Xu, Dong, Zhang, Shuang-Nan, Peng, Wen-Xi, Li, Xiao-Bo, Zhang, Peng, Lu, Fang-Jun, Lin, Lin, Liu, Liang-Duan, Zhang, Zhen, Ge, Ming-Yu, Tuo, You-Li, Xue, Wang-Chen, Fu, Shao-Yu, Liu, Xing, Liu, Jin-Zhong, Li, An, Wang, Tian-Cong, Zheng, Chao, Wang, Yue, Jiang, Shuai-Qing, Li, Jin-Da, Liu, Jia-Cong, Cao, Zhou-Jian, Luo, Xi-Hong, Yang, Jiao-Jiao, Yi, Shu-Xu, Wang, Xi-Lu, Cai, Ce, Yi, Qi-Bin, Zhao, Yi, Xie, Sheng-Lun, Li, Cheng-Kui, Luo, Qi, Song, Li-Ming, Zhang, Shu, Qu, Jin-Lu, Liu, Cong-Zhan, Li, Xu-Fang, Xu, Yu-Peng, Li, Ti-Pei
Publikováno v:
ApJ 970 6 (2024)
The milestone discovery of GW 170817-GRB 170817A-AT 2017gfo has shown that gravitational wave (GW) could be produced during the merger of neutron star-neutron star/black hole and that in electromagnetic (EM) wave a gamma-ray burst (GRB) and a kilonov
Externí odkaz:
http://arxiv.org/abs/2205.02186
Autor:
Song, Xin-Ying, Xiong, Shao-Lin, Zhang, Shuang-Nan, Li, Cheng-Kui, Li, Xiao-Bo, Huang, Yue, Guidorzi, Cristiano, Frontera, Filippo, Liu, Cong-Zhan, Li, Xu-Fang, Li, Gang, Liao, Jin-Yuan, Cai, Ce, Luo, Qi, Xiao, Shuo, Yi, Qi-Bin, Zheng, Yao-Guang, Zhou, Deng-Ke, Liu, Jia-Cong, Xue, Wang-Chen, Zhang, Yan-Qiu, Zheng, Chao, Chang, Zhi, Li, Zheng-Wei, Lu, Xue-Feng, Zhang, Ai-Mei, Zhang, Yi-Fei, Jin, Yong-Jie, Li, Ti-Pei, Lu, Fang-Jun, Song, Li-Ming, Wu, Mei, Xu, Yu-Peng, Ma, Xiang, Ge, Ming-Yu, Jia, Shu-Mei, Li, Bing, Nie, Jian-Yin, Wang, Ling-Jun, Zhang, Juan, Zheng, Shi-Jie, Yang, Xue-Juan, Yang, Rong-Jia
The Hard X-ray Modulation Telescope (Insight-HXMT), is China's first X-ray astronomy satellite launched on June 15, 2017. The anti-coincidence CsI detectors of the High Energy X-ray telescope (HE) onboard Insight-HXMT could serve as an all-sky gamma-
Externí odkaz:
http://arxiv.org/abs/2203.00878