Zobrazeno 1 - 10
of 29
pro vyhledávání: '"Dang Shi-Jun"'
Autor:
You, Zi-Yi, Pan, Yun-Rong, Ma, Zhi, Zhang, Li, Xiao, Shuo, Zhang, Dan-Dan, Dang, Shi-Jun, Zhao, Ru-Shuang, Wang, Pei, Dong, Ai-Jun, Jiang, Jia-Tao, Leng, Ji-Bing, Li, Wei-An, Li, Si-Yao
Pulsar search is always the basis of pulsar navigation, gravitational wave detection and other research topics. Currently, the volume of pulsar candidates collected by Five-hundred-meter Aperture Spherical radio Telescope (FAST) shows an explosive gr
Externí odkaz:
http://arxiv.org/abs/2311.08134
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, Li, Xiao-Bo, Xue, Wang-Chen, Xiong, Shao-Lin, Zhang, Shuang-Nan, Peng, Wen-Xi, Dong, Ai-Jun, Tuo, You-Li, Cai, Ce, Luo, Xi-Hong, Yang, Jiao-Jiao, Wang, Yue, Zheng, Chao, Zhang, Yan-Qiu, Liu, Jia-Cong, Tan, Wen-Jun, Wang, Chen-Wei, Wang, Ping, Li, Cheng-Kui, Yi, Shu-Xu, Dang, Shi-Jun, Shang, Lun-Hua, Zhao, Ru-Shuang, Ma, Qing-Bo, Xie, Wei, Feng, Jian-Chao, Zhang, Bin, Zhang, Zhen, Ge, Ming-Yu, Zheng, Shi-Jie, Song, Li-Ming, Zhi, Qi-Jun
The study of quasi-periodic oscillations (QPOs) and power density spectra (PDS) continuum properties can help shed light on the still illusive emission physics of magnetars and as a window into the interiors of neutron stars using asteroseismology. I
Externí odkaz:
http://arxiv.org/abs/2307.14884
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:
Li, Wei, Dang, Shi-Jun, Yuan, Jian-Ping, Li, Lin, Wang, Wei-Hua, Shang, Lun-Hua, Wang, Na, Li, Qing-Ying, Lu, Ji-Guang, Kou, Fei-Fei, Wang, Shuang-Qiang, Xiao, Shuo, Zhi, Qi-Jun, Liu, Yu-Lan, Zhao, Ru-Shuang, Dong, Ai-Jun, Zhang, Bin, You, Zi-Yi, Cai, Yan-Qing, Yang, Ya-Qin, Ren, Ying-Ying, Liu, Yu-Jia, Xu, Heng
In this paper, we presented the 23.3 years of pulsar timing results of PSR J1456-6413 based on the observation of Parkes 64m radio telescope. We detected two new glitches at MJD 57093(3) and 59060(12) and confirmed its first glitch at MJD 54554(10).
Externí odkaz:
http://arxiv.org/abs/2306.13611
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
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
Timing observations from the Nanshan 26-m radio telescope for nine pulsars between 2000 and 2014 have been used to search for glitches. The data span for nine pulsars ranges from 11.6 to 14.2 years. From the total of 114 yr of pulsar rotational histo
Externí odkaz:
http://arxiv.org/abs/2206.12886
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Akademický článek
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