Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Shi-Jun Dang"'
Autor:
Shuo Xiao, Mei-Xin Hong, Zi-Yi You, Tong-Lei Liao, Shao-Lin Xiong, Shu-Xu Yi, Ping Wang, Jiao-Jiao Yang, Zheng-Huo Jiang, Yue Wang, Yan-Qiu Zhang, Ming-Yu Ge, Zhen Zhang, Xi-Hong Luo, Shi-Jun Dang, Ru-shuang Zhao, Ai-Jun Dong, Qi-Jun Zhi, He Gao, Di Li, Shuang-Nan Zhang
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 274, Iss 1, p 14 (2024)
The overall temporal and spectral characteristics (e.g., duration, fluence, peak flux, peak count rate, and total counts) of X-ray bursts (XRBs) originating from magnetars have been extensively studied to confirm their self-organized criticality (SOC
Externí odkaz:
https://doaj.org/article/7231e63741ec46278ef806bc41468e6f
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:
Zhi Ma, Zi-Yi You, Ying Liu, Shi-Jun Dang, Dan-Dan Zhang, Ru-Shuang Zhao, Pei Wang, Si-Yao Li, Ai-Jun Dong
Publikováno v:
Universe, Vol 8, Iss 9, p 461 (2022)
Pulsar candidate sifting is an essential part of pulsar analysis pipelines for discovering new pulsars. To solve the problem of data mining of a large number of pulsar data using a Five-hundred-meter Aperture Spherical radio Telescope (FAST), a paral
Externí odkaz:
https://doaj.org/article/9006505440504700a53790ad34b5268f
Autor:
Jun-Tao, Bai, Xin, Xu, Quan-Wei, Lin, Qi-Jun, Zhi, Lun-Hua, Shang, Yuan-Jie, Du, You-Li, Tuo, Shi-Jun, Dang, Shuang-Qiang, Wang, Ru-Shuang, Zhao, Ai-Jun, Dong, Guo-Jun, Qiao
Publikováno v:
In New Astronomy February 2021 83
Publikováno v:
Research in Astronomy and Astrophysics. 22:095008
Pulsar timing measurements with a 26 m radio telescope at Nanshan between 2000 and 2014 were used to search for glitch events. The data span of nine pulsars ranges from 11.6 to 14.2 yr, and 16 new glitch events were identified in nine pulsars. Glitch
Autor:
Hua Shen, Bei Xiaomin, J. T. Bai, LinLi Yan, Qi-Jun Zhi, Shi-Jun Dang, Guojun Qiao, Yuanjie Du, Qingqing Lin, Jiguang Lu, Youli Tuo, LunHua Shang, Rihong Zhu, Liangwei Huang, Zhang Xinyuan, XiangQun Cui
Publikováno v:
Science China Physics, Mechanics & Astronomy. 63
The pulse profiles of the Crab pulsar (as well as some other pulsars) vary with time. They can lead to a major source of intrinsic timing noise, which lacks a detailed physical model. The phase separation Δ between the first left peak (P1) and the s
Publikováno v:
Astrophysics and Space Science. 365
Using the archival data of the Neutron star Interior Composition Explorer, we study the evolution of two-peak phase separations of the Crab pulsar’s X-ray pulse profiles, and present a possible method to predict the next glitch epochs of the Crab p
Publikováno v:
Research in Astronomy and Astrophysics. 22:025018
We report the “Bi-drifting” subpulses observed in PSR J0815+0939 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The observation at band from 1050 to 1450 MHz is evenly divided into two bands, i.e., the bands at center fre