The Astrophysical Journal Supplement Series (Jan 2023)
Pulsar and Magnetar Navigation with Fermi/GBM and GECAM
- 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
Affiliations
- Xi-Hong Luo
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Shuo Xiao
- ORCiD
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Shi-Jie Zheng
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Ming-Yu Ge
- ORCiD
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- You-Li Tuo
- ORCiD
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]; Institut für Astronomie und Astrophysik, University of Tübingen , Sand 1, D-72076 Tübingen, Germany
- Shao-Lin Xiong
- ORCiD
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Shuang-Nan Zhang
- ORCiD
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]; University of Chinese Academy of Sciences, Chinese Academy of Sciences , Beijing 100049, People's Republic of China
- Fang-Jun Lu
- ORCiD
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Yue Huang
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Cheng Yang
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Qi-Jun Zhi
- ORCiD
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Li-Ming Song
- ORCiD
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Wen-Xi Peng
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Xiang-Yang Wen
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Xin-Qiao Li
- ORCiD
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Zheng-Hua An
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Jin Wang
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Ping Wang
- ORCiD
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Ce Cai
- ORCiD
- College of Physics, Hebei Normal University , 20 South Erhuan Road, Shijiazhuang 050024, People's Republic of China
- Cheng-Kui Li
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Xiao-Bo Li
- ORCiD
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Fan Zhang
- Key Laboratory of Particle Astrophysics, Institute of High Energy Physics , Chinese Academy of Sciences, Beijing 100049, People's Republic of China [email protected], [email protected]
- Ai-Jun Dong
- ORCiD
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Wei Xie
- ORCiD
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Jian-Chao Feng
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Qing-Bo Ma
- ORCiD
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Hua Wang De
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Lun-Hua Shang
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Xin Xu
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Meng-Xuan Zhang
- School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Zi-Ping Dong
- School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- Shi-Jun Dang
- Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University , Guiyang 550001, People’s Republic of China [email protected]; School of Physics and Electronic Science, Guizhou Normal University , Guiyang 550001, People’s Republic of China ; [email protected]
- DOI
- https://doi.org/10.3847/1538-4365/acc79d
- Journal volume & issue
-
Vol. 266,
no. 1
p. 16
Abstract
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 position autonomously may perform better than those that must rely on transmission solutions. In this work, we report an absolute navigation accuracy of ∼20 km using 16 day Crab pulsar data observed with Fermi’s Gamma-ray Burst Monitor (GBM). In addition, we propose a new method with the inverse process of the triangulation for joint navigation using repeated bursts like those from the magnetar SGR J1935+2154 observed by the Gravitational-wave High-energy Electromagnetic Counterpart All-sky Monitor and GBM.
Keywords
