基于 Insight-HXMT 卫星的 X 射线脉冲星导航在轨演示
天体物理仪器与方法
2019-09-04 v1
摘要
在这项工作中，我们报道了利用 2017 年 6 月 15 日发射的 Insight-硬 X 射线调制望远镜（Insight-HXMT）进行的 X 射线脉冲星导航在轨演示。采用新的脉冲星导航方法“基于轨道动力学增强脉冲轮廓显著性”（SEPO）仅利用一颗脉冲星的观测来确定轨道。在此次测试中，选取 Crab 脉冲星并由 Insight-HXMT 于 2017 年 8 月 31 日至 9 月 5 日进行观测。利用长达 5 天的观测数据，分别利用星载三台望远镜——高能 X 射线望远镜（HE）、中能 X 射线望远镜（ME）和低能 X 射线望远镜（LE）——成功确定了 Insight-HXMT 的轨道。综合所有数据，Insight-HXMT 的位置和速度分别被精确定位至 10 km（3 sigma）和 10 m/s（3 sigma）以内。
引用
@article{arxiv.1908.01922,
title = {In-orbit demonstration of X-ray pulsar navigation with the Insight-HXMT satellite},
author = {S. J. Zheng and S. N. Zhang and F. J. Lu and W. B. Wang and Y. Gao and T. P. Li and L. M. Song and M. Y. Ge and D. W. Han and Y. Chen and Y. P. Xu and X. L. Cao and C. Z. Liu and S. Zhang and J. L. Qu and Z. Chang and G. Chen and L. Chen and T. X. Chen and Y. B. Chen and Y. P. Chen and W. Cui and W. W. Cui and J. K. Deng and Y. W. Dong and Y. Y. Du and M. X. Fu and G. H. Gao and H. Gao and M. Gao and Y. D. Gu and J. Guan and C. Gungor and C. C. Guo and D. W. Han and W. Hu and Y. Huang and J. Huo and J. F. Ji and S. M. Jia and L. H. Jiang and W. C. Jiang and J. Jin and Y. J. Jin and B. Li and C. K. Li and G. Li and M. S. Li and W. Li and X. Li and X. B. Li and X. F. Li and Y. G. Li and Z. J. Li and Z. W. Li and X. H. Liang and J. Y. Liao and G. Q. Liu and H. W. Liu and S. Z. Liu and X. J. Liu and Y. Liu and Y. N. Liu and B. Lu and X. F. Lu and T. Luo and X. Ma and B. Meng and Y. Nang and J. Y. Nie and G Ou and N. Sai and R. C. Shang and L. Sun and Y. Tan and L. Tao and W. Tao and Y. L. Tuo and G. F. Wang and J. Wang and W. S. Wang and Y. S. Wang and X. Y. Wen and B. B. Wu and M. Wu and G. C. Xiao and S. L. Xiong and H. Xu and L. L. Yan and J. W. Yang and S. Yang and Y. J. Yang and A. M. Zhang and C. L. Zhang and C. M. Zhang and F. Zhang and H. M. Zhang and J. Zhang and Q. Zhang and T. Zhang and W. Zhang and W. C. Zhang and W. Z. Zhang and Y. Zhang and Y. Zhang and Y. F. Zhang and Y. J. Zhang and Z. Zhang and Z. Zhang and Z. L. Zhang and H. S. Zhao and J. L. Zhao and X. F. Zhao and Y. Zhu and Y. X. Zhu and C. L. Zou},
journal= {arXiv preprint arXiv:1908.01922},
year = {2019}
}
备注
Accepted by the Astrophysical Journal Supplement