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In-orbit demonstration of X-ray pulsar navigation with the Insight-HXMT satellite

Authors :
Zheng, S. J.
Zhang, S. N.
Lu, F. J.
Wang, W. B.
Gao, Y.
Li, T. P.
Song, L. M.
Ge, M. Y.
Han, D. W.
Chen, Y.
Xu, Y. P.
Cao, X. L.
Liu, C. Z.
Zhang, S.
Qu, J. L.
Chang, Z.
Chen, G.
Chen, L.
Chen, T. X.
Chen, Y. B.
Chen, Y. P.
Cui, W.
Cui, W. W.
Deng, J. K.
Dong, Y. W.
Du, Y. Y.
Fu, M. X.
Gao, G. H.
Gao, H.
Gao, M.
Gu, Y. D.
Guan, J.
Gungor, C.
Guo, C. C.
Hu, W.
Huang, Y.
Huo, J.
Ji, J. F.
Jia, S. M.
Jiang, L. H.
Jiang, W. C.
Jin, J.
Jin, Y. J.
Li, B.
Li, C. K.
Li, G.
Li, M. S.
Li, W.
Li, X.
Li, X. B.
Li, X. F.
Li, Y. G.
Li, Z. J.
Li, Z. W.
Liang, X. H.
Liao, J. Y.
Liu, G. Q.
Liu, H. W.
Liu, S. Z.
Liu, X. J.
Liu, Y.
Liu, Y. N.
Lu, B.
Lu, X. F.
Luo, T.
Ma, X.
Meng, B.
Nang, Y.
Nie, J. Y.
Ou, G
Sai, N.
Shang, R. C.
Sun, L.
Tan, Y.
Tao, L.
Tao, W.
Tuo, Y. L.
Wang, G. F.
Wang, J.
Wang, W. S.
Wang, Y. S.
Wen, X. Y.
Wu, B. B.
Wu, M.
Xiao, G. C.
Xiong, S. L.
Xu, H.
Yan, L. L.
Yang, J. W.
Yang, S.
Yang, Y. J.
Zhang, A. M.
Zhang, C. L.
Zhang, C. M.
Zhang, F.
Zhang, H. M.
Zhang, J.
Zhang, Q.
Zhang, T.
Zhang, W.
Zhang, W. C.
Zhang, W. Z.
Zhang, Y.
Zhang, Y. F.
Zhang, Y. J.
Zhang, Z.
Zhang, Z. L.
Zhao, H. S.
Zhao, J. L.
Zhao, X. F.
Zhu, Y.
Zhu, Y. X.
Zou, C. L.
Publication Year :
2019

Abstract

In this work, we report the in-orbit demonstration of X-ray pulsar navigation with Insight-Hard X-ray Modulation Telescope (Insight-HXMT), which was launched on Jun. 15th, 2017. The new pulsar navigation method 'Significance Enhancement of Pulse-profile with Orbit-dynamics' (SEPO) is adopted to determine the orbit with observations of only one pulsar. In this test, the Crab pulsar is chosen and observed by Insight-HXMT from Aug. 31th to Sept. 5th in 2017. Using the 5-day-long observation data, the orbit of Insight-HXMT is determined successfully with the three telescopes onboard - High Energy X-ray Telescope (HE), Medium Energy X-ray Telescope (ME) and Low Energy X-ray Telescope (LE) - respectively. Combining all the data, the position and velocity of the Insight-HXMT are pinpointed to within 10 km (3 sigma) and 10 m/s (3 sigma), respectively.<br />Comment: Accepted by the Astrophysical Journal Supplement

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1908.01922
Document Type :
Working Paper
Full Text :
https://doi.org/10.3847/1538-4365/ab3718