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ACTA AERONAUTICAET ASTRONAUTICA SINICA ›› 2023, Vol. 44 ›› Issue (3): 526588.doi: 10.7527/S1000-6893.2022.26588

• Articles • Previous Articles     Next Articles

Timing analysis for five navigation X-ray pulsars

Linli YAN1, Mingyu GE2(), Youli TUO2, Qingyong ZHOU3,4, Wentao YE2, Shijie ZHENG2, Dawei HAN2   

  1. 1.School of Mathematics and Physics,Anhui Jianzhu University,Hefei  230601,China
    2.Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing  100049,China
    3.Xi’an Institute of Surveying and Mapping,Xi’an  710054,China
    4.State Key Laboratory of Geographic Information Engineering,Xi’an  710054,China
  • Received:2021-10-29 Revised:2021-11-22 Accepted:2022-02-13 Online:2023-02-15 Published:2022-02-17
  • Contact: Mingyu GE E-mail:gemy@ihep.ac.cn
  • Supported by:
    National Key R&D Program of China(2021YFA0718500);Strategic Priority Program on Space Science, Chinese Academy of Sciences(XDA15020503);National Natural Science Foundation of China(11903001);Key Project of Natural Science Research Project of Universities of Anhui Province(KJ2019A0787);Doctor Foundation of Anhui Jianzhu University(2019QDZ14)

Abstract:

The timing analysis of pulsars, the basis for pulsar navigation and pulsar time research, provides accurate timing model parameters and radiation information of the pulsar. This work provides a systematic summary of pulsar timing analysis methods and timing analysis results of the five most widely used pulsars in current pulsar navigation including the Crab pulsar and PSR B1509-58 whose observations are made from the “Insight”Hard X-ray Modulation Telescope (HXMT) in China, and PSRs J1821-2452A, J1939+2134 and J0030 +0451 whose observations are made from the Neutron-star Interior Composition Explorer (NICER). Through the analysis of high precision timing observations from “Insight” HXMT and NICER in 2017-2021, the latest rotation characteristics and physical information of pulsars are obtained. On the one hand, the latest X-ray ephemeris of the pulsar with long period time and higher accuracy of rotation parameters are given, and it is proved that high precision ephemeris can be obtained independently in X-ray. On the other hand, clear and significant integrated pulse profiles for five pulsars are established, in which the pulse profiles of the three millisecond pulsars within the selected energy bands are the most accurate, which can provide the latest standard template for pulsar navigation research. This work only analyzes the X-ray observations of pulsars, and using multiple telescopes at home and abroad to carry out multi-band joint timing analysis will be an important direction of pulsar timing research in the future.

Key words: pulsar, navigation, X-ray, timing analysis, ephemeris

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