In-orbit timing calibration of the Insight-Hard X-ray Modulation Telescope
Youli Tuo, Xiaobo Li, Mingyu Ge, Jianyin Nie, Liming Song, Yupeng Xu,, Shijie Zheng, Fangjun Lu, Shuang-Nan Zhang, Congzhan Liu, Xuelei Cao, Yong, Chen, Jinlu Qu, Shu Zhang, Haisheng Zhao, Shuo Xiao, Baiyang Wu, Xiangyang, Wen, Weichun Jiang, Bin Meng, Weiwei Cui, Wei Li

TL;DR
This paper details the timing calibration process for Insight-HXMT's three X-ray payloads, including correction methods for temperature effects and long-term oscillator variations, verified through Crab pulsar observations and NICER comparisons.
Contribution
It introduces a novel calibration method for temperature-dependent and long-term timing variations in Insight-HXMT's payloads, improving timing accuracy for X-ray observations.
Findings
Timing system accuracy achieved within 12.1-15.8 microseconds.
Calibration method effectively corrects temperature and oscillator variations.
Systematic timing errors characterized for all three payloads.
Abstract
We describe the timing system and the timing calibration results of the three payloads on-board the Insight-Hard X-ray Modulation Telescope (Insight-HXMT). These three payloads are the High Energy X-ray telescope (HE, 20-250 keV), the Medium Energy X-ray telescope (ME, 5-30 keV) and the low Energy X-ray telescope (LE, 1-10 keV). We present a method to correct the temperature-dependent period response and the long-term variation of the on-board crystal oscillator, especially for ME that does not carry a temperature-compensated crystal oscillator. The time of arrivals (ToAs) of the Crab pulsar are measured to evaluate the accuracy of the timing system. As the ephemeris of the Crab pulsar given by Jodrell Bank observatory has systematic errors around 40 {\mu}s (Rots et al. 2014), we use the quasi-simultaneous observations of the X-ray Timing Instrument (XTI) on-board the Neutron star…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Superconducting and THz Device Technology
