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	New pulse profile variability associated with a glitch of PSR J0738-4042 期刊论文 OAI收割 Monthly Notices of the Royal Astronomical Society, 2022, 卷号: 519, 期号: 1, 页码: 74-84 作者: Zhou, S. Q.; Guegercinoglu, E.; Yuan, J. P.; Ge, M. Y.; Yu, C. \| 收藏 \| 浏览/下载：14/0 \| 提交时间：2023/06/19 methods: data analysis stars:neutron pulsars: general pulsars: individual: (PSR J0738-4042) gamma-ray pulsar vortex creep timing observations neutron-stars crab pulsar inclination angle braking indexes magnetic-field radio pulsars state change Astronomy & Astrophysics
	A model to obtain timing solution with un-differenced observations suitable for single-station/multi-station, a case study of BDS data 期刊论文 OAI收割 ACTA GEODAETICA ET GEOPHYSICA, 2020, 页码: 15 作者: Zhang, Pengfei; Tu, Rui; Zhang, Rui; Han, Junqiang; Fan, Lihong \| 收藏 \| 浏览/下载：13/0 \| 提交时间：2020/09/01 BeiDou Satellite Navigation System Un-differenced observations Precise timing service Solution model
	Timing analysis of Swift J1658.2-4242's outburst in 2018 with Insight-HXMT, NICER and AstroSat 期刊论文 OAI收割 Journal of High Energy Astrophysics, 2019, 卷号: 24, 页码: 30-40 作者: HXMT \| 收藏 \| 浏览/下载：57/0 \| 提交时间：2022/02/08 Accretion accretion disks Black hole physics X-rays: binaries: Swift J1658.2-4242 Astrophysics - High Energy Astrophysical Phenomena Abstract: We present the observational results from a detailed timing analysis of the black hole candidate Swift J1658.2-4242 during its 2018 outburst with the observations of Hard X-ray Modulation Telescope (Insight-HXMT), Neutron Star Interior Composition Explorer (NICER) and AstroSat in 0.1-250 keV. The evolution of intensity, hardness and integrated fractional root mean square (rms) observed by Insight-HXMT and NICER are presented in this paper. Type-C quasi-periodic oscillations (QPOs) observed by NICER (0.8-3.5 Hz) and Insight-HXMT (1-1.6 Hz) are also reported in this work. The features of the QPOs are analyzed with an energy range of 0.5-50 keV. The relations between QPO frequency and other characteristics such as intensity, hardness and QPO rms are carefully studied. The timing and spectral properties indicate that Swift J1658.2-4242 is a black hole binary system. Besides, the rms spectra of the source calculated from the simultaneous observation of Insight-HXMT, NICER and AstroSat support the Lense-Thirring origin of the QPOs. The relation between QPO phase lag and the centroid frequency of Swift J1658.2-4242 reveals a near zero constant when < 4Hz and a soft phase lag at 6.68 Hz. This independence follows the same trend as the high inclination galactic black hole binaries such as MAXI J1659-152.