Zobrazeno 1 - 10
of 62
pro vyhledávání: '"Ye, W. T."'
Autor:
Liu, P., Yuan, J. -P., Ge, M. -Y., Ye, W. -T., Zhou, S. -Q., Dang, S. -J., Zhou, Z. -R., Gügercinoğlu, E., Tu, Z. H., Wang, P., Li, A., Li, D., Wang, N.
Pulsar glitch is a phenomenon characterized by abrupt changes in the spin period over less than a minute. We present a comprehensive analysis of glitches in four gamma-ray pulsars by combining the timing observation data of \textit{Fermi} Large Area
Externí odkaz:
http://arxiv.org/abs/2408.15022
Autor:
Zhou, S. Q., Ye, W. T., Ge, M. Y., GügercinoğLu, E., Zheng, S. J., Yu, C., Yuan, J. P., Zhang, J.
Through a detailed timing analysis of $\textit{Fermi}$-LAT data, the rotational behavior of the $\gamma$-ray pulsar PSR J1522$-$5735 was tracked from August 2008 (MJD 54692) to January 2024 (MJD 60320). During this 15.4-year period, two over-recovery
Externí odkaz:
http://arxiv.org/abs/2408.09204
Autor:
Li, P. P., Tao, L., Ma, R. C., Ge, M. Y., Zhao, Q. C., Zhao, S. J., Zhang, L., Bu, Q. C., Kong, L. D., Tuo, Y. L., Ji, L., Zhang, S., Qu, J. L., Zhang, S. N., Huang, Y., Ma, X., Ye, W. T., Shui, Q. C.
We present a comprehensive timing analysis on the Be/X-ray binary pulsar RX J0440.9+4431 using observations from \textit{NICER} and \textit{Insight}-HXMT during the 2022--2023 outburst. The power density spectrum (PDS) of RX J0440.9+4431 exhibits typ
Externí odkaz:
http://arxiv.org/abs/2402.14226
Autor:
Xiao, Y. X., Xu, Y. J., Ge, M. Y., Lu, F. J., Zhang, S. N., Zhang, S., Tao, L., Qu, J. L., Wang, P. J., Kong, L. D., Tuo, Y. L., You, Y., Zhao, S. J., Peng, J. Q., Du, Y. F., Zhang, Y. H., Ye, W. T.
We report the phase-resolved spectral results of the first Galactic Pulsating Ultra-Luminous X-ray source (PULX) Swift J0243.6+6124, modeling at its 2017-2018 outburst peak using data collected by the Hard X-ray Modulation Telescope (Insight-HXMT). T
Externí odkaz:
http://arxiv.org/abs/2401.15992
Autor:
Liu, P., Yuan, J. -P., Ge, M. -Y., Ye, W. -T., Zhou, S. -Q., Dang, S. -J., Zhou, Z. -R., Gügercinoğlu, E., Wang, W. -H., Wang, P., Li, A., Li, D., Wang, N.
Publikováno v:
MNRAS 533, 4274-4286 (2024)
PSR J1048$-$5832 (B1046$-$58) is a Vela-like pulsar that has exhibited multiple glitch events. In this study, we analyze the timing data spanning nearly 16 years, acquired from both the Fermi Gamma-ray Space Telescope and the Parkes 64 m radio telesc
Externí odkaz:
http://arxiv.org/abs/2312.04305
Autor:
Li, P. P., Tao, L., Tuo, Y. L., Ge, M. Y., Kong, L. D., Zhang, L., Bu, Q. C., Ji, L., Qu, J. L., Zhang, S., Zhang, S. N., Huang, Y., Ma, X., Ye, W. T., Zhao, Q. C., Ma, R. C., Zhao, S. J., Hou, X., Yang, Z. X., Wang, P. J., Jia, S. M., Shui, Q. C., Guan, J.
RX J0440.9+4431, a Be/X-ray binary, had its brightest outburst in 2022 since its discovery, with a peak X-ray flux of 2.25 Crab (as recorded by Swift/BAT, 15-50 keV). We analyze the timing properties of this giant outburst using data from Insight-HXM
Externí odkaz:
http://arxiv.org/abs/2309.14858
Autor:
Li, P. P., Tao, L., Zhang, L., Bu, Q. C., Qu, J. L., Ji, L., Wang, P. J., Chen, Y. P., Zhang, S., Ma, R. C., Yang, Z. X., Ye, W. T., Zhao, S. J., Zhao, Q. C., Huang, Y., Ma, X., Qiao, E. L., Jia, S. M., Zhang, S. N.
MAXI J181-195 is a newly discovered accreting millisecond X-ray pulsar that went outburst in June 2022. Through timing analysis with NICER and NuSTAR observations, we find a transient modulation at ~2.5 Hz during the decay period of MAXI J1816-195. T
Externí odkaz:
http://arxiv.org/abs/2307.13955
Autor:
Liu, P, Yuan, J -P, Ge, M -Y, Ye, W -T, Zhou, S -Q, Dang, S -J, Zhou, Z -R, Gügercinoğlu, E, Wang, W -H, Wang, P, Li, A, Li, D, Wang, N
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Oct2024, Vol. 533 Issue 4, p4274-4286, 13p
Akademický článek
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Timing properties of the X-ray accreting pulsar RX J0440.9+4431 studied with Insight-HXMT and NICER.
Autor:
Li, P P, Tao, L, Tuo, Y L, Ge, M Y, Kong, L D, Zhang, L, Bu, Q C, Ji, L, Qu, J L, Zhang, S, Zhang, S N, Huang, Y, Ma, X, Ye, W T, Zhao, Q C, Ma, R C, Zhao, S J, Hou, X, Yang, Z X, Wang, P J
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Dec2023, Vol. 526 Issue 3, p3637-3651, 15p