Zobrazeno 1 - 10
of 18 614
pro vyhledávání: '"Ye W."'
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
Publikováno v:
International Journal of General Medicine, Vol Volume 17, Pp 4769-4780 (2024)
Liu Liang,1 Xuemin Guo,1 Wei Ye,1 Yuxiang Liu2 1Department of Laboratory Medicine, Meizhou People’s Hospital, Meizhou, People’s Republic of China; 2Department of Medical Oncology, Meizhou People’s Hospital, Meizhou, People’s Republic of China
Externí odkaz:
https://doaj.org/article/fefc12e1eda24e46bf9aa81b757c5a5a
Publikováno v:
Neuropsychiatric Disease and Treatment, Vol Volume 20, Pp 1879-1887 (2024)
Zeqiang Ji,1,2 Wanxing Ye,2 Xinyu Wen,1,2 Xingquan Zhao,1– 4,* Na Li1– 3,* 1Department of Neurology, Beijing Tiantan Hospital, Capital Medical University, Beijing, People’s Republic of China; 2China National Clinical Research Center for
Externí odkaz:
https://doaj.org/article/538a13a1679948648ae74ef5263467f4
Publikováno v:
Helminthologia, Vol 53, Iss 1, Pp 62-75 (2016)
During a nematode biodiversity survey from 2012 to 2014 in Shenzhen, China, ten nematode populations (SZX1301–SZX1310) of Xiphinema were recovered from rhizosphere of different plants, namely Acacia mangium (SZX1306), A. confuse (SZX1309), Blechnum
Externí odkaz:
https://doaj.org/article/6fc5ab40f88f4932ad8f1c320af98b59
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