UT1 measurement and service, EOP prediction, Earth Rotation
Radio Astronomy, VLBI astrometry, maser, Milky Way Structure

2001 - 2005, Nanjing University of Aeronautics and Astronautics (NUAA), bachelor degree, applied physics
2007 - 2010, Purple Mountain Observotary, Chinese Academy of Sciences, master degree, astrophysics
2010 - 2013, Purple Mountain Observotary, Chinese Academy of Sciences, ph.D degree, astrophysics

2010 - 2013, Max-Plank institue for radio astronomy (MPIfR), pre doctor
2014 - 2017, National Astronomical Observatory of Jpan (NAOJ), Mizusawa VLBI observatory, post doctor
2017 - now, Time Service Center of Chinese Academy of Sciences

（1）Searching Masers from the Sgr Stellar Stream   2022年中澳甚长基线干涉测量研讨会   2022-10-20
（2）EOP Prediction for the 2nd EOPPCC of NTSC   第二届国际EOP预报竞赛在线研讨会   2022-02-14
（3）国家授时中心自主世界时测量与服务系统   2021年全国时间频率学术会议   2021-10-28
（4）基于有效角动量函数的UT1和极移预报   2021年全国时间频率学术会议   2021-10-28
（5）The NTSC geodetic VLBI system and its application of UT1 measurements   2021国际测地学大会   2021-06-30
（6）国家授时中心测地VLBI等领域的工作进展   2020年中国天文学年会   2020-10-12
（7）VLBI Maser Astrometry of SFRs in the Sagittarius Spiral Arm   射电天文前沿与技术研讨会   2020-04-20

BeSSeL project, http://www3.mpifr-bonn.mpg.de/staff/abrunthaler/BeSSeL/index.shtml

现指导学生

李西顺  博士研究生  081001-通信与信息系统  

张泽文  硕士研究生  070402-天体测量与天体力学  

王伟龙  硕士研究生  080402-测试计量技术及仪器  

National Prize for National in Sciences (second class) in 2020

https://orcid.org/my-orcid?orcid=0000-0003-3188-5983

EOP measurement and service

(1)“国家授时中心自主世界时测量与服务系统”，2022，时频学报，45卷3期，184-193页，吴元伟，李西顺，孙保琪，尹东山，姚当，马浪明，刘佳，杨海彦，高玉平，杨旭海，张首刚

(2)“基于有效角动量函数的多参数极移预报”，2022，天文学报，63卷4期，47-57页，赵鑫，吴元伟，杨新宇，杨旭海，张首刚

(3)“Multi-parameter Polar Motion Prediction Based on Effective Angular Momentum Function”2022，Chinese Astronomy and Astrophysics, Vol 46, Issue 4, P486-499, Zhao Xin, Wu Yuan-wei, Yang Xin-yu,Yang Xu-hai, Zhang, Shou-gang 

(4)“Improved Prediction of Polar motions by piecewise parameterization”, 2022, Artificial Satellites, Vol. 57, P290-299, Yuanwei WU, Xin ZHAO, Xinyu YANG

(5)“基于超快速ΔLOD/UT1融合的近实时UT1序列”2022，仪器仪表学报，43卷8期，17-24页， 李西顺，吴元伟，杨旭海，张首刚

(6)“基于国内宽带VLBI系统及iGMAS的UT1/△LOD数据融合方法”，2022，系统工程与电子技术，44卷4期，28-35页, 李西顺，吴元伟，姚当，刘佳，马浪明，杨旭海，张首刚

(7) “The NTSC VLBI System and its application in UT1 measurement”, 2020, Research in Astronomy and Astrophysics (RAA), Vol. 20, Issue 6, P93-102，Yao Dang, Wu Yuan-wei, Zhang Bo, Sun Jing，Sun, Yan， Xu Shuang-jing，Liu Jia， Ma Langming，Gong Jian-Jun，Yang Ying，Yang Xu-Hai

 

VLBI astrometry/Milky Way structure

(1) “Trigonometric Parallaxes of Star-forming Regions beyond the Tangent Point of the Sagittarius Spiral Arm”, Astrophysical Journal (ApJ), 2019, Vol. 847, P94-106, Y. W. Wu, M. J. Reid, N. Sakai, T. M. Dame, K. M. Menten, A. Brunthaler, Y. Xu, J. J. Li, B. Hu, B. Zhang, K. J. Rygl, X. W. Zheng

(2)“Revisiting LSI +61^o303 with VLBI astrometry”, Monthly Notices of Royal Astronomical Society (MNRAS), 2018, Y. W. Wu, G. Torricelli-Ciamponi, M. Massi, M. J. Reid, B. Zhang, L. Shao, X. W. Zheng

(3)“Trigonometric Parallaxes of Star Forming Regions in the Sagittarius Spiral Arm”, 2014, A&A, 2014, Vol. 566,P17-44, Y. W. Wu; M. Sato; M. J. Reid; L. Moscadeli; B. Zhang; Y. Xu; A. Brunthaler; K. M. Menten; T. M. Dame; X. W. Zheng

(4)“Trigonometric Parallaxes of High-mass Star-forming Regions: Our View of the Milky Way”; 2019, ApJ, Vol. 885, P131, Reid, M. J.; Menten, K. M.; Brunthaler, A.; Zheng, X. W.; Dame, T. M.; Xu, Y.; Li, J.; Sakai, N.; Wu, Y.; Immer, K.; Zhang, B.; Sanna, A.; Moscadelli, L.; Rygl, K. L. J.; Bartkiewicz, A.; Hu, B.; Quiroga-Nuñez, L. H.; van Langevelde, H. J，

(5)“基于天文开源软件的卫星干涉测量数据处理系统”，2021, 天文学报，62卷, 4期，40-57页，朱梦祎，吴元伟，姚当，弓剑军，刘佳，李西顺，马浪明，韦沛，雷辉，杨旭海

(6)“The spiral structure of the Milky Way”, 2018, RAA, Vol.18, P146，Ye Xu, Li-Gang Hou, Yuan-wei, Wu 

(7)“The chniques for Accurate Parallax Measurements for 6.7 GHz Methanol Masers”, 2017, AJ, 154, 63,Reid, M.J., Brunthaler, A., Menten, K.M., Sanna, A., Xu, Y., Li, J.J., Wu, Y., Hu, B., Zheng, X. W., Zhang, B., Immer, K., Rygl, K., Moscadeli, L., Sakai, N., Bartkiewicz, A., Choi, Y,K.

 

Maser

(1)“Water-mase survey towards off-plane O-rich AGBs around the orbital plane of the Sagittarius stellar stream”, 2022, MNRAS, Vol. 516, P1881-1893，Yuanwei Wu, Bo Zhang, Jingjing Li, Xing-Wu Zheng

(2)“SiO Maser Survey towards off-plane O-rich AGBs around the orbital plane of the Sagittarius Stellar Stream”, 2018, MNRAS，Vo. 473, P3325-3350, Y. W. Wu, Noriyuki Matsunaga, Ross A. Burns4, B. Zhang

(3)“Ammonia and CO Observations Towards Low-luminosity 6.7 GHz Methanol Masers”, 2010 ApJ, Vol.720, P392,Wu, Y. W.; Xu, Y.; Pandian, J. D.; Yang, J.; Henkel, C.; Menten, K. M.; Zhang, S. B. 

(4)“Multiwavelength study of low-luminosity 6.7 GHz Methanol Masers”, 2010 RAA, 11,137,Wu, Y. W.; Xu, Y.; Yang, J.

(5)“Herschel/HIFI Observations of a New Interstellar Water Maser: The 532 – 441 Transition at 620.701 GHz”, 2013 ApJ, 769, 48，Neufeld, D. A.; Wu, Y. W.,  Kraus, A.; Menten, K. M.; Tolls, V.; Melnick, G. J.; Nagy, Z.