Title:

associate professor

pEmail:

xmkong@sdu.edu.cn

Research Interests:

Data mining, Stellar abundance, spectral analysis

Archievements:

PUBLICATIONS:

[1]   Kong, X.   M.;Zhao, G.; Zhao, J. K.; Shi, J. R.; Kumar, Y. Bharat; Wang, L.; Zhang, J.   B.; Wang, Y.; Zhou, Y. T. Chemical abundances of primary stars in the   Sirius-like binary systems, Monthly Notices of the Royal Astronomical   Society, 2018, 476(1): 724-740

[2] Kong, X. M.; Y. Bharat   Kumar; G. Zhao; J. K. Zhao; X.S. Fang; J. R. Shi; L. Wang; J. B. Zhang; H. L.   Yan, Three new barium dwarfs with white dwarf companions: BD+68°1027, RE   J0702+129 and BD+80°670, Monthly Notices of the Royal Astronomical Society, 2018,   474(2) : 2129-2141

[3] Zhao, J. K.; Zhao, G.;   Aoki, W.; Ishigaki, M. N.; Suda, T.; Matsuno, T.; Shi, J. R.; Xing, Q. F.;   Chen, Y. Q.; Oswalt, Terry D.; Kong, X. M.; Liang, X. L.; Tracing the   Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo   Stream LAMOST-N1, The Astrophysical Journal, 2018, 868(2):105-123
  [4] Liang, X. L.; Zhao, J. K.; Zhao, G.; Aoki, W.; Ishigaki, M. N.; Matsuno,   T.; Chen, Y. Q.; Kong, X. M.; Shi, J. R.; Xing, Q. F.,
  Tracing the Origin of Moving Groups. I. The γ Leo Moving Group with   High-resolution Spectra from the Subaru Telescope,
  The Astrophysical Journal,2018,863(1):4-12

[5]   Yongjian Zhao*, Xiaoming Kong, Haining   Jiang, Meixia Qu. Constrained independent component analysis techniques [A].   In: Proceedings of the IEEE Workshop on Electronics, Computer and   Applications [C], Ottawa, Canada, May 8-9, 2014, pp. 419-422.

[6]   Yongjian Zhao*, Xiaoming Kong, Haining   Jiang, Meixia Qu. Improved techniques for independent component analysis [A].   In: Proceedings of the IEEE Workshop on Electronics, Computer and   Applications [C], Ottawa, Canada, May 8-9, 2014, pp. 415-418.

ONGOING PROJECT:

[1]   National Natural Science Foundation of China.   Study of barium stars in Kepler field based on the medium - resolution   spectra from the LAMOST survey. 2019.01-2021.12. (Grant No. 11803016)

[2]   National Natural Science Foundation of China.   Solution of some difficulties in stellar parameter measurement based on   multivariate associated characteristics. 2020.01-2023.12(Grant No. U1931209)