章博
研究方向:
- 恒星光谱学:利用恒星光谱确定恒星大气参数与元素丰度
- 统计和机器学习应用:利用统计与机器学习方法解决天文数据处理问题
- 光谱数据处理:光谱原始数据自动化处理和定标
邮箱:bozhang@bnu.edu.cn
Github主页:https://github.com/hypergravity
教育背景:
2013.09-2019.12 中国科学院大学/国家天文台 天体物理 理学博士
2009.09-2013.06 浙江工业大学 应用物理学 理学学士
工作经历:
2020.01-2022.01 北京师范大学 博士后/LAMOST特聘青年研究员
已发表的工作:
- Yang, F., Long, R. J., Shan, S.-S., Zhang, B., Guo, R., Bai, Y., Bai, Z., Cui, K.-M., Wang, S., & Liu, J.-F., A Catalog of Short Period Spectroscopic and Eclipsing Binaries Identified from the LAMOST and PTF Surveys, The Astrophysical Journal Supplement Series, 2020, 249, 31.
- Tian, H., Liu, C., Wang, Y., Xu, Y., Yang, C., Zhang, B., & Xue, X.-X., Differential Rotation of the Halo Traced by K-giant Stars, The Astrophysical Journal, 2020, 899, 110.
- Zhang, B., Liu, C., Li, C.-Q., Deng, L.-C., Yan, T.-S., & Shi, J.-R., Exploring the spectral information content in the LAMOST medium-resolution survey (MRS), Research in Astronomy and Astrophysics, 2020, 20, 051.
- Zhang, B., Liu, C., & Deng, L.-C., Deriving the Stellar Labels of LAMOST Spectra with the Stellar LAbel Machine (SLAM), The Astrophysical Journal Supplement Series, 2020, 246, 9.
- Yang, C., Xue, X.-X., Li, J., Liu, C., Zhang, B., Rix, H.-W., Zhang, L., Zhao, G., Tian, H., Zhong, J., Xing, Q., Wu, Y., Li, C., Carlin, J. L., & Chang, J., Tracing Kinematic and Chemical Properties of Sagittarius Stream by K-Giants, M-Giants, and BHB stars, The Astrophysical Journal, 2019, 886, 154.
- Wang, K., Luo, C., Zhang, X., Zhang, B., Deng, L., & Luo, Z., V1224 Cas: An EL CVn-type Eclipsing Binary Consisting of a Helium White Dwarf Precursor and a Delta Scuti Pulsator, The Astronomical Journal, 2018, 156, 187.
- Zhang, B., Chen, X.-Y., Liu, C., Chen, L., Deng, L.-C., Hou, J.-L., Shao, Z.-Y., Yang, F., Wu, Y., Yang, M., Zhang, Y., Hou, Y.-H., & Wang, Y.-F., Candidate members of star clusters from LAMOST DR2, Research in Astronomy and Astrophysics, 2015, 15, 1197.
- Liu, C., Cui, W.-Y., Zhang, B., Wan, J.-C., Deng, L.-C., Hou, Y.-H., Wang, Y.-F., Yang, M., & Zhang, Y., Spectral classification of stars based on LAMOST spectra, Research in Astronomy and Astrophysics, 2015, 15, 1137.