恒星光谱分析、太阳系外行星
刘凡,男,1986年出生,云南昆明人,中国科学院国家天文台项目研究员。2016年获得澳大利亚国立大学博士学位。2016年至2019年,2019年至2022年分别在瑞典隆德大学和澳大利亚斯威本科技大学从事博士后研究,2022年至2025年在澳大利亚莫纳什大学担任ASTRO3D研究员。于2025年通过人才引进计划入职中科院国家天文台工作至今。2024年获得国家自然科学基金优秀青年基金(海外)项目资助。主要从事恒星光谱分析、太阳系外行星方面的研究。研究成果发表于国际知名期刊,包括Nature, Science等,总计40余篇。承担国家自然科学基金项目1项。
1. F. Liu, D. Yong, Y.-S. Ting, et al. 'At least one in a dozen stars shows evidence of planetary ingestion', 2024, Nature, 627, 501
2. D. Yong, F. Liu, Y.-S. Ting, et al. 'C3PO: Towards a complete census of co-moving pairs of stars. I. High precision stellar parameters for 250 stars', 2023, MNRAS, 526, 2181
3. F. Liu, M.T. Murphy, C. Lehmann, et al. 'Survey for Distant Solar Twins (SDST) -- II. Design, observations and data', 2022, MNRAS, 517, 5569
4. M.T. Murphy, D.A. Berke, F. Liu, C. Flynn, C. Lehmann, V.A. Dzuba, V.V. Flambaum. 'A limit on variations in the fine-structure constant from spectra of nearby Sun-like stars', 2022, Science, 378, 634
5. F. Liu, B. Bitsch, M. Asplund, et al. 'Detailed elemental abundances of binary stars: Searching for signatures of planet formation and atomic diffusion', 2021, MNRAS, 508, 1227
6. F. Liu, D. Yong, M. Asplund, et al. 'Detailed chemical compositions of planet hosting stars: I. Exploration of possible planet signatures', 2020, MNRAS, 495, 3961
7. F. Liu, M. Asplund, D. Yong, et al. 'Chemical (in)homogeneity and atomic diffusion in the open cluster M67', 2019, A&A, 627, A117
8. F. Liu, D. Yong, M. Asplund, et al. 'Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation', 2018, A&A, 614, A138
9. F. Liu, M. Asplund, D. Yong, et al. 'The chemical compositions of solar twins in the open cluster M67', 2016, MNRAS, 463, 696
10. F. Liu, D. Yong, M. Asplund, et al. ‘The Hyades open cluster is chemically inhomogeneous’, 2016, MNRAS, 457, 3934
11. F. Liu, D. Yong, M. Asplund, et al. ‘The detailed chemical composition of the terrestrial planet host Kepler-10’, 2016, MNRAS, 456, 2636
12. F. Liu, M. Asplund, I. Ramirez, et al. ‘A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation’, 2014, MNRAS, 442, L51