现任中国科学院紫金山天文台副研究员。2016年意大利国际高等研究院博士毕业，曾先后在意大利博洛尼亚大学、北京大学科维理天文与天体物理研究所从事博士后研究工作。符晓婷深度参与了包括 Gaia, Gaia-ESO survey 在内的多项大型国际巡天合作项目，并作为科学组长领导11米望远镜莫纳克亚光谱探索者(MaunaKea Spectroscopic Explorer)银河系科学小组的工作，是我国空间站巡天望远镜恒星模拟星表的主要负责人之一。截止至 2025 年底 h-index 21。
其主要研究方向为恒星物理，包括从理论和观测两个方面研究恒星结构与演化、恒星元素丰度、银河系结构及化学演化。是国际著名恒星演化模型 PARSEC 的核心成员之一。
论文列表见：https://ui.adsabs.harvard.edu/public-libraries/AXP--HTKRDi77jN1awFnWw
[1]Fu, X., Bressan, A., Molaro, P., and Marigo, P., “Lithium evolution in metal-poor stars: from pre-main sequence to the Spite plateau”, Monthly Notices of the Royal Astronomical Society, vol. 452, no. 3, OUP, pp. 3256–3265, 2015. doi:10.1093/mnras/stv1384.
[2]Fu, X., Bressan, A., Marigo, P., et al., “New PARSEC data base of α-enhanced stellar evolutionary tracks and isochrones - I. Calibration with 47 Tuc (NGC 104) and the improvement on RGB bump”, Monthly Notices of the Royal Astronomical Society, vol. 476, no. 1, OUP, pp. 496–511, 2018. doi:10.1093/mnras/sty235.
[3]Fu, X., Romano, D., Bragaglia, A., et al., “The Gaia-ESO Survey: Lithium enrichment histories of the Galactic thick and thin disc”, Astronomy and Astrophysics, vol. 610, Art. no. A38, EDP, 2018. doi:10.1051/0004-6361/201731677.
[4]Fu, X., Bragaglia, A., Liu, C., et al., “LAMOST meets Gaia: The Galactic open clusters”, Astronomy and Astrophysics, vol. 668, Art. no. A4, EDP, 2022. doi:10.1051/0004-6361/202243590.
[5]Bragaglia, A., Fu, X., Mucciarelli, A., et al., “The chemical composition of the oldest nearby open cluster Ruprecht 147”, <i>Astronomy and Astrophysics</i>, vol. 619, Art. no. A176, EDP, 2018. doi:10.1051/0004-6361/201833888.
[6]Kirby, E. N., Fu, X., Guhathakurta, P., and Deng, L., “Discovery of Super-Li-rich Red Giants in Dwarf Spheroidal Galaxies”, The Astrophysical Journal, vol. 752, no. 1, Art. no. L16, IOP, 2012. doi:10.1088/2041-8205/752/1/L16.
[7]Chen, Y., Fu, X., Liu, C., et al., “The first comprehensive Milky Way stellar mock catalogue for the Chinese Space Station Telescope Survey Camera”, Science China Physics, Mechanics, and Astronomy, vol. 66, no. 11, Art. no. 119511, Springer, 2023. doi:10.1007/s11433-023-2181-x.
[8]Jian, M., Fu, X., Matsunaga, N., et al., “Stellar Population Astrophysics (SPA) with the TNG. Measurement of the He I 10 830 Å line in the open cluster Stock 2”, Astronomy and Astrophysics, vol. 687, Art. no. A189, EDP, 2024. doi:10.1051/0004-6361/202449476.
[9]Jian, M., Fu, X., D’Orazi, V., et al., “Stellar population astrophysics (SPA) with the TNG. The phosphorus abundance on the young side of Milky Way”, Monthly Notices of the Royal Astronomical Society, vol. 545, no. 2, Art. no. staf1797, OUP, 2026. doi:10.1093/mnras/staf1797.
[10]Xu, M., Fu, X., Chen, Y., et al., “Nearby open clusters with tidal features: Golden sample selection and 3D structure”, Astronomy and Astrophysics, vol. 698, Art. no. A156, EDP, 2025. doi:10.1051/0004-6361/202554212.
[11]Chen, Y., Girardi, L., Fu, X., et al., “YBC: a stellar bolometric corrections database with variable extinction coefficients. Application to PARSEC isochrones”, Astronomy and Astrophysics, vol. 632, Art. no. A105, EDP, 2019. doi:10.1051/0004-6361/201936612.
[12]Wang, F., Fang, M., Fu, X., et al., “Empirical Color Correction to MIST and PARSEC Isochrones on Gaia BR − RP and G − RP with Benchmark Open Clusters”, The Astrophysical Journal, vol. 979, no. 1, Art. no. 92, IOP, 2025. doi:10.3847/1538-4357/ad960a.
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