办公室:
海韵物理楼 521
个人简历:
2010.09 - 2014.06:厦门大学,物理学,学士
2014.09 - 2020.06:北京大学,天体物理,博士
2021.06 - 2023.02:德国马斯克普朗克射电天文学研究所,Humboldt Fellow 博士后
2023.03 - 2025.12:日本东京大学宇宙数学与物理研究所,KIPMU Fellow 博士后
2026.01 - 至今:厦门大学物理科学与技术学院 天文学系 副教授
研究领域:
星系的形成与演化
恒星形成
荣誉:
2020年8月获得“北京大学优秀博士学位论文”
2021年7月入选“洪堡学者”
2025年5月入选“东京大学青年研究员全球活动支持计划”
2025年入选“南强青年拔尖人才支持计划b类”
主要文章:
[15] Yu, S.-Y.*, et al. 2026, "Through Thick and Thin: The Cosmic Evolution of Disk Scale Height", ApJS, 283, 35
[14] Li, S., Yu, S.-Y.*, Ho, L.~C., et al. 2025, “Linking Electron Density with Elevated Star Formation Activity from z = 0 to z = 10”, ApJL, 993, 2, L51
[13] Yu, S.-Y.*, Xu, D.*, Kalita, B.~S., et al. 2025, “Color profiles of disk galaxies at z = 1–3 observed with JWST: Implications for outer-disk formation histories”, A&A, 693, L9
[12] Liang, X., Yu, S.-Y.*, Fang, T., Ho, C. L. 2023, “The robustness in identifying and quantifying high-redshift bars using JWST observations”, A&A, 688, A158
[11] Xu, D. & Yu, S.-Y.*, 2024, “JWST reveals a high fraction of disk breaks at 1 < z < 3”, A&A, 682, L17
[10] Yu, S.-Y.*; Cheng, Cheng; Pan, Yue; Sun, Fengwu; Li, Yang A. 2023, “Redshifting galaxies from DESI to JWST CEERS: Correction of biases and uncertainties in quantifying morphology”, A&A, 676, A74
[9] Yu, S.-Y.*, Kalinova, V., Colombo, D. et al. 2022, “The EDGE-CALIFA survey: The role of spiral arms and bars in driving central molecular gas concentrations”, A&A, 666, A175
[8] Yu, S.-Y.*, Xu, D., Ho, L. C., et al. 2022, “Strong spiral arms drive secular growth of pseudo bulges in disk galaxies”, A&A, 661, A98
[7] Yu, S.-Y.*, Ho, L. C., & Wang, J. 2021, “Spiral structure boosts star formation in disk galaxies”, ApJ, 917, 88
[6] Chen, E., Yu, S.-Y.*, & Ho, L. C. 2021, “Global spiral density wave modes in protoplanetary disk: Morphology of spiral arms”, ApJ, 906, 19
[5] Yu, S.-Y.* & Ho, L. C. 2020, “The statistical properties of spiral arms in nearby disk galaxies”, ApJ, 900, 150
[4] Yu, S.-Y.*, Ho, L. C., & Zhu, Z. 2019, “A tight relation between spiral arm pitch angle and protoplanetary disk mass”, ApJ, 877, 100
[3] Yu, S.-Y.* & Ho, L. C. 2019, “On the connection between spiral arm pitch angle and galaxy properties”, ApJ, 871, 194
[2] Yu, S.-Y.* & Ho, L. C. 2018, “Dependence of the spiral arms pitch angle on wavelength as a test of the density wave theory”, ApJ, 869, 29
[1] Yu, S.-Y.*, Ho, L. C., Barth, A. J., et al. 2018, “The Carnegie-Irvine galaxy survey. VI. Quantifying spiral structure”, ApJ, 862, 13
联系:
syu_at_xmu.edu.cn