沈璐

助理教授/Assistant Professor

2019年美国加州大学戴维斯分校博士/Ph.D.(2019), University of California, Davis

电话：+86-13810312846

Email: lushen@fudan.edu.cn

主要经历:

2010.9-2014.7 厦门大学物理学学士

2014.9-2019.9 美国加州大学戴维斯分校物理学博士

2019.9-2021.7 中国科学技术大学天文学博士后

2021.7-2022.8 中国科学技术大学天文学特任副研究员

2022.9-2026.4 美国德州农工大学物理与天文学博士后

2026.4-至今 复旦大学物理系助理教授

教学与研究领域:

科研：观测天文，星系的形成与演化，高红移星系，恒星形成，星系团与原初星系团，活动星系核反馈。

Lu Shen

Associate Professor

Ph.D(2019), University of California, Davis

Research Interest:

Observational astronomy, Galaxy formation and evolution, High redshift galaxies, Star formation, Galaxy cluster and protocluster, AGN feedback.

Selected Publications:

1) Lu Shen, et al “NGDEEP: The Star Formation and Ionization Properties of Galaxies at 1.7 < z < 3.4”, ApJ Letter, 980, 45 (2025).

2) Lu Shen, et al “NGDEEP Epoch 1: Spatially Resolved Hα Observations of Disk and Bulge Growth in Star-forming Galaxies at z ∼ 0.6─2.2 from JWST NIRISS Slitless Spectroscopy”, ApJ Letter, 963, 49 (2024).

3) Lu Shen, et al “Discovery of spectacular quasar-driven superbubbles in red quasars” Sci. Adv. eadg8287 (2023).

4) Lu Shen, et al “CEERS: Spatially Resolved UV and Mid-infrared Star Formation in Galaxies at 0.2 < z < 2.5: The Picture from the Hubble and James Webb Space Telescopes”, ApJ, 950, 7 (2023).

5) Lu Shen, et al “The ALPINE-ALMA [C II] Survey: The Infrared-Radio Correlation and Active Galactic Nucleus Fraction of Star-forming Galaxies at z ~ 4.4-5.9”, ApJ, 935, 177 (2022). 

6) Lu Shen, et al “Implications of the Environments of Radio-detected Active Galactic Nuclei in a Complex Protostructure at z ∼ 3.3”, ApJ, 912, 60 (2021).

7) Lu Shen, et al “The properties of radio and mid-infrared detected galaxies and the effect of environment on the co-evolution of AGN and star formation at z ∼ 1”, MNRAS, 494, 5374 (2020).