Metallicity Gradients Across Cosmic Time
Spatially resolved gas-phase metallicity from grism spectroscopy, tracing how galaxies assemble from the local Universe to z ≈ 9.
Key papers: Li et al. 2025, ApJS
PhD Candidate in Astrophysics
Cosmic Dawn Center (DAWN) · Niels Bohr Institute · University of Copenhagen
I am a PhD candidate at the Cosmic Dawn Center (DAWN), Niels Bohr Institute, University of Copenhagen, working with Lise Christensen and Koki Kakiichi. I study the chemical enrichment of galaxies across cosmic time, from metallicity gradients at cosmic noon to metal-poor galaxies and first-star signatures near the end of reionization.
At DAWN, I work on the data reduction of JWST NIRCam and NIRISS wide-field slitless spectroscopy, and study the chemical enrichemnt of high redshift galaxies and cosmic reionization. I received my M.Sc. in Astronomy from Tsinghua University, advised by Zheng Cai, and my B.Sc. with honors in Aerospace Engineering from Sichuan University.
Spatially resolved gas-phase metallicity from grism spectroscopy, tracing how galaxies assemble from the local Universe to z ≈ 9.
Key papers: Li et al. 2025, ApJS
JWST ASPIRE/EIGER spectroscopy combined with chemical evolution models to study metal enrichment, environmental effects, and possible first-star (Pop III) imprints at z ≈ 5–7.
Key papers: Li et al. 2025, A&A; Li et al. 2026, arXiv
Data reduction and analysis of JWST NIRCam/NIRISS WFSS for the COSMOS-3D survey, including spatially resolved kinematics of a lensed z = 8.34 disk candidate.
Key papers: Li et al. 2023, arXiv
How protocluster environments shape galaxy chemistry at cosmic noon, and mapping the intergalactic medium with Lyα forest tomography.
Key papers: Li et al. 2022, ApJL; Wang et al. 2022, ApJ; Li et al. 2021, ApJ
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University of Copenhagen, Denmark
Tsinghua University, China
Sichuan University, China
For collaborations, conversations, or questions, feel free to reach out.