publications
You can also find the latest publication list on NASA/ADS.
2025
- JWST PRIMER: a lack of outshining in four normal z = 4 ‑ 6 galaxies from the ALMA-CRISTAL Survey\mnras, May 2025
- Unveiling the Ionized and Neutral ISM at z > 10 : The Origin of [O III] /[C II] Ratios from a Sub-parsec Resolution Radiative Transfer SimulationarXiv e-prints, May 2025
- Comprehensive JWST+ALMA Study on the Extended Lyα Emitters, Himiko and CR7 at z∼7: Blue Major Merger Systems in Stark Contrast to Submillimeter GalaxiesarXiv e-prints, Apr 2025
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- JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z \ensuremath∼ 7–14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe\apj, Feb 2025
- Detection of the [O I] 63 \textmum emission line from the z = 6.04 quasar J2054-0005\pasj, Feb 2025
2024
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- A Merger-driven Scenario for Clumpy Galaxy Formation in the Epoch of Reionization: Physical Properties of Clumps in the FirstLight Simulation\apj, Nov 2024
- Redshift-dependent galaxy formation efficiency at z = 5 ‑ 13 in the FirstLight Simulations\aap, Sep 2024
- The Supersonic Project: Lighting Up the Faint End of the JWST UV Luminosity Function\apjl, Jan 2024
2023
- A photon burst clears the earliest dusty galaxies: modelling dust in high-redshift galaxies from ALMA to JWST\mnras, Dec 2023
- The Supersonic Project: Star Formation in Early Star Clusters without Dark Matter\apjl, Oct 2023
- Reionization and the ISM/Stellar Origins with JWST and ALMA (RIOJA): The Core of the Highest-redshift Galaxy Overdensity at z = 7.88 Confirmed by NIRSpec/JWST\apjl, Sep 2023
- Simulations of High-redshift [O III] Emitters: Chemical Evolution and Multiline Diagnostics\apj, Aug 2023
- Detections of [C II] 158 \ensuremathμm and [O III] 88 \ensuremathμm in a Local Lyman Continuum Emitter, Mrk 54, and Its Implications to High-redshift ALMA Studies\apj, May 2023
- The Supersonic Project: The Eccentricity and Rotational Support of SIGOs and DM GHOSts\apj, Mar 2023
- The Supersonic Project: The Early Evolutionary Path of Supersonically Induced Gas Objects\apj, Feb 2023
- The formation of Supersonically Induced Gas Objects (SIGOs) with H_2 coolingIn The Predictive Power of Computational Astrophysics as a Discover Tool, Jan 2023