publications
The PDF version (with an additional brief explanation of the papers) is available here.
You can also find the latest publication list on NASA/ADS.
2026
- Unveiling the Ionized and Neutral ISM at z > 10: The Origin of [O III] /[C II] Ratios from a Subparsec Resolution Radiative Transfer Simulation\apj, Feb 2026
-
- Clump-Scale Dust Attenuation in Epoch of Reionization Galaxies: Spatially Resolved Properties from FirstLight SimulationsarXiv e-prints, Feb 2026
- A UV-Luminous Galaxy at z=11 with Surprisingly Weak Star Formation ActivityarXiv e-prints, Jan 2026
2025
- A merger-driven scenario for clumpy galaxy formation in the epoch of reionization: Physical properties of clumps in the FirstLight simulationIn IAU Symposium, Dec 2025
- Rapid Carbonaceous Dust Evolution in EoR Galaxies: Synergies Among JWST, PRIMA, and ALMAIn PRIMA General Observer Science Book Volume 2, Dec 2025
- Far-infrared line properties of Green Pea galaxies, the best local analogues of galaxies in the epoch of reionization eraIn PRIMA General Observer Science Book Volume 2, Dec 2025
-
- Comprehensive JWST+ALMA Study on the Extended Ly\ensuremathα Emitters, Himiko, and CR7 at z \ensuremath∼ 7: Blue Major Merger Systems in Stark Contrast to Submillimeter Galaxies\apj, Dec 2025
- RIOJA. Young starburst and ionized gas outflows in a z = 7.212 galaxy uncovered by JWST NIRCam and NIRSpec observations\mnras, Dec 2025
-
- RIOJA. Dusty outflows and density-complex ISM in the N-enhanced lensed galaxy RXCJ2248-ID at z=6.1arXiv e-prints, Nov 2025
-
- RIOJA. JWST and ALMA Unveil the Inhomogeneous and Complex Interstellar Medium Structure in a Star-forming Galaxy at z = 6.81\apjl, Oct 2025
- Early massive galaxy formation in the core of a galaxy protocluster 650 million years after the Big BangarXiv e-prints, Oct 2025
- ELPIS: Accelerated metal and dust enrichment in a proto-cluster core at z\approx8arXiv e-prints, Oct 2025
- JWST PRIMER: a lack of outshining in four normal z = 4 ‑ 6 galaxies from the ALMA-CRISTAL Survey\mnras, May 2025
-
- Detection of the [O I] 63 \textmum emission line from the z = 6.04 quasar J2054-0005\pasj, Feb 2025
- 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
2024
-
- 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