Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity
Elie Cueto, Anne Hutter
astro-ph.GA
Submitted: 2026-07-21
Comments: 19 pages, 7 figures. Submitted to MNRAS
Code: https://github.com/E-Cueto/SimpleGal
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Spatially Resolved Physical Properties of Young Star Clusters and Star-forming Clumps in the Brightest z>6 Galaxy, the Strongly Lensed Cosmic Spear at z=6.2
- JADES: Evolution of nitrogen abundances in star-forming galaxies from z 1.5-7
- Feedback-Free Star Formation in Clusters within a Galaxy Simulated at High Resolution in Cosmic Dawn
- JWST PRIMER: A new multi-field determination of the evolving galaxy UV luminosity function at redshifts $\mathbf{z \simeq 9-15}$
- The Thesan-Zoom project: bursty star formation is incompatible with prolonged dust survival
- A search for the first galaxies across $>0.6$ deg$^2$ of JWST imaging: new evidence for a rapid decline in star-formation activity at $z>12$
- VENUS: A Strongly Lensed Clumpy Galaxy at $z\sim11-12$ behind the Galaxy Cluster MACS J0257.1-2325
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