What becomes of JWST/NIRCam-selected high-redshift massive galaxies?
Devontae C. Baxter, Alison L. Coil, Ethan O Nadler, Xuejian Shen, Mark Vogelsberger
astro-ph.GA
Submitted: 2026-07-09
Comments: Manuscript contains 18 pages and 9 figures. Submitted to ApJ. Comments are welcome
Code: https://github.com/bd-j/sedpy
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Quantifying biases in stellar masses of JWST high-z quasar host galaxies caused by quasar subtraction
- JWST Predictions for $z > 10$ Galaxies from the Renaissance Simulations -- I: Photometry and Sizes
- Stellar masses of optically dark galaxies: uncertainty introduced by the attenuation law and star-formation histories
- On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$
- Accelerated Emergence of Evolved Galaxies in Early Overdensities at $z\sim5.7$
- Resolving galaxy formation in the early Universe with BonFIRE and CampFIRE
- JWST observes the assembly of a massive galaxy at z~4
- Too many protoclusters? Reconciling the overabundance of cluster progenitors within the first billion years of the Universe
- A Census of the 200 Most Massive Galaxies Spectroscopically Observed with JWST at zspec about 3-15
- Explaining the "too massive" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation
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