Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations

[2605.03008] Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations Skip to main content Search Submit Donate Log in Search arXiv Press Enter to search · Advanced search Astrophysics > Astrophysics of Galaxies arXiv:2605.03008 (astro-ph) [Submitted on 4 May 2026 ( v1 ), last revised 15 Aug 2026 (this version, v2)] Title: Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations Authors: Aleyna Döven , Mohammadreza Ayromlou , Cristiano Porciani View a PDF of the paper titled Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations, by Aleyna D\"oven and 2 other authors View PDF HTML (experimental) Abstract: Recent observations of the high-redshift Universe, particularly with JWST, have revealed a population of quenched galaxies that challenges current galaxy formation models, which systematically underpredict their abundance. This discrepancy has been extensively studied for massive systems, motivating revisions to internal quenching mechanisms such as AGN feedback. However, the origin of quenching in lower-mass galaxies at high-z has received far less attention, largely due to previous observational limitations. JWST has now identified low-mass quenched galaxies (${M_{\star}}<10^{10}{\rm M_{\odot}}$). Given this emerging observational evidence, we investigate the viability of environmental quenching as the primary mechanism suppressing star formation in low-mass galaxies at $z>3$. We analyze several simulations, including L-GALAXIES, IllustrisTNG, SIMBA, and TNG-Cluster, jointly comprising more than half a million galaxies at z=5. Across all simulations, quenched systems are overwhelmingly satellites, despite representing less than 10\% of the total galaxy population. Satellite quenching increases with host halo mass and decreases with both stellar mass and halocentric distance, showing strong correlations with enhanced ram-pressure exposure and gas depletion. The simulations, particularly L-GALAXIES, produce low-mass quenched galaxies broadly consistent with those observed by JWST. Our results suggest that the recently discovered high-redshift quenched low-mass galaxies are possibly environmentally quenched systems residing in the vicinity of massive halos. According to the simulations, these galaxies are often only temporarily quenched: nearly 90\% of them merge within a few hundred megayears, and a small fraction rejuvenate and resume star formation. Extended samples from future observations will enable robust tests of the environmental origin of galaxy quenching in the early Universe. Comments: 12 pages, 11 figures, plus Appendix (8 pages, 8 figures). Accepted for publication in A&A Subjects: Astrophysics of Galaxies (astro-ph.GA) Cite as: arXiv:2605.03008 [astro-ph.GA] (or arXiv:2605.03008v2 [astro-ph.GA] for this version) https://doi.org/10.48550/arXiv.2605.03008 Focus to learn more arXiv-issued DOI via DataCite Related DOI : https://doi.org/10.1051/0004-6361/202660728 Focus to learn more DOI(s) linking to related resources Submission history From: Aleyna Döven [ view email ] [v1] Mon, 4 May 2026 18:00:06 UTC (4,259 KB) [v2] Sat, 15 Aug 2026 01:29:57 UTC (4,233 KB) Full-text links: Access Paper: View a PDF of the paper titled Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations, by Aleyna D\"oven and 2 other authors View PDF HTML (experimental) TeX Source view license Current browse context: astro-ph.GA < prev | next > new | recent | 2026-05 Change to browse by: astro-ph References & Citations NASA ADS Google Scholar Semantic Scholar export BibTeX citation Loading... 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