Beyond No No Tension: JWST z > 10 Galaxies Push Simulations to the Limit

JWST has identified some of the Universe’s earliest galaxies, repeatedly pushing the frontier to ever higher redshifts and stellar masses. The presence of such extreme galaxies at such early times, with large stellar populations and high star-formation rates, naturally results in a tension between observation and theory. This tension between numerical models and observations can be either due to our underlying cosmological models or due to a gap in our understanding of early Universe astrophysics. In a prelude to this letter, we showed how the Renaissance simulations, which focused on high redshift galaxy formation were able to reconstruct similar stellar masses to the earliest and highest mass galaxies that had been discovered by JWST at the time of its publication (McCaffrey et al.2023). Since then many more galaxies have been discovered by JWST, in particular the “Mirage-or-Miracle” (MoM) survey broke the record recently with the highest redshift galaxy MoM-z14, which has a spectroscopically confirmed redshift of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>z</mml:mi> <mml:mo>∼</mml:mo> <mml:mn>14.44</mml:mn> </mml:mrow> </mml:math> followed closely by GS-z14 with a spectroscopically confirmed redshift of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>z</mml:mi> <mml:mo>∼</mml:mo> <mml:mn>14.3</mml:mn> </mml:mrow> </mml:math> . We investigate in this letter whether these newly discovered galaxies are in conflict with the Renaissance simulations and thus whether they are causing tension with our established models of cosmology and/or high-redshift astrophysics. We discover that MoM-z14’s high mass at early redshift can be explained by the Renaissance simulation suite, whereas the extremely high stellar mass of GS-z14 remains an outlier when compared to previous measurements of high-redshift galaxies detected by JWST and our numerical models (even after accounting for cosmic variance).

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Publication Details

Journal
The Open Journal of Astrophysics
Published
2025-11-14
DOI
https://doi.org/10.33232/001c.147278
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
0.00
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article

Beyond No No Tension: JWST z > 10 Galaxies Push Simulations to the Limit

John A. Regan, John Wise, Joe McCaffrey, Samantha Hardin
The Open Journal of Astrophysics
Galaxies: Formation, Evolution, Phenomena
article

Beyond No No Tension: JWST z > 10 Galaxies Push Simulations to the Limit

John A. Regan, John Wise, Joe McCaffrey, Samantha Hardin
article en

Abstract

JWST has identified some of the Universe’s earliest galaxies, repeatedly pushing the frontier to ever higher redshifts and stellar masses. The presence of such extreme galaxies at such early times, with large stellar populations and high star-formation rates, naturally results in a tension between observation and theory. This tension between numerical models and observations can be either due to our underlying cosmological models or due to a gap in our understanding of early Universe astrophysics. In a prelude to this letter, we showed how the Renaissance simulations, which focused on high redshift galaxy formation were able to reconstruct similar stellar masses to the earliest and highest mass galaxies that had been discovered by JWST at the time of its publication (McCaffrey et al.2023). Since then many more galaxies have been discovered by JWST, in particular the “Mirage-or-Miracle” (MoM) survey broke the record recently with the highest redshift galaxy MoM-z14, which has a spectroscopically confirmed redshift of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>z</mml:mi> <mml:mo>∼</mml:mo> <mml:mn>14.44</mml:mn> </mml:mrow> </mml:math> followed closely by GS-z14 with a spectroscopically confirmed redshift of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>z</mml:mi> <mml:mo>∼</mml:mo> <mml:mn>14.3</mml:mn> </mml:mrow> </mml:math> . We investigate in this letter whether these newly discovered galaxies are in conflict with the Renaissance simulations and thus whether they are causing tension with our established models of cosmology and/or high-redshift astrophysics. We discover that MoM-z14’s high mass at early redshift can be explained by the Renaissance simulation suite, whereas the extremely high stellar mass of GS-z14 remains an outlier when compared to previous measurements of high-redshift galaxies detected by JWST and our numerical models (even after accounting for cosmic variance).

The Open Journal of AstrophysicsVol. 8
Georgia Institute of Technology (US), National University of Ireland, Maynooth (IE), ORCID (US)
Openalex Percentile: Top 76%
Galaxies: Formation, Evolution, Phenomena
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