Galaxy quenching at the high redshift frontier: A fundamental test of cosmological models in the early universe with JWST-CEERS
Asa F. L. Bluck, Christopher J. Conselice, Katherine Ormerod, Joanna, M. Piotrowska, Nathan Adams, Duncan Austin, Joseph Caruana, K. J. Duncan,, Leonardo Ferreira, Paul Goubert, Thomas Harvey, James Trussler, Roberto, Maiolino

TL;DR
This study uses JWST-CEERS data to analyze galaxy quenching in the early universe, finding that stellar potential is the best predictor of quiescence, supporting models linking black hole growth to galaxy quenching.
Contribution
It demonstrates that stellar potential predicts galaxy quenching across cosmic time, validating simulation predictions about black hole influence in early galaxy evolution.
Findings
Stellar potential outperforms other parameters in predicting quenching.
Black hole mass proxies are consistent with stellar potential in observations.
A stable quenching mechanism linked to gravitational potential operates from early to late universe.
Abstract
We present an analysis of the quenching of star formation in massive galaxies () within the first 0.5 - 3 Gyr of the Universe's history utilizing JWST-CEERS data. We utilize a combination of advanced statistical methods to accurately constrain the intrinsic dependence of quenching in a multi-dimensional and inter-correlated parameter space. Specifically, we apply Random Forest (RF) classification, area statistics, and a partial correlation analysis to the JWST-CEERS data. First, we identify the key testable predictions from two state-of-the-art cosmological simulations (IllustrisTNG & EAGLE). Both simulations predict that quenching should be regulated by supermassive black hole mass in the early Universe. Furthermore, both simulations identify the stellar potential () as the optimal proxy for black hole mass in photometric data. In photometric…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Gamma-ray bursts and supernovae
