Updated Metallicity Diagnostics for Precision Oxygen Abundance Measurements in High-redshift Galaxies with JWST
Shihong Liu, Yu Rong, Tie Li, Yao Yao, Cheng Jia, Enci Wang, Hongxin Zhang, Zhicheng He, Huiyuan Wang, Xu Kong

TL;DR
This paper develops new metallicity diagnostics for high-redshift galaxies using JWST data, incorporating ionization and nitrogen effects to improve oxygen abundance measurements and understand cosmic chemical evolution.
Contribution
It introduces updated indicators that explicitly include ionization and nitrogen proxies, significantly improving the accuracy of metallicity estimates in high-redshift galaxies.
Findings
Updated indicators tighten the correlation with true oxygen abundance.
Calibration achieves R^2 > 0.5, up to 0.7 at z>2.
Reveals redshift evolution in metallicity diagnostics near cosmic noon.
Abstract
Recent work has demonstrated that widely used strong-line oxygen abundance indicators, such as O3N2, , and , suffer from large uncertainties when applied to high-redshift galaxies. We show that this loss of precision primarily arises because, at fixed \Oabund, galaxies span a wide dynamic range in ionization parameter and nitrogen enrichment. Here we develop updated indicators that explicitly incorporate both effects via the proxies O32 and N2O2. We define , , and , and calibrate \Oabund~as low-order polynomials in each composite indicator. Applied to a JWST sample with -method abundances, the updated indicators substantially tighten the correlations with \Oabund,…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
