Fig. 2.
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Comparison between the gas-phase metallicity of CEERS-14821 (coloured stars, slightly shifted horizontally for clarity) with the MZR (solid blue line) and other galaxies (green circles) at z = 4 − 6 (Curti et al. 2024). Vertical grey shadows show the stellar mass of CEERS-14821 derived based on the two different dust extinction laws.
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