Fig. 11.
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Stellar mass-stellar metallicity relation over z ≈ 0.1 (Zahid et al. 2017) to z ≈ 3 − 5 (Cullen et al. 2019). The green data points show measurements by Cullen et al. (2019) shifted down by 0.1 dex to account for differences in the stellar population models. The grey shaded region shows the average gas-phase metallicity measured in DLAs at z ≈ 4.5 (Rafelski et al. 2012).
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