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This article has an erratum: [https://doi.org/10.1051/0004-6361/202555385e]


Fig. B.1.

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Best-fit high-redshift fundamental planes of metallicity (HFPZ) at z = 6, 8, 12 for the evolving IMF (left) and Salpeter IMF (right) models. Coloured lines show the HFPZ at fixed SFR values, while the tiles depict the median SFR values in the respective stellar mass – metallicity bin according with their colours encoding the SFR value according to the colour bar on the right side of each panel.

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