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Fig. 8.

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Relation between residuals and the redshifts of BH seeding (ZBH,  seed, left panel), galaxy transition (ZG,  tran, middle panel), and galaxy formation (ZG,  form, right panel). Galaxies with stellar mass ranges 10.0 < log(M*/M) < 10.5, 10.5 < log(M*/M) < 11, and 11.0 < log(M*/M) < 13 are shown as navy, cyan, and yellow lines, respectively, with errors estimated from the 16th to 84th percentile ranges. Correlation coefficients for each stellar mass bin are shown in each panel in the corresponding colours.

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