Fig. 4.
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Best-fit double Schechter function parameters of the GSMFs shown in Fig. 3, using the same colour-coding. The x-axes distinguish between all, grouped, and ungrouped galaxies; within each sample, the three ticks correspond to the total (T), star-forming (SF), and passive (P) subsamples. Corresponding corner plots illustrating the correlations among fitted parameters are provided in Figs. A.1–A.3.
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