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Fig. 4.

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C-A diagram based on MIRI F560W morphology, separating galaxies at 3<z<3.75 with log(M/M)<9.5 (low-z/low-M; blue dots and shaded region), galaxies at 3<z<3.75 with log(M/M)>9.5 (low-z/high-M; green stars and shaded region), and galaxies at 3.75<z<5 (high-z/all-M; red squares and shaded region). Mergers and late-type galaxies are separated according to Conselice (2003). The boundaries between late-type galaxies and intermediate galaxies are defined as in Bershady et al. (2000).

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