Similar to Figure 3 but focused on the difference between the subclass pairs of early- and late-quenched galaxies as well as quenched and main-sequence rejuvenators. Here, the colors refer to the subclass types instead of quenching incidents. The large points show the cherry-picked representative galaxies from Figure 4, again set to the bottom of the panels as half-circles for visibility in case of low SFR values. By construction, the difference between early- and late-quenched is most pronounced at z = 1. At z ≈ 0, the non-zero distributions are barely noticeable. Analogously, the difference between the two rejuvenator subclasses is the sharpest at z ≈ 0. Both subclasses undergo rejuvenation cycles at different times, but the relation to the SFMS determines the classification.