Fractions of formation class members in stellar mass bins at z ≈ 0. Slight shifts of data points originate from taking the median stellar masses instead of bin centers. Early-quenched galaxies (dark red) peak at around M_* = 10¹¹, while late-quenched ones (dark blue) peak at slightly higher masses. Galaxies with rejuvenation cycles (dashed magenta line) in their formation histories are more prevalent on the lower- and higher-mass ends of the range between 10¹⁰ M_⊙ ≤ M_* ≤ 10¹² M_⊙. Quenched rejuvenators (lilac) tend more toward lower masses, while a rejuvenation sustained until z ≈ 0 (pink) is more often found at higher masses. Main-sequence (cyan) and caught types (blue) are generally rare with a faint preference for the high-mass end. Both subtypes are more prevalent on the lower- and higher- mass ends of the range between 10¹⁰ M_⊙ ≤ M_* ≤ 10¹² M_⊙.