Evolution of median relative accretion rates of each class across cosmic time. The underlying values were retrieved by calculating the ratio of accretion rates at 0.1 ⋅ R_vir and R_vir for each galaxy at each particle snapshot. Early-quenched galaxies exceed at accretion rates onto the center at high redshifts while abruptly decreasing after redshift z < 2. Main-sequence and late-quenched types have a similar evolution but with a clearly delayed peak. Rejuvenators do not peak but rather reach a plateau, while caught-types reach the same plateau after a strong delayed peak.