Notes. Regions of origin (at z_p) of galaxies identified as MS at z_i (left part of the table) and passive galaxies at z_i (right part) from Figs. 17 and 18. The table presents the percentage of galaxies coming from each region of the M_⋆ − SFR plane–SB, star forming (SF), GV, and passive–alongside their associated uncertainties. Uncertainties were computed as the quadrature sum of bootstrap errors and systematic uncertainties due to deviations of the MS definition (±0.2 dex). Bootstrap errors were derived from 100 repetitions, where 80% of the total data set was sampled at each iteration, with the observed SFR, M_⋆, and migration vector randomly computed from a normal distribution with central values and standard deviations based on the CIGALE Bayesian-like analysis. Systematic uncertainties account for reclassification due to MS adopted and the typical bias with respect to the observed distribution (see Sect. 6.1), including the definition of progenitor populations on the reconstructed M_⋆ − SFR plane. dT reports the cosmic time elapsed between z_p and z_i.