Results of the mock analysis on the SED modeling using the non-parametric SFH model. The input parameters used to build the mock catalog are shown on the x-axis, and the results from fitting the mock catalogs are shown on the y-axis. From left to right, the upper panels present the instantaneous SFR (here defined as the SFH in the first bin of 10 Myr), and the stellar mass M_⋆. The Φ_Δt values are presented as defined on Eq. (1) and computed over the last 300 to 1000 Myr, on the uppermost right panel and over the second-row panels. The third row and the left panel of the fourth row count for r_Δt (i.e., the norm of the migration vector) computed over the same timescales as Φ_Δt. The two rightmost panels on the fourth row and bottom panels present the mass formation times (noted Ti%[Myr] and defined as the time taken to form the {i} percentage of a galaxy’s total stellar mass) for the 90 to the 40%. The solid black lines indicate the one-to-one relation. The bias and precision estimated for the parameters are indicated in each panel.