Difference in estimated physical properties of galaxies from the final sample using different SFH models within the MIRI run as a function of redshift. From left to right: DelayedBQ-non-parametric, non-parametric-regulator, and regulator-delayedBQ. From top to bottom: Distribution of difference for: A_V in mag, age in Myr, SFR in M_⊙/yr, and the M_★ in M_⊙. The dashed blue line presents the median of distribution. The hatched region shows the 90th percentiles of the distributions (P₉₀) above and below the median value.