Notes. For each object, we consider all Bagpipes runs performed over the full redshift prior range (0 ≤ z ≤ 25) and for all combinations of star-formation histories and dust attenuation laws explored. Given the typically bimodal shape of the resulting P(z) distributions, we identify the best-fit solutions at z ≤ 8 (“low”) and z > 8 (“high”) as those yielding the lowest χ² value within each redshift regime. The reported best-fit parameters (redshift z, stellar mass log M/M_⊙, and dust attenuation A_V) are those corresponding to these two solutions, while their uncertainties are derived as the 16th–84th percentile range around the best-fit values of each physical quantities. The integrated probability ∫P(z > 8),dz is instead computed over the full prior range (0 ≤ z ≤ 25) and considering the combination of SFH and dust law that minimizes χ² at z > 8. The full list of physical parameters is reported in Table D.1.