BAGPIPES fitting of the UV and optical SED. Top: Observed SED (coloured points) and best-fit model spectrum (orange). The lines at the bottom of the panel show the filter bandpasses of the imaging data used in the fit. The inset shows a zoom into the optical part of the SED. Bottom: Posterior probability distribution of the fitted and derived model parameters redshift z, mass-weighted age Age_MW, the time since the SFH began Age_exp, metallicity Z_exp, stellar mass M_*, and dust extinction A_V. The 16, 50, and 84 percentiles are shown with vertical dashed lines.