Example BAGPIPES fit to the photometry in a single Voronoi bin, plotted against the rest-frame wavelengths. The blue points indicate the measured flux at the pivot point of each filter, with their uncertainty (including the additional systematic component; see Appendix C). The shaded orange region indicates the 16th–84th percentile of the model spectrum, and the orange points the corresponding predicted fluxes in each filter. In the inset, we show the derived SFH of this region as a function of both redshift and the age of the Universe, with the shaded region denoting the 16th–84th percentile of the posterior PDF in each age bin.