(a) Spatially resolved map of the stellar mass surface density for 29 959, with all external objects masked out. The discontinuity in the tail is due to the very low S/N in this area. (b) Specific star formation rate density. We note that the lower limit of the colour map differs from Fig. 5, in order to preserve as much detail as possible. (c) Mass-weighted age, Age_MW, expressed on a linear scale in units of Gyr.