Galaxy property maps. We include only the pixels with a S/N (averaged between F277W, F356W, and F444W) higher than 5. We use a τ-delayed prior for the SFHs. From left to right: RGB images (built using the method described in Lupton et al. (2004) with the filters specified above each image to enhance the different structures), and the inferred properties per pixel ${log}_{10}({\mathrm{\Sigma }}_{\star }/\left(M_{\odot }{\mathrm{kpc}}^{-2}\right))$, the mass-weighted age [Gyr], and A_V [mag]. In the lower-left corner of the first column, we show circles with diameters equal to the FWHM of the F444W PSF. Scale bars in the first column indicate angular (arcseconds) and physical (kiloparsecs) sizes.