SFERA 2.0 results for region 1. Panels (a)-(b): recovered SFH and mass using PARSEC-COLIBRI (orange line) and MIST (blue line) isochrones. The shaded areas mark the 16–84 percentiles. Panels (c)-(d): data (black points) vs. model CMD luminosity functions for different luminosity intervals (indicated on the upper-right). Again, the PARSEC-COLIBRI solution is in orange, while the MIST in blue. Panels (e)-(g): observational CMD, SFERA 2.0 best fit model CMD and normalized residuals for each CMD cell ($data-model/\sqrt{\mathit{model}}$). The diagrams are color-coded according to the number of stars in each cell (see color-bar in the upper-right corner). The dark-shade masks the region of the CMD that is below our fiducial 50% completeness limit. This region is excluded from the fitting procedure.