Photometric quantities for synthetic galaxies that consist of a bulge and a disk forming according to the τ0.5+contSF (left column), τ1+τ5 (middle column) and τ1+iB (right column) model (cf. Fig. A.1). Results from EvCon and single-age simulations are shown, respectively, with thin solid and dotted curves. Thick curves show rest-frame values in V (green) and H (gray), as obtained from EvCon models. Simulated galaxies in the first two columns comprise only stellar emission, whereas those in the right-hand column additionally include nebular emission.