RGB images corresponding to ﹩0.3,0.5﹩, and 1 μm colors from model LATTE for three different viewing angles. Dust lanes in the galaxy (here, the dust mass is tied to the metal mass as a model assumption) are visible. As in Figure 8, the model galaxy is set at 30 Mpc. Images generated following the Lupton et al. (2004) scalings.