Left: Model SED fits to the observed SED of IRAS 04361+2547 using from top to bottom: IRAC points only, JHK + IRAC points, JHK + IRAC + IRAS 12 and 25 μm, JHK + IRAC + All IRAS bands, and JHK + IRAC + All IRAS bands + submillimeter points (when more than 200 model SEDs fit the data well, we show the 200 best‐fit SEDs, and one in 10 SEDs beyond this). Center and right: Selection of parameters for the model fits. Filled circles are the good fits shown in the SED plots. The gray scale shows the parameter space of the grid of models as for Fig. 3. The alignment of all the fits along a curve in the ﹩T_{\star }﹩ vs. ﹩M_{\star }﹩ plots (right) is due to the sampling of the models using evolutionary tracks, i.e., for a given ﹩M_{\star }﹩ and ﹩t_{\star }﹩ we find ﹩T_{\star }﹩ using evolutionary tracks (see Paper I).