Modeled optical and 4.5 μm lightcurves for Mon-660 at i = 77°. The modeled CoRoT lightcurve is represented by filled circles, and the modeled Spitzer photometric magnitudes at 4.5 μm are plotted as solid squares. For comparison the observed + 1σ CoRoT (points) and the + 1σ Spitzer 4.5 μm (asterixs) lightcurves are presented. We use all the cycles presented in McGinnis et al. (2015) to calculate the observed curves. At the upper left corner, we show the value for the mean standard deviation for the CoRoT and Spitzer data.