Spectral energy distribution of systems classified as full disks. The circles show data from the U band (0.3 μm) to the MIPS 24 μm band. The black solid line is the best fit to the SED (Robitaille 2017) and the dashed lines correspond to the stellar (blue) and dust (red) emission components (Robitaille 2011). The gray solid lines are all the model with , where n_data is the number of available data points from the literature, following Robitaille (2017). All these systems were observed by Spitzer at 24 μm and/or WISE at 22 μm.