Example of an MCFOST model with SEDs for all 10 different inclinations. The blue points show the stellar flux at different wavelengths between 0.1 µm and 2 µm (both shown as vertical blue lines). The blue line encode the limit, which is used to distinguish non- shielded inclinations (green SEDs) that were accepted for the sample and shielded inclinations (red SEDs) that were discarded.