Observed and best-fitted flux densities for one example source, J120022.63-631523.2, for which we obtained T_eff = 1700 K and A_V = 0.5, which is a transition disk object according to Koenig & Leisawitz (2014)’s criteria. The dashed line indicates the observed photometric data. Circles represent dereddened data, where solid circles denote data points that have been considered in the fitting process by VOSA. The solid lines indicate the best-fitted BT-Settl model. Some infrared excess is evident at wavelengths larger than ~10 μm.