Fig. 9.— The SEDs of our non-accreting transition disk targets. All of them have low disk masses ( < 2.5 M$_{JUP}$ ), and are consistent with photoevaporation. The filled circles are detections while the arrows represent 3- σ limits. The open squares correspond to the observed optical and near-IR fluxes before being corrected for extinction using the A$_{J}$ values listed in Table 3 and the extinction curve provided by the Asiago database of photometric systems (Fiorucci & Munari 2003). For each object, the average of the two R-band magnitudes (from the USNO-B1 catalog) listed in Table 1 has been used. The solid blue line represent the stellar photosphere normalized to the extinction-corrected J-band. The dotted lines correspond to the median mid-IR SED of K5–M2 CTTSs calculated by Furlan et al. (2006). The dashed lines are the quartiles. – 58 –