UV excess as a function of Hα equivalent width (a) and mass accretion rate as a function of UV excess (b). More negative values indicate larger UV excess. The UV excess and mass accretion rate were calculated by Venuti et al. (2014) and the Hα equivalent width was measured by Sousa et al. (2016) and Dahm & Simon (2005). As expected, diskless stars do not present UV excess, while full disk systems do. Transition disk candidates, in general, present UV excess similar to stars with full disks, which is consistent with active accretion, as discussed in the text.