Disk models for selected SEDs of dust-depleted disks (magenta lines). See Table 4 for information on the individual models. For comparison, the photosphere of a star with the same spectral type from the MARCS models (Gustafsson et al. 2008) is displayed. All datapoints have been extinction-corrected according to their individual values of A_V and assuming a standard extinction law (see Table A.1). Information about the Hα EW (in Å) is also displayed.