SED models for the debris disks. Left: the photometry data are shown as red circles and triangles (upper limits). Stellar photospheric, disk, and total emission (stellar photospheric + disk models) are represented by gray dotted lines, and red and blue continuous lines, respectively (see Table 2 for details on individual models). The blue dots in the SED of RX J1005.3-7749 show the detection from Murphy et al. (2010). Right: results of the SED modeling of the debris disks showing the mass of the disk as a function of the location of the narrow dust ring.