SEDs of the members and probably members with low IR excess consistent with dust-depleted disks. This includes objects with disks but no significant 24 μm detection, in cloud-free regions. Some objects like 213844343+573626211 could be truncated disks. Objects like 213839749+572753080, 213854760+572450268, 213944898+573537212, 214000478+571839617, 214021922+573005424, and 214026262+573402317 may also have inner holes being thus both transitional and dust-depleted disk candidates. Inverted triangles mark upper limits, and open circles are uncertain values.