SEDs of the members and probably members with IR excess typical of full-disks (continued). 213917481+571747432 has strong 8 μm, could be PTD. 213911452+572425205 has [3.6]−[4.5] = 0.27 and a strong kink in the SED, it could be a PTD although its 24 μm flux is likely contaminated by cloud emission. 214011348+574414105 has [3.6]−[4.5] = 0.11 but a SED that suggests strong variability and a flared, massive full-disk.