Fig. B.3
SEDs of the members and probably members with IR excess consistent with TD. Objects like 213819411+572203907, 213839571+572916412, 21394010+5730113 may be also dust-depleted. 213750297+570909399 may be partially contaminated by nebular emission but the detection is real. Inverted triangles mark upper limits, and open circles are uncertain values.
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