Examples of SEDs of some of the members with IR excess. 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. The rest of SEDs of objects with IR excesses are displayed in the online material.