Spectral energy distributions of the sources for which we have detected an IR excess. The black dots indicate the photometric measurements used in the fit, the grey crosses indicate the photometric measures not used in the fit (either poor-quality photometry or upper limits), and the red triangles indicate a photometric excess detected by VOSA. We report the 3σ uncertainties, some of which are smaller than the markers. We note that the DANCe photometry has a minimum uncertainty of 0.05 mag. The grey line represents the photospheric best fitted Kurucz model.