SEDs for the 30 Taurus‐Auriga sources analyzed in this paper. Filled circles are the flux values listed in Tables 8, 9, 10 and 11. Triangles are upper limits. Error bars are shown if larger than the data points. The solid black line indicates the best‐fitting model, and the gray lines show all models that also fit the data well (defined by ﹩\chi ^{2}-\chi ^{2}_{\mathrm{best}\,}< 3﹩, where χ² is the value per data point). The dashed line shows the SED of the stellar photosphere in the best‐fitting model.