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Fig. 12

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Series of spectral index plots shown as a function of stellar effective temperature, merging the known Taurus Class II (filled circles) and Class III (crosses) members with; mid-IR emission (IRAC, MIPS and WISE), far-IR emission (PACS and MIPS), and 1.3 mm emission (for those targets not with no reported 1.3 mm observations, the nearest submm/mm observation was scaled to 1.3 mm assuming Fνν2). Symbols leftwards of the vertical dotted lines, plotted at Teff = 2963 K and Teff = 3270 K, indicate the substellar (M6.25) members and members of the TBOSS sample (M4), respectively. Blue squares enclose the targets identified in the literature with transition disks and green squares enclose the candidate transition disks objects identified within this paper.

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