Fig. 14
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Age from isochrone fitting as a function of the α′ value (defined as the slope of the SED between W1 and W3 bands, see Sect. 3.4) for stars with mass >0.075 M⊙ belonging to CrA-Main (blue circles) and CrA-North (red open squares). The dashed lines separate the different categories of disks as labeled in Table 2. Thick disks and flat spectra are merged together.
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