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Fig. 13
Same as Fig. 12 but here for the Baraffe et al. (1998) 4 Myr isochrone and shifted to a distance of 4.8 kpc. The arrows indicate the 50% completeness limit as determined in the artificial star experiments. Log-normal fits are performed below 1 M⊙ down to the 50% completeness limit and shown as solid lines.
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