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Fig. 5.


Same as Fig. 3 (with the same color scale) for all stars in the PMS and Upper-MS loci from Fig. 4. The red polygon is the same as in Fig. 3. Dots indicate members from PM16 (their Table 7), with Gaia parallax π >  5. Outside the red polygon the density of stars is very low, but not zero. The dotted gray polygon is a reference region to estimate contamination (see Sect. 4.4).

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