Fig. 5.
Comparison between the Pisa best isochrone (corresponding to 
Myr, 
mag and 
mag) and the observations in several photometric bands, namely BV (Piatti et al. 1998), JHKs (2MASS), GBPGRPG (Gaia DR2), and gri (VPHAS+). The uncertainties in magnitude and colour are too small to show on the two right-most diagrams. No uncertainties were available for the BV photometry.
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