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Fig. 14.


Radial velocity single cluster members (grey circles), (likely) binary members (black circles) and additional Gaia/TGAS proper motion members (white squares) of NGC 3532 in four colour-magnitude diagrams. For comparison with each other and the data we show the YaPSI (blue), PARSEC (green), BaSTI (orange), MIST (yellow), and BHAC (purple, not available in (B − V)) models. The solar-mass model for 300 Myr is marked with a black plus sign.

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