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Table 9

Ages and reddening values for the sample clusters, as obtained by adopting the PROSECCO, PARSEC, and MIST isochrones in the (J,H, Ks) and in the (J, H, Ks, V) planes – first and second set of values, respectively.


PROSECCO PARSEC MIST
Cluster τ(Myr) E(BV) τ(Myr) E(BV) τ(Myr) E(BV)
NGC 2451A
NGC 2451B
NGC 2516
NGC 2547
IC 2391
IC 2602
IC 4665
NGC 6633a

NGC 2451A
NGC 2451B
NGC 2516
NGC 2547
IC 2391
IC 2602
IC 4665
NGC 6633a
             

Notes. (a) βov = 0.250 in the PROSECCO models.

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