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Table 2:

Newly derived ages, metallicity and reddening for the target clusters and other clusters included in the analysisa.

Name
$\log$(t) $\Delta$log(t) Z E(B-V) Mvb
This survey          
B015D-D041 7.85 $\pm $0.15 0.019 0.60 -8.53
B040-G102 7.90 $_{\rm -0.15}^{+0.20}$ 0.019 0.23 -7.80
B043-G106 7.90 -0.15+0.20 0.019 0.23 -8.22
B066-G128 7.85 $\pm0.15$ 0.019 0.23 -7.76
B081-G142 8.15 $\pm0.15$ 0.019 0.30 -8.60
B257D-D073 7.90 $_{\rm -0.15}^{+0.20}$ 0.019 0.40 -8.31
B318-G042 7.85 $\pm0.15$ 0.008 0.17 -7.98
B321-G046 8.23 $_{\rm -0.15}^{+0.10}$ 0.019 0.25 -7.57
B327-G053 7.70 $_{\rm -0.10}^{+0.15}$ 0.008 0.20 -8.51
B376-G309 8.00 $\pm0.15$ 0.019 0.30 -7.34
B448-D035 7.90 $_{\rm -0.15}^{+0.20}$ 0.019 0.35 -8.07
B475-V128 8.30 $\pm0.20$ 0.008 0.35 -8.00
V031 8.45 $\pm0.15$ 0.004 0.35 -8.12
VdB0 7.40 $\pm0.30$ 0.019 0.20 -10.03
B083-G146 >8.70 $\dots$ 0.008 0.20 -8.00
B222-G277 >8.60 $\dots$ 0.019 0.20 -7.66
B347-G154 >8.80 $\dots$ 0.008 0.06 -8.16
B374-G306 >8.50 $\dots$ 0.019 0.30 -7.09
NB16 >8.70 $\dots$ 0.019 0.25 -7.69
P09b          
B049-G112 8.45 $\pm $0.20 0.019 0.30 -7.84
B367-G292 8.30 $\pm $0.20 0.019 0.25 -6.79
B458-D049 8.50 $\pm $0.20 0.019 0.25 -7.40
B521 8.60 $\pm $0.30 0.019 0.55 $\dots$
M039 8.50 $\pm $0.20 0.019 0.10 -5.84
M050 8.75 $\pm $0.30 0.019 0.15 -6.22
WH01          
B315-G038 8.00 $_{\rm -0.20}^{+0.15}$ 0.008 0.31 -8.96
B319-G044 8.00 $_{\rm -0.20}^{+0.15}$ 0.008 0.23 -7.57
B342-G094 8.20 $_{\rm -0.20}^{+0.15}$ 0.008 0.20 -7.36
B368-G293 7.80 $\pm $0.10 0.019 0.20 -7.17

Notes. For five surveyed clusters only a lower limit to the age can be obtained from our CMDs. (a) The additional clusters are six clusters studied in Perina et al. (2009a), from HST archive data, and the four clusters studied by Williams & Hodge (2001). (b) Integrated V magnitudes from the RBC.


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