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Table 3:

Basic parameters obtained for the investigated clusters.
  Fit   Literature  
Cluster E(B-V) Distance Log(Age) Z   E(B-V) distance Log(Age) Ref.
  (mag) (pc) (yr)     (mag) (pc) (yr)  
NGC 2477 $0.29\pm0.03$ $1385\pm64 $ $8.90\pm0.09$ 0.019   $0.26\pm0.08$ $ 1227\pm166$ $8.94\pm0.11 $ 152
NGC 7044 $0.55\pm0.05$ $3093\pm345 $ $9.35\pm0.17$ 0.019   $0.63\pm0.06$ $ 3097\pm145$ $9.26\pm0.08 $ 62
NGC 2266 $0.17\pm0.02$ $3100\pm244 $ $8.90\pm0.07$ 0.008   $0.10\pm0.01$ $ 3490\pm180$ $8.87\pm0.04 $ 41
Berkeley 32 $0.12\pm0.04$ $3483\pm186 $ $9.65\pm0.13$ 0.008   $0.15\pm0.03$ $ 3491\pm401$ $9.54\pm0.08 $ 40
NGC 2682 $0.02\pm0.01$ $774\pm25 $ $9.55\pm0.05$ 0.019   $0.05\pm0.02$ $ 820\pm47$ $9.61\pm0.09 $ 335
  $0.05\pm0.01$ $758\pm26 $ $9.60\pm0.06$ 0.019   $0.05\pm0.02$ $ 820\pm47$ $9.61\pm0.09 $ 31
  $0.04\pm0.01$ $869\pm57 $ $9.50\pm0.07$ 0.019   $0.05\pm0.02$ $ 820\pm47$ $9.61\pm0.09 $ 54
NGC 2506 $0.03\pm0.01$ $3587\pm198 $ $9.20\pm0.05$ 0.008   $0.06\pm0.04$ $ 3315\pm219$ $9.22\pm0.11 $ 284
  $0.07\pm0.01$ $3137\pm177 $ $9.25\pm0.05$ 0.008   $0.06\pm0.04$ $ 3315\pm219$ $9.22\pm0.11 $ 163
NGC 2355 $0.25\pm0.02$ $2316\pm103 $ $8.80\pm0.05$ 0.008   $0.14\pm0.06$ $ 2086\pm163$ $8.92\pm0.07 $ 217
  $0.19\pm0.02$ $2022\pm88 $ $8.85\pm0.05$ 0.008   $0.14\pm0.06$ $ 2086\pm163$ $8.92\pm0.07 $ 44
Melotte 105 $0.47\pm0.02$ $1750\pm111 $ $8.40\pm0.06$ 0.019   $0.48\pm0.05$ $ 2094\pm159$ $8.35\pm0.09 $ 289
  $0.49\pm0.03$ $2005\pm139 $ $8.45\pm0.07$ 0.019   $0.48\pm0.05$ $ 2094\pm159$ $8.35\pm0.09 $ 32
Trumpler 1 $0.59\pm0.05$ $2419\pm185 $ $7.85\pm0.19$ 0.019   $0.57\pm0.04$ $ 2356\pm511$ $7.48\pm0.08 $ 320
  $0.53\pm0.03$ $2309\pm121 $ $7.55\pm0.31$ 0.019   $0.57\pm0.04$ $ 2356\pm511$ $7.48\pm0.08 $ 86

Notes. The numbers, in the last column are the WEBDA reference codes, E(B-V) is the extinction, d the distance to the cluster, $\log(Age)$ the logarithm of the age (in years), Z the adopted metallicity. The literature values are those of Paunzen & Netopil (2006).


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