\begin{table}%t3
%\centering
\par
\caption{\label{tab3}Basic parameters obtained for the investigated  clusters.} 
\begin{tabular}{lccccccccc}
\hline\hline
& \multicolumn{4}{c}{Fit} & &\multicolumn{3}{c}{Literature} \\
{Cluster} & {$E(B-V)$} & {Distance} & {Log(Age)} & {$Z$} & & {$E(B-V)$} &  {distance} & {Log(Age)}   &  {Ref.} \\
& (mag) & (pc)   & (yr)   &     & &    (mag) & (pc)   & (yr)   &          \\  
\hline 
\object{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   \\
\object{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   \\
\object{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    \\
\object{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    \\
\object{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    \\
    \object{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   \\
    \object{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    \\
    \object{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    \\
    \object{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    \\
\hline      
\end{tabular} 
\tablefoot{The numbers,  in the last column are the WEBDA reference codes, $E(B-V)$ is the extinction, {\em 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 \cite{PN06}.}
\end{table}