\begin{table}%t3
\caption{\label{tab3}Derived fundamental parameters.}
\small%\centerline
 {
\begin{tabular}{lrrrrr}
\hline\hline \noalign{\smallskip}
Cluster&Age&$N_{1\sigma}$&$E(B-V)$&$d_{\odot}$&$R_{\rm GC}$\\
&(Gyr)&&(mag)&(kpc)&(kpc)\\
 ($1$)&($2$)&($3$)&($4$)&($5$)&($6$)\\
\hline
Be~63 &$0.03\pm0.01$&3.7&$0.96\pm0.03$&5.7&11.8\\
Be~84 &$0.36\pm0.05$&5.4&$0.58\pm0.06$&1.7&6.8\\
Cz~6 &$0.01\pm0.005$&8.3&$0.26\pm0.03$&2.7&6.9\\
Cz~7 &$0.22\pm0.05$&3.6&$0.70\pm0.03$&3.3&9.7\\
Cz~12 &$1.25\pm0.4$&4.6&$0.26\pm0.03$&2.0&8.8\\
Ru~141 &$0.03\pm0.02$&12.8&$0.45\pm0.1$&1.8&5.5\\
Ru~144 &$0.45\pm0.1$&7.7&$0.77\pm0.1$&1.6&5.7\\
Ru~172 &$0.9\pm0.2$&5.6&$0.64\pm0.06$&3.1&7.0\\
FSR~101 &$0.9\pm0.2$&7.1&$2.37\pm0.03$&1.9&7.1\\
FSR~1430 &$1.0\pm0.3$&8.3&$2.56\pm0.03$&3.6&8.4\\
FSR~1471 &$1.0\pm0.2$&6.2&$1.22\pm0.02$&2.7&7.7\\
FSR~162 &$0.2\pm0.05$&3.5&$1.57\pm0.03$&7.1&7.5\\
FSR~178 &$1.5\pm0.5$&3.9&$1.34\pm0.03$&3.7&6.4\\
FSR~198 &$0.01\pm0.005$&6.6&$0.96\pm0.03$&1.7&6.9\\
\hline
\end{tabular}}
\medskip
Notes. The parameter $N_{1\sigma}$  corresponds to the ratio of the number of stars in the decontaminated CMD with respect to the $1\sigma$~Poisson fluctuation measured in the observed CMD \citep{Bica2007}. Column~4: reddening in the cluster's central region. Column~6: $R_{\rm GC}$~calculated using $R_{\odot}=7.2$~kpc \citep{Bica2006b} as the distance of the Sun to the Galactic centre. Uncertainties in~$d_{\odot}$ and $R_{\rm GC}$ are of the order of~$0.1$~kpc.
\end{table}