\begin{table}%t3
%\centering
\par
\caption {\label{tab3}Parameters that have been used to obtain the best fit between
the observed CMD and the BaSTI isochrones.}
\par
\scriptsize {
\begin{tabular}{lcccll}
\hline\hline  ID  &  $(m-M)_{0}$ & $\it{E(B-V)}$ & $Z$  &  Age (Myr) & $\Delta_{\rm{age}}$ \\
%------------------------------------------------------------------------
\hline
ESO057-SC075 & 18.46 & 0.14 & 0.008 & 1400--1600 & $200\pm50$ \\
HODGE7  & 18.48 & 0.04 & 0.008 & 1400--1550 & $150\pm50$ \\
IC2146  & 18.50 & 0.07 & 0.008 & 1550      & $<$50      \\ 
NGC~1644 & 18.48 & 0.01 & 0.008 & 1550      & $<$50      \\ 
NGC~1652 & 18.48 & 0.06 & 0.008 & 1700      & $<$50      \\ 
NGC~1751 & 18.45 & 0.22 & 0.008 & 1300--1500 & $200\pm50$ \\
NGC~1783 & 18.46 & 0.06 & 0.008 & 1400--1600 & $200\pm50$ \\
NGC~1795 & 18.45 & 0.10 & 0.008 & 1300      & $<$50      \\ 
NGC~1806 & 18.44 & 0.09 & 0.008 & 1400--1600 & $200\pm50$ \\
NGC~1846 & 18.49 & 0.09 & 0.008 & 1350--1600 & $250\pm50$ \\
NGC~1852 & 18.50 & 0.08 & 0.008 & 1200--1450 & $250\pm50$ \\
NGC~1917 & 18.48 & 0.08 & 0.008 & 1200--1350 & $150\pm50$ \\
NGC~1978 & 18.49 & 0.09 & 0.008 & 2000      & $<$100     \\ 
NGC~1987 & 18.40 & 0.04 & 0.010 &  950--1200 & $250\pm50$ \\
NGC~2108 & 18.40 & 0.21 & 0.010 &  950--1100 & $150\pm50$ \\
NGC~2154 & 18.48 & 0.04 & 0.008 & 1350--1500 & $150\pm50$ \\
%----------------------------------------------------------------------
\hline
\end{tabular}
}
\end{table}