\begin{table}%t3
\caption{\label{tab_lit}Values adopted from the literature (Table~\ref{dadosliteratura}) for the clusters studied in this work, where masses are estimated based on models by \cite{schulz02}.}
\par
%\centering
\par
\begin{tabular}{lcccc}
\hline \hline \noalign{\smallskip}
Cluster &  Age  & [$Z/Z_{\odot}$]  & log($M/M_{\odot}$) & log($M/M_{\odot}$) \\
        &  (Gyr) &                 & Salpeter & Scalo \\
\hline
HW1                 & 5      $\pm$  1.0  	& --0.7   $\pm$ ---  & --- & --- \\
K3                    & 6.5   $\pm$  0.5  	& --1.2   $\pm$ 0.2   & 5.0  & 4.6  \\
L3             	& 1.5   $\pm$  0.5  	& --0.7   $\pm$ ---  & --- & --- \\
L11          	& 3.5   $\pm$  0.5  	& --0.8   $\pm$ 0.14 & 4.0  & 3.7  \\
L113                & 4.0   $\pm$  0.7           & --1.24 $\pm$ 0.11 & --- & --- \\
NGC 121 	  	& 11    $\pm$  0.5  	& --1.46 $\pm$ 0.10 & 5.5  & 5.2  \\
NGC 152 		& 3.0   $\pm$  1.0  	& --1.25 $\pm$ 0.25 & 4.4  & 3.9  \\
NGC 222        	& 0.10 $\pm$  0.03	& --0.3   $\pm$ ---  & 3.8  & 3.8  \\
NGC~256        	& 0.10 $\pm$  0.03	& --0.3   $\pm$ ---  & 3.8  & 3.8  \\
NGC~269        	& 0.3   $\pm$  0.2  	& --0.3   $\pm$ ---  & 4.0  & 3.8  \\
NGC~294        	& 0.4   $\pm$  0.2  	& --0.3   $\pm$ ---  & 4.4  & 4.0  \\
NGC~361 		& 6.8   $\pm$  0.5  	& --1.45 $\pm$ 0.11 & 5.1  & 4.7  \\
NGC~419        	& 1.4   $\pm$  0.2  	& --0.3   $\pm$ ---  & 5.3  & 4.9  \\
NGC~458        	& 0.13 $\pm$  0.06	& --0.23 $\pm$ ---  & 3.9  & 4.2  \\
\hline
\end{tabular}
\end{table}