\begin{table}%t3
\caption{\label{tab3}Mass in stars formed in the last 1.0 and 6.2~Gyr for all the models compared with the total number of stars. Observed values by Kaviraj (\cite{Kavi08b}).}
%\centering
\small
\begin{tabular}{cccc}
\hline
\hline
Model & $M_{*}$ [$M_{\odot}$] (last 1.0 Gyr [$z$ = 0.08]) & $M_{*}$ [$M_{\odot}$] (last 6.2~Gyr [$z$~= 0.7]) & $M_{*}$ [$M_{\odot}$] (13.12~Gyr) \\
\hline
&&& \\[-8pt]
1 & 4.17 $\times$ $10^{8}$ (0.21\%) & 3.66 $\times$ $10^{9}$ (1.85\%) & 1.98 $\times$ $10^{11}$ \\
2 & 0.00 (0.00\%) & 0.00 (0.00\%) & 1.58 $\times$ $10^{11}$ \\
3 & 7.95 $\times$ $10^{9}$ (4.25\%) & 5.54 $\times$ $10^{10}$ (29.63\%) & 1.87 $\times$ $10^{11}$ \\
\hline
Kaviraj (\cite{Kavi08b}) & 1--6\% & 5--13\% & \\
\hline
\end{tabular}
\end{table}