\begin{table}%t4
\caption{\label{tabyoung}Weights of stellar populations obtained by modelling of OASIS~data, and compared to \citet{Cid04}, on aperture ${\sim}1\arcsec$. The symbols~$\mu_{\rm Y},\mu_{\rm I},\mu_{\rm O}$ denote mass fractions of young, intermediate and old populations, respectively. Analogously for $\mu_{\rm young}$, $\mu_{\rm old}$ in our OASIS~data.}
%\centering
\small
\begin{tabular}{l|ll|lll}
\hline\hline
Galaxy & \multicolumn{2}{c|}{OASIS data}& \multicolumn{3}{c}{\citet{Cid04}} \\
& $\mu_{\rm young}$ & $\mu_{\rm old}$ & $\mu_{\rm Y}$ &  $\mu_{\rm I}$ & $\mu_{\rm O}$ \\
\hline
NGC 2992 & 0.09 &  0.91 &      0.0000 & 0.0260  & 0.9740 \\
NGC 3081 & 0.008&  0.992&      0.0000 & 0.0000  & 1.0    \\
NGC 4388 & 0.02 & 0.98  &      0.0002 & 0.0000  & 0.9998 \\
NGC 5728 & 0.06 & 0.94  &      0.0002 & 0.0699  & 0.9299 \\
\hline
\end{tabular}
\end{table}