\begin{table}%t4
%\centering
\par
\caption{\label{tab:limmass}Limiting masses (in logarithm of solar masses) of our various samples
in order to define volume-limited samples, as a function of the redshift
ranges and for various mass-to-light completeness levels.}
\small \begin{tabular}{lccccccccccccccc}
\hline \hline 
& \multicolumn{3}{c}{$z<0.5$} & \multicolumn{3}{c}{$z<0.6$} & \multicolumn{3}{c}{$z<0.7$} & \multicolumn{3}{c}{$z<0.8$} & \multicolumn{3}{c}{$z<0.9$}\\
\hline
 & 50\% & 80\% & 95\% & 50\% & 80\% & 95\% & 50\% & 80\% & 95\% & 50\% & 80\% & 95\% & 50\% & 80\% & 95\%\\
wide (all) & $9.6$ & $10.0$ & $10.2$ & $9.7$ & $10.2$ & $10.4$ & $9.9$ & $10.3$ & $10.6$ & $10.0$ & $10.5$ & $10.7$ & $10.2$ & $10.6$ & $10.9$\\
wide (star-forming) & $9.3$ & $9.6$ & $9.9$ & $9.4$ & $9.7$ & $10.1$ & $9.6$ & $9.9$ & $10.2$ & $9.7$ & $10.0$ & $10.3$ & $9.8$ & $10.1$ & $10.4$\\
deep (all) & $8.7$ & $9.2$ & $9.5$ & $8.9$ & $9.3$ & $9.7$ & $9.0$ & $9.5$ & $9.9$ & $9.1$ & $9.6$ & $10.0$ & $9.2$ & $9.7$ & $10.1$\\
deep (star-forming) & $8.6$ & $8.9$ & $9.2$ & $8.7$ & $9.0$ & $9.3$ & $8.8$ & $9.0$ & $9.3$ & $8.8$ & $9.1$ & $9.4$ & $8.9$ & $9.2$ & $9.5$\\
\hline
\end{tabular}
\end{table}