\begin{table}%t4
\caption{\label{stackmag}Stacked magnitudes for the sample.}
%\centerline
{
\small\begin{tabular}{l c c c c }
\hline
\hline
 & Total sample  & Red sample & Blue sample & $K_{\rm s}$-detected  \\
\hline
\emph{u$^*$}     &   $25.21\pm0.03$   &  $25.16\pm0.05$  & $25.34\pm0.06$  & $24.75\pm0.06$  
\\
{\it Bj}                           &  $25.14\pm0.03$   &   $25.11\pm0.04$ & $25.34\pm0.05$ & $24.00\pm0.02$  
\\
{\it Vj}                           &  $24.99\pm0.08$   &  $24.89\pm0.11$  & $25.18\pm0.03$ & $23.04\pm0.01$  
\\
\emph{i$^+$}      &   $24.95\pm0.14$  &   $24.72\pm0.13$  & $25.37\pm0.15$ & $21.83\pm0.01$   
\\
\emph{z$^+$}     &   $24.86\pm0.22$  &   $24.57\pm0.15$ &  $25.40\pm0.16$  & $21.46\pm0.01$   
\\
$K_{\rm s}$                  &   $24.00\pm0.29$  &  $23.65\pm0.19$ &  $25.55\pm0.98^*$ & $20.44\pm0.02$   \\
\hline
\end{tabular}}
\medskip
\par
 Upper limits are $3\sigma$. $K_{\rm s}$-detected sample is without AGN-detected galaxies. $^*$Blue sample $K_{\rm s}$ magnitude is calculated from the $K_{\rm s}$ magnitudes of the total and red samples.
\end{table}