\begin{table}%t4
%\centering
\par
\caption{Number of galaxies and mean $B$ rest-frame absolute magnitude ($h=1$)
of the sample separated using the color bimodality. 
The number of "red'' and "blue'' galaxies classified
as early (T1\&2) and late (T3\&4) spectral types are identified.
We note that the populations of "red'' and T1\&2 as well
as the populations of "blue'' and T3\&4 galaxies are
mostly the same, except for a significant cross-over population
which could explain the observed difference
in clustering (see text).
\label{table_red_blue_t12_t34}}
\small
\begin{tabular}{c c c c c }
\hline\hline
\noalign{\smallskip}
 Redshift  & \multicolumn{2}{c}{Red} & \multicolumn{2}{c}{Blue} \\
 range     &    T1\&2   &    T3\&4   &    T1\&2   &    T3\&4    \\
\hline
 0.2--0.5 &       221  &       49   &       86   &     895     \\
           &    --18.181 &   --16.403  &   --18.701  &  --17.411    \\
\hline
 0.5--0.7 &       253  &       24   &      121   &     1044    \\
           &    --18.892 &   --17.646  &   --19.215  &  --18.467    \\
\hline
 0.7--0.9 &       313  &       42   &       77   &     965     \\
           &    --19.713 &   --18.468  &   --19.748  &  --19.138    \\
\hline
 0.9--1.2 &       283  &       13   &       88   &     1016    \\
           &    --20.263 &   --19.314  &   --20.557  &  --19.679    \\
\hline
 1.2--2.0 &       41   &        0   &       94   &    480      \\
           &    --20.926 &        0   &   --21.078  & --20.567     \\
\hline
\end{tabular}
\end{table}