\begin{table}%t5
%\centering
\par
\caption{Measurements of the clustering length and slope for 
galaxy subsamples divided following the color bimodality.
\label{table_red_blue}}
\small
\begin{tabular}{l c c c c c c}
\hline\hline
\noalign{\smallskip}
Sample  & Number of & Redshift  & Effective & $M_{B_{AB}} - 5 \log(h)$ &         $r_0(z)$        &        $\gamma$        \\
        & galaxies  & range     & redshift  &        mean             &      ($h^{-1}$~Mpc)     &                        \\
\hline
  red   &   270     & 0.2--0.5 &   0.345   &          --17.858        &  $\rm 3.84^{+0.87}_{-0.93}$ & $\rm 1.88^{+0.23}_{-0.16}$ \\
        &   277     & 0.5--0.7 &   0.610   &          --18.784        &  $\rm 4.35^{+0.65}_{-0.71}$ & $\rm 1.99^{+0.22}_{-0.18}$ \\
        &   355     & 0.7--0.9 &   0.809   &          --19.565        &  $\rm 3.78^{+0.70}_{-0.74}$ & $\rm 1.87^{+0.28}_{-0.22}$ \\
        &   296     & 0.9--1.2 &   1.022   &          --20.221        &  $\rm 3.72^{+0.63}_{-0.67}$ & $\rm 1.83^{+0.32}_{-0.32}$ \\
\hline
\noalign{\smallskip}
  blue  &   980     & 0.2--0.5 &   0.357   &          --17.521        &  $\rm 2.07^{+0.34}_{-0.39}$ & $\rm 1.67^{+0.14}_{-0.09}$ \\
        &  1164     & 0.5--0.7 &   0.604   &          --18.544        &  $\rm 2.55^{+0.39}_{-0.41}$ & $\rm 1.68^{+0.15}_{-0.09}$ \\
        &  1042     & 0.7--0.9 &   0.811   &          --19.183        &  $\rm 2.18^{+0.32}_{-0.30}$ & $\rm 1.40^{+0.16}_{-0.11}$ \\
        &  1105     & 0.9--1.2 &   1.035   &          --19.749        &  $\rm 2.49^{+0.28}_{-0.22}$ & $\rm 1.84^{+0.14}_{-0.10}$ \\
        &   574     & 1.2--2.0 &   1.404   &          --20.651        &  $\rm 3.24^{+0.63}_{-0.70}$ & $\rm 1.91^{+0.20}_{-0.18}$ \\
\hline
\end{tabular}
\end{table}