**Table 5:** The amplitudes of the three-dimensional correlation function $\xi (r)$ at a comoving distance of r=1 Mpc, for red ( $SED\leq 60$ ) and blue (*SED*>60) galaxies; the integral constraint has been taken into account in the calculation.
$\begin{displaymath}\begin{tabular}{\vert l\vert r@{ $z$ }r\vert c\vert c\vert} \... ...m^{6.51}_{3.44}$&$4.01\pm^{1.42}_{0.98}$\\ \hline \end{tabular}\end{displaymath}$

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