**Table 3:** The measured amplitude of the projected correlation function at $r_{\rm p}\approx316 ~h^{-1}$ kpc for the bright ( $M_B\leq-18+5 \log h$ ) galaxies, the integral constraint ${\cal I}$ , and $\xi_{1{\rm ~Mpc}}$ , calculated from the ${\cal I}$ -corrected A, for different world models. Note that for the bright sample the calculation for the first redshift bin was started at z=0.25 instead of z=0.2, because there are only very few bright galaxies at redshifts smaller than 0.3.
$\begin{displaymath}\begin{tabular}{\vert l\vert r@{ $z$ }l\vert r@{$\pm$}l\vert ... ...1\pm0.25$&$1.33$&$2.81\pm^{1.04}_{0.72}$\\ \hline \end{tabular}\end{displaymath}$

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