**Table 2:** The measured amplitude of the projected correlation function in different redshift intervals, at $r_{\rm p}\approx316 ~h^{-1}$ kpc for CADIS and at $r_{\rm p}\approx500 ~h^{-1}$ kpc for the LCRS (first lines), respectively, the integral constraint ${\cal I}$ and $\xi_{1{\rm ~Mpc}}$ as calculated from the ${\cal I}$ -corrected amplitudes of $w(r_{\rm p})$ , for different world models. Numbers in italic indicate that this values are inferred from the LCRS.
$\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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