Table 4: The measured amplitude of the projected correlation function at $r_{\rm p}=316 ~h^{-1}$ kpc and the integral constraint ${\cal I}$, in different redshift intervals for two SED bins, for different world models.
\begin{displaymath}\begin{tabular}{\vert l\vert r@{ $z$ }r\vert c\vert c\vert r\... ...5\pm^{3.89}_{2.74}$&$1.89\pm0.28$&$1.98$\\ \hline \end{tabular}\end{displaymath}


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