\begin{table}%T3
%\centering
\renewcommand{\arraystretch}{1.25}
\caption{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. \label{brightones}}
$$
\begin{tabular}{|l|r@{ $z$ }l|r@{$\pm$}l|c|c|c|} \hline\hline
Model &\multicolumn{2}{c|}{$z$ interval}&\multicolumn{2}{c|}{$A$} &
 $\gamma$ & ${\cal I}$ &  $\xi_{1{\rm ~Mpc}}$   \\ \hline
 &$0.25\leq~$ &$<0.5$&$27.38$&$^{5.31}_{4.45}$&$1.98\pm0.14$&$8.26$&$6.80\pm^{1.02}_{0.85}$\\\cline{2-8}
\raisebox{1.5ex}[-1.5ex]{$\Omega_{\rm m}=1$}&$0.5\leq~$&$<0.75$&$11.14$&$^{3.27}_{2.53}$&$2.02\pm0.19$&$4.12$&$4.05\pm^{0.87}_{0.67}$\\\cline{2-8}
\raisebox{1.5ex}[-1.5ex]{$\Omega_\Lambda=0$}&$0.75\leq~$&$\leq1.07$&$3.88$&$^{1.31}_{0.98}$&$2.03\pm0.18$&$1.06$&$1.82\pm^{0.48}_{0.36}$\\\hline
&$0.25\leq~$ &$<0.5$&$31.50$&$^{6.55}_{5.42}$&$1.85\pm0.17$&$10.24$&$8.02\pm^{1.26}_{1.04}$\\\cline{2-8}
\raisebox{1.5ex}[-1.5ex]{$\Omega_{\rm m}=0.2$}&$0.5\leq~$&$<0.75$&$15.42$&$^{3.98}_{3.16}$&$2.02\pm0.16$&$4.66$&$5.34\pm^{1.06}_{0.84}$\\\cline{2-8}
\raisebox{1.5ex}[-1.5ex]{$\Omega_\Lambda=0$}&$0.75\leq~$&$\leq1.07$&$5.01$&$^{1.81}_{1.33}$&$1.97\pm0.22$&$1.30$&$2.31\pm^{0.66}_{0.48}$\\\hline
&$0.25\leq~$ &$<0.5$&$39.46$&$^{8.15}_{6.76}$&$1.83\pm0.18$&$12.74$&$10.01\pm^{1.57}_{1.29}$\\\cline{2-8}
\raisebox{1.5ex}[-1.5ex]{$\Omega_{\rm m}=0.3$}&$0.5\leq~$&$<0.75$&$22.21$&$^{5.27}_{4.26}$&$2.00\pm0.16$&$5.85$&$7.23\pm^{1.40}_{1.13}$\\\cline{2-8}
\raisebox{1.5ex}[-1.5ex]{$\Omega_\Lambda=0.7$}&$0.75\leq~$&$\leq1.07$&$6.19$&$^{2.78}_{1.92}$&$2.11\pm0.25$&$1.33$&$2.81\pm^{1.04}_{0.72}$\\\hline
\end{tabular}
$$
\end{table}