\begin{table}%t5
\caption{Cosmological density parameters.} 
\label{table:no4} 
%\centering
\par
\begin{tabular}{c c c} 
\hline\hline 
Fit & $\Omega_{\rm M}$ & $\Omega_{\Lambda}$ \\ 
\hline 
$d_{\rm l}(z)$ LZ & $0.04 \pm 0.03$ & $0.65 \pm 0.73$  \\ 
$d_{\rm l}(z)$ GGL & $0.46 \pm 0.43$ & $0.54 \pm 2.82$  \\
$\ln [d_{\rm l}/z ~{\rm Mpc}]$ LZ & $0.37 \pm 0.31$ & $0.63 \pm 1.13$ \\
$\ln [d_{\rm l}/z ~{\rm Mpc}]$ GGL & $0.28 \pm 0.30$ & $0.72 \pm 1.09$ \\
\hline 
\end{tabular}
\end{table}