Table 5: Cosmological density parameters.
Fit $\Omega_{\rm M}$ $\Omega_{\Lambda}$
$d_{\rm l}(z)$ 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 $0.28 \pm 0.30$ $0.72 \pm 1.09$


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