Table 6: The parameter q for early type ( $SED\leq 60$ ) galaxies, for a fit done without taking the the LCRS point into account, and for a fit including it. The evolution of the bright sample is shown for comparison.
Cosmology $q(SED\leq60)$ , without LCRS $q(SED\leq60)$ , with LCRS $q_{\rm bright}$

$\Omega_{\rm m}=1.0$ , $\Omega_\Lambda=0.0$ $-2.60\pm0.91$ $-1.52\pm0.30$ $-3.44\pm0.29$

$\Omega_{\rm m}=0.2$ , $\Omega_\Lambda=0.0$ $-2.03\pm0.82$ $-0.74\pm0.28$ $-2.84\pm0.30$

$\Omega _{\rm m}=0.3$ , $\Omega _\Lambda =0.7$ $-0.85\pm0.82$ $-0.34\pm0.28$ $-2.28\pm0.31$

**Table 6:** The parameter q for early type ( $SED\leq 60$ ) galaxies, for a fit done without taking the the LCRS point into account, and for a fit including it. The evolution of the bright sample is shown for comparison.
Cosmology	$q(SED\leq60)$ , without LCRS	$q(SED\leq60)$ , with LCRS	$q_{\rm bright}$
$\Omega_{\rm m}=1.0$ , $\Omega_\Lambda=0.0$	$-2.60\pm0.91$	$-1.52\pm0.30$	$-3.44\pm0.29$
$\Omega_{\rm m}=0.2$ , $\Omega_\Lambda=0.0$	$-2.03\pm0.82$	$-0.74\pm0.28$	$-2.84\pm0.30$
$\Omega _{\rm m}=0.3$ , $\Omega _\Lambda =0.7$	$-0.85\pm0.82$	$-0.34\pm0.28$	$-2.28\pm0.31$

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