\begin{table}%T6
%\centering
\par
\caption{The parameter $q$ for early type ($SED\leq60$) 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. \label{qparaSEDtab}}
\begin{tabular}{l|c c c}\hline\hline
Cosmology& $q(SED\leq60)$, without LCRS&$q(SED\leq60)$, with
LCRS&$q_{\rm bright}$\\\hline
$\Omega_{\rm m}=1.0$, $\Omega_\Lambda=0.0$&$-2.60\pm0.91$ &$-1.52\pm0.30$ &$-3.44\pm0.29$\\
$\Omega_{\rm m}=0.2$, $\Omega_\Lambda=0.0$&$-2.03\pm0.82$ &$-0.74\pm0.28$ &$-2.84\pm0.30$\\
$\Omega_{\rm m}=0.3$, $\Omega_\Lambda=0.7$&$-0.85\pm0.82$ &$-0.34\pm0.28$ &$-2.28\pm0.31$\\\hline
\end{tabular}
\end{table}