\begin{table}%t2
\caption{\label{tab:iter}The ML-parameter sets which occur when choosing different starting cosmologies in the iterative likelihood analysis.}
%\centering
\small
\begin{tabular}{c| c c| c c| c c| c c| c c}	
\hline \hline
Step& \multicolumn{2}{|c|}{run1}& \multicolumn{2}{|c|}{run2} &\multicolumn{2}{|c|}{run3} &\multicolumn{2}{|c|}{run4} &\multicolumn{2}{|c}{run5} \\ 
&$\om$&$\sig$&$\om$&$\sig$&$\om$&$\sig$&$\om$&$\sig$&$\om$&$\sig$ \\ 
\hline
$\vpi_{\rm start}$ & 0.20 &0.60& 0.237 &0.740& 0.250 &0.90& 0.274 &0.850& 0.40 &1.0 \\
$\vpi_{\rm ML}$ 1& 0.254 &0.892& 0.254 &0.892&0.245  &0.914& 0.259 &0.884& 0.277 &0.858 \\
$\vpi_{\rm ML}$ 2& 0.260 &0.882& 0.260 &0.882& 0.245 &0.914& 0.260 &0.882& 0.259 &0.884 \\
$\vpi_{\rm ML}$ 3& 0.260 &0.882& 0.260 &0.882&  \multicolumn{2}{|c|}{converged}& 0.260 &0.882& 0.260 &0.882 \\
$\vpi_{\rm ML}$ 4&\multicolumn{2}{|c|}{converged}&\multicolumn{2}{|c|}{converged}& \multicolumn{2}{|c|}{converged} &\multicolumn{2}{|c|}{converged}& 0.260 &0.882 \\
\hline
\end{tabular}
\end{table}