\begin{table}%t4
\caption{\label{resultstable}Summary of the main results.}
\par
%\centering
\par
\begin{tabular}{l l l l}
\hline
\hline \noalign{\smallskip}
Method & $\sigma_v$ [$\kms$]& $r_{200}$ [kpc] & $M_{200}$ [$10^{14}~{M_\odot}$]\\
\hline
Galaxy counts       & --                  & \boldmath$811\pm46$   & $0.74\pm0.15$\\
Spectr. (early type)  & \boldmath$480\pm20$ & $1054\pm44$           & $1.69\pm0.14$\\
Spectr. (late type) & \boldmath$590\pm20$ & $1295\pm44$           & $3.14\pm0.21$\\
X-ray ($\beta$-model) & \boldmath$316\pm26$ & $617\pm28$          & $0.34\pm0.10$\\
Weak lens. (SIS)  & \boldmath$476\pm46$ & $853\pm82$            & $0.90\pm0.26$\\
Weak lens. (NFW)  & --                  & \boldmath$834\pm219$  & $0.84\pm0.66$\\
Weak lens. (MR)   & --                  & $650\pm50$\tablefootmark{*}        & \boldmath$0.38\pm0.09$\tablefootmark{*}  \\
Strong lensing      & \boldmath$319\pm4$  & $700\pm9$             & $0.50\pm0.01$\\
\hline
\end{tabular}
\tablefoot {Values in bold face are the primary measurements, the others were derived from these. \\
\tablefoottext{*}{The mass estimate from the weak lensing mass reconstruction is obtained within a~radius of 182~kpc, significantly smaller than~$r_{200}$. The given values are therefore lower limits.}}
\end{table}