\begin{table}%t1[htbp]
  %\centering
\par
  \caption{Best fit NFW model parameters and their 68\% CL
    uncertainty (marginalized over all the other parameters).
    (SL) corresponds to a model in which weak lensing constraints
    are ignored whereas (SL+WL) takes both strong and weak lensing
    constraints into account. (1)~Refers to the CHANDRA
    X-rays values of \citet{allen01}. The apparent disagreement
    between their estimates and ours is discussed in the text.} 
  \label{tab:resNFW}
  \begin{tabular}{ccccc}\hline\hline
                & (SL) & (SL+WL) & (1)  &Unit\\\hline
    $\kappa_{\rm s}$   & $0.67\pm0.05$ & $0.66\pm0.03$  & $0.30\pm0.15$  &   \\
    $r_{\rm s}$    & $\rm 158\mypm{15}{13}$ & $\rm 162\mypm{11}{9}$ & $160\pm30$ &$\hmkpc$ \\
    $r_{\rm 200}$& $1.88\pm{0.05}$ & $1.89\pm{0.04}$ & $\rm 1.39\mypm{0.49}{0.38}$ &$\hmMpc$\\
    $M_{\rm 200}$ & $\rm 7.56\mypm{0.63}{0.54}$ & $\rm 7.72\mypm{0.47}{0.42}$ & -- &$10^{14}\hmmsun$ \\
    $c$          & $\rm 11.92\mypm{0.77}{0.74}$ & $11.73\pm0.55$ & $\rm 8.7\mypm{1.2}{0.9}$& \\
    $q$          & $0.774\pm0.010$ & $0.777\pm0.007$ & --  &  \\
    $\psi_0$   & $5.86\pm0.14$ & $5.88\pm0.13$ & --  & deg \\
    $\Upsilon_V$ & $2.40\pm0.45$ & $2.48\pm0.39$ & --  &$\mslsun$\\\hline
  \end{tabular}
\end{table}