\begin{table}%t9
\caption{Luminous and dark mass measurements of the lens galaxy, without the cluster contribution. The ranges represent the intervals at 68\% confidence level.}
\label{table:11}
%\centering
\small
\begin{tabular}{c c c c c}
\hline\hline 
& $M_{{\rm len}}$ &  $M_{{\rm dyn}}$ & $M_{{\rm phot}}$ & $f_{{\rm DM}}$ \\
 & $(10^{11}~M_{\odot})$ & $(10^{11}~M_{\odot})$ & $(10^{11}~M_{\odot})$ &  \\ 
 \hline
  $R\leq8.10$ kpc & $3.9{-}5.2$ & $2.8{-}4.0$ & $0.6{-}0.9$ & $0.44{-}0.99$ \\ 
  $R\leq9.54$ kpc & $4.6{-}6.2$ & $3.3{-}4.7$ & $0.7{-}1.1$ & $0.50{-}0.99$ \\ 
  \hline
\end{tabular}
\end{table}