\begin{table}%t6
\caption{\label{tab6}The 1$\sigma$ confidence intervals of the mass in the form of dark matter.}
%\centerline
 {\begin{tabular}{ccc} 
\hline\hline    
 & Sal, BC/Sal, M & Cha, BC/Kro, M \\
\noalign{\smallskip} \hline \noalign{\smallskip}
$M_{{\rm D}}[(R_{{\rm Ein}}/R_{{\rm e}}) \le 0.2]~(M_{*})$ & $[0.04,0.22]$ & $[0.18,0.43]$ \\
$M_{{\rm D}}[(R_{{\rm Ein}}/R_{{\rm e}}) \le 0.6]~(M_{*})$ & $[0.19,0.31]$ & $[0.58,0.70]$ \\
$M_{{\rm D}}[(R_{{\rm Ein}}/R_{{\rm e}}) \le 1.0]~(M_{*})$ & $[0.20,0.41]$ & $[0.63,1.12]$ \\
 \hline
\end{tabular}}
\par
\smallskip
Notes: in each aperture, the lower and upper limits of the intervals are chosen as the smallest and the largest values predicted, at 1$\sigma$ confidence level, by the best-fit  {\it power-law} and  {\it pseudo-Jaffe} models. These values are given in units of the luminous mass, that is determined by adopting a Salpeter ({\it left}) or Chabrier/Kroupa ({\it right}) IMF.
\end{table}