\begin{table}%t8
%\centering
\par
\caption{\label{tab_dynres}Halo circular velocity $V_{\rm c}$, halo core radius $r_{\rm c}$, average dark matter density $\langle \rho_{\rm DM} \rangle$ (within $2 ~ r_{\rm eff}$) and stellar mass-to-light ratio
$\Upsilon$ (last column: photometric band) for the best-fit dynamical models of
\object{NGC~1600}, \object{NGC~4125} and \object{NGC~7619} (no cutoff radius).}
\par
\begin{tabular}{lccccc}
\hline\hline \noalign{\smallskip}
Name   & $V_{\rm c}$  & $r_{\rm c}$ & $\log_{10} \langle \rho_{\rm DM} \rangle$ & $\Upsilon$ & band\\
& (km~s$^{-1}$) & (kpc) & ($M_\odot/pc^3$) & ($M_\odot/L_{\odot}$) &\\
\hline\noalign{\smallskip}
\object{NGC~1600} &  $\rm 350^{+250}_{-50}$  & $\rm 31^{+62}_{-12}$ & $-2.1 \pm 0.5$ & $7.3 \pm 0.5$ & $R$\\
\object{NGC~4125}  & $\rm 350^{+100}_{-100}$  & $\rm 32^{+7}_{-7}$ & $-2.2 \pm 0.1$ & $5.7 \pm 0.7$ & $I$\\
\object{NGC~7619}  & $\rm 600^{+200}_{-150}$  & $\rm 49^{+9}_{-16}$ & $-2.0 \pm 0.2$ & $6.5 \pm 0.5$ & $I$\\
\noalign{\smallskip}\hline\noalign{\smallskip}
\end{tabular}
\end{table}