\begin{table}%t4
\caption{\label{table:darkmatter}Mass models for Malin~1 and NGC~7589.}
%\centerline
{\small
\begin{tabular}{l c c}
\hline
\hline
Parameter & MALIN 1 & NGC 7589 \\
\hline
$M_{*}/L_{R}$ ($M_{\odot}/L_{\odot}$) & 3.4 & 2.5\\
$\rho_{0}$ ($10^{-3} \; M_{\odot}$ pc$^{-3}$) & $121.4 \pm 93.8$ & $2.3 \pm 0.3$\\
$r_{\rm{C}}$ (kpc) & $2.2 \pm 0.9$ & $19.9 \pm 2.0$\\
$\chi^{2}_{r}$ & 4.6 & 4.0\\
\hline
$M_{\rm{HSB}}/L_{R}$ ($M_{\odot}/L_{\odot}$) & 3.3 & 2.6\\
$M_{\rm{LSB}}/L_{R}$ ($M_{\odot}/L_{\odot}$) & 0.9 & 0.9\\
$\rho_{0}$ ($10^{-3} \; M_{\odot}$ pc$^{-3}$) & $73.9 \pm 36.5$ & $2.4 \pm 0.2$\\
$r_{\rm{C}}$ (kpc) & $2.9 \pm 0.8$ & $20.7 \pm 1.6$\\
$\chi^{2}_{r}$ & 3.1 & 2.7\\
\hline
\end{tabular}}
\tablefoot{\textit{Top}: mass models using a single stellar component and maximizing the stellar mass-to-light ratio. \textit{Bottom}: mass models using a HSB-LSB decomposition. The stellar mass-to-light ratio of the LSB disk was fixed at 0.9, whereas that of the HSB disk was maximized. See text for details.}
\end{table}