\begin{table}%t2
\caption{\label{tab:halo}Mass decomposition using isothermal halo.}
%\centering
\par
\begin{tabular}{l|ccc|cccc}
\hline\hline
 && {\bf{KK98~250}}    &&&& {\bf{KK98~251}}  &\\
{\bf{HI~Curve}}  &~$\Upsilon_V$&$r_{\rm c}$ (kpc)&$\rho_0~(10^{-3}~{M}_\odot$~pc$^{-3})$& &$\Upsilon_I$&$r_{\rm c}$ (kpc)&$\rho_0~(10^{-3}~{M}_\odot$~pc$^{-3})$\\\hline
Best fit  & 0.20~$\pm$~0.05&$1.5\pm0.2$&$37.6\pm1.2$&&$-$&$-$&$-$ \\
Maximum disk  & 3.0&$4.1\pm1.0$&$10.0\pm1.1$&&1.0&$10.5\pm14.5$&$13.4\pm1.6$ \\
From observed~$\langle V-I\rangle$  & 0.7&$1.6\pm0.1$&$30.4\pm1.0$ && 0.5&$4.2\pm1.6$&$15.7\pm1.3$ \\
Minimum disk &0.0&$1.4\pm0.04$&$39.0\pm1.0$& & 0.0&$2.8\pm0.5$&$18.5\pm1.0$ \\
Hybrid (HI+H$\alpha$) Curve &0.2 &$0.9\pm0.1$&$65.4\pm5.6$&&$-$ &$-$&$-$\\
H$\alpha$ Curve &0.0 &$0.63\pm0.08$&$117.8\pm16.5$&&$-$ &$-$&$-$\\
\hline
\end{tabular}
\end{table}