\begin{table}%t5
\caption{\label{Tableparameters}Parameters of our SED models using or not submm constraints and Dust-to-Gas mass ratios of our galaxies.}
\small%\centerline
 {
 \begin{tabular}{c|cc|cc|cc}
\hline
\hline
&&&&&& \\[-8pt]
& \multicolumn{2}{c|}{Haro~11}  & \multicolumn{2}{c|}{Mrk~1089} & \multicolumn{2}{c}{NGC~1705} \\
& no submm & submm &  no submm &  submm & no submm &  submm \\
\hline
&&&&&& \\[-8pt]
$M_{\rm dust}$ (\msun)	& 6.2 $\times$ 10$^6$ &  1.7 $\times$ 10$^7$ ($\pm$40$\%$)       & 3 $\times$ 10$^7$  &  {\bf{5.12 $\times$ 10$^7$}} ($\pm$20$\%$)  $^a$    &  2.9 $\times$ 10$^4$   & 1.3 $\times$ 10$^6$ ($\pm$50$\%$) \\
$f_{\rm PAH}$   & 0.22   & 0.1      & 0.18 &  0.18 &  0.11 & 4.4 $\times$ 10$^{-2}$\\
$\alpha$ 	  &  1.88 	 &  1.73	& 2.21&  2.18    & 2.5     &1.84 \\
$U_{\rm min}$      & 12.2    &  1.44   &  1.5	    &  0.82 & 3.68      & 9 $\times$ 10$^{-3}$\\
$U_{\rm max}$     & 1.3 $\times$ 10$^5$      & 5.77 $\times$ 10$^4$    &  3.84 $\times$ 10$^5$ 	 &  3.5 $\times$ 10$^5$    &  1.47 $\times$ 10$^4$    & 8.67 $\times$ 10$^2$\\
\hline
&&&&&& \\[-8pt]
$M_{\rm HI}$  (\msun) & \multicolumn{2}{c|}{$\sim$10$^{8}$} &  \multicolumn{2}{c|}{2.7 $\times$ 10$^{10}$} & \multicolumn{2}{c}{4.1 $\times$ 10$^{7}$ $^b$} \\
$M_{\rm dust}$/$M_{\rm HI}$  & 6 $\times$ 10$^{-2}$ & 0.17 & 10$^{-3}$ & {\bf 1.9 $\times$ 10$^{-3}$} & 7 $\times$ 10$^{-4}$ & 3.2 $\times$ 10$^{-2}$\\
\hline
\end{tabular}}
\medskip
$^a$ Bold numbers are the dust mass and the dust-to-gas mass ratio values of our prefered SED for the galaxy Mrk~1089.  \\ 
$^b$ HI mass associated with the aperture chosen for the dust mass determination, namely 80\% of the the total HI~mass.
\vspace*{2.3mm}
\end{table}