\begin{table}%t5
\caption{Summary of best-fitting parameters of the SEDs of the
sources. We give the total galactic extinctions in magnitudes~$A_{\ion{H}{i}}$ and
$A_{\rm H_2}$, the X-ray extinction of the source in magnitudes~$A_{\rm x}$ and then the
parameters themselves: the extinction in the optical~$A_{\rm v}$, the temperature~$T_\ast$ and the
$\frac{{R}_{\ast}}{{D}_{\ast}}$ ratio of the companion and the temperature and radius~$T_{\rm D}$ and ${R}_{{\rm D}}$ (in ${R}_{\ast}$ unit) of the dust component when needed. We also add the reduced~$\chi^2$ we reach for each fit.}\label{tab5} 
%\centering
\small
\begin{tabular}{c c c c c c c c c c}
  \hline
  \hline
%&&&&&&&&& \\[-8pt]
Sources & $A_{\ion{H}{i}}$ & $A_{\rm H_2}$ & $A_{\rm x}$ & $A_{\rm v}$ & $T_{\ast} ({\rm K})$ & $\frac{{R}_{\ast}}{{D}_{\ast}}$ & $T_{\rm D} ({\rm K})$ & ${R}_{\rm D} \left({R}_{\ast}\right)$ & $\chi^2/{\rm d.o.f.}$\\
%&&&&&&&&& \\[-8pt]
\hline
%&&&&&&&&& \\[-8pt]
IGR~J16195-4945 & 11.7 & 28.6 & 37.4 & 15.5 & 23~800 & $5.96\times 10^{-{11}}$ &1160&5.1&3.9/2\\
IGR~J16207-5129 & 9.3&11.8&19.8&10.5&33~800& $9.42\times10^{-{11}}$&&&28.5/9\\
IGR~J16318-4848 &11.0&19.2&1069.5&17.0&22~200& $3.74\times 10^{-{10}}$ &1100&10.0&6.6/6\\
IGR~J16320-4751 &11.4&23.6&112.2&35.4&33~000& $1.38\times 10^{-{10}}$ &&&7.7/6\\
IGR~J16358-4726 &11.8&39.4&176.4&17.6&24~500& $3.16\times 10^{-{11}}$ &810&10.1&3.6/2\\
IGR~J16418-4532 &10.1&19.3&53.5&14.5&32~800& $3.77\times 10^{-{11}}$ &&&1.4/4\\
IGR~J16465-4507 &11.3&31.4&320.7&5.9&25~000& $6.40\times 10^{-{11}}$ &&&13.9/7\\
IGR~J16479-4514 &11.4&43.8&41.2&18.5&32~800& $1.00\times 10^{-{10}}$ &&&7.4/6\\
IGR~J17252-3616 &8.3&20.1&80.2&20.8&32~600& $7.57\times 10^{-{11}}$ &&&3.8/5\\
IGR~J17391-3021 &7.3&23.9&160.4&9.2&31~400& $1.80\times 10^{-{10}}$ &&&11.7/10\\
IGR~J17544-2619 &7.7&41.5&7.70&6.1&31~000& $1.27\times10^{-{10}}$ &&&6.1/8\\
IGR~J19140+0951 &9.0&14.0&32.1&16.5&22~500& $1.92\times10^{-{10}}$ &&&14.4/6\\
\hline
\end{tabular}
\end{table}