\begin{table}%t4
\caption{\label{tab4}Summary of parameters we used to fit the SEDs of the sources. We give their name and then the parameters themselves: the extinction in the optical~$A_{v}$, the temperature~$T_{\rm \ast}$ and the $\frac{R_{\rm \ast}}{D_{\rm \ast}}$~ratio of the star, and the
temperature~$T_{\rm D}$ and radius~$R_{\rm D}$ (in $R_{\rm \ast}$~unit) of the dust component. We also add the reduced~$\chi^2$ we reach for each fit, as well as the uncertainties on the parameters.}
\par
%\centering
\small
  \begin{tabular}{ccccccc}
    \hline
    \hline
%&&&&&& \\[-8pt]
    {Sources}& $A_{v}$ & $T_{\rm \ast}[\Delta{T_{\rm \ast}}](\textrm{K})$ & $\frac{R_{\rm \ast}}{D_{\rm \ast}}$ & $T_{\rm  D} (\textrm{K})$ & $R_{\rm D}\left(R_{\ast}\right)$ & $\chi^2/\textrm{d.o.f.}$\\
%&&&&&& \\[-8pt]
    \hline
%&&&&&& \\[-8pt]
    {LBV~1806-20 (A) (2005)}& $\rm {28.6}_{-1.5}^{+1.5}$ & $21~500~[17~900{-}26~200]$ & $3.08_{-0.48}^{+0.36}\times10^{-{10}}$ & $\rm 1130_{-110}^{+130}$ & $\rm 8.4_{-0.9}^{+1.0}$ & $3.1/4$\\
    {LBV~1806-20 (A) (2006)}& $\rm 29.0_{-1.2}^{+1.2}$ & $17~600~[15~000{-}21~200]$ & $3.68_{-0.36}^{+0.24}\times10^{-{10}}$ & $\rm 1020_{-100}^{+140}$ & $\rm 6.5_{-0.7}^{+0.7}$ & $3.9/4$\\
    {WC9 (B)}& $\rm 35.2_{-1.8}^{+1.4}$ & $53~000~[25~000{-}71~000]$ & $4.36_{-0.68}^{+1.36}\times10^{-{11}}$ & $\rm 1850_{-120}^{+60}$ & $\rm 46.0_{-14.0}^{+8.0}$ & $6.8/4$\\
    {Supergiant (C)}& $\rm 31.8_{-2.1}^{+0.8}$ & $25~700~[11~600{-}40~500]$ & $1.38_{-0.36}^{+0.62}\times10^{-{10}}$ &&& $6.0/5$\\
    \hline
  \end{tabular}
\end{table}