\begin{table}%T4
\par
      \caption{\label{tab:allbandfits}Best fit results for the 7 objetcs in Fig.~\ref{fig:sedplots}.}
  \small%\centering
\par
    \begin{tabular}{lrrrrrlrrrrr}
      \hline
      \hline\noalign{\smallskip}
      ID & $z_{\rm phot}$ & $\chi^{2}_{\rm min}/\nu$ & $P_{\chi^2}$ & $\nu$ & Ext. & Age & $\Theta$ & $\theta_{\rm view}$ & $\log[L_{\rm sb}]$ & $\log[L_{\rm agn}]$ & $\log[L_{\rm tot}]$ \\
         &              &                         &             &       &      & (Myr) &       & (deg)             &  ($L_{\odot}$) &  ($L_{\odot}$) &  ($L_{\odot}$)  \\
      \hline\noalign{\smallskip}
1716 & $\rm 1.02_{-0.27}^{+0.12}$ & 1.99 & 0.01 & 13 & LMC & $\rm 500_{-100}^{+100}$ & $\rm 1.4_{-0.1}^{+0.6}$ & $\rm 47_{-3}^{+42}$ & $\rm 12.0_{-0.11}^{+0.16}$ & $\rm 10.4_{-0.51}^{+0.17}$ & $\rm 12.0_{-0.11}^{+0.16}$ \\
1771 & $\rm 0.78_{-0.11}^{+0.93}$ & 4.45 & 0.00 & 13 & SMC & $\rm 400_{-370}^{+200}$ & $\rm 1.6_{-0.4}^{+1.4}$ & $\rm 42_{-3}^{+3}$ & $\rm 12.3_{-0.31}^{+0.93}$ & $\rm 10.9_{-0.02}^{+1.09}$ & $\rm 12.3_{-0.27}^{+0.92}$ \\
1827 & $\rm 0.76_{-0.14}^{+0.07}$ & 2.65 & 0.00 & 13 & LMC & $\rm 500_{-100}^{+100}$ & $\rm 1.6_{-0.1}^{+0.1}$ & $\rm 47_{-3}^{+10}$ & $\rm 11.4_{-0.23}^{+0.12}$ & $\rm 9.92_{-0.18}^{+0.07}$ & $\rm 11.4_{-0.24}^{+0.11}$ \\
1985 & $\rm 0.88_{-0.15}^{+0.27}$ & 1.33 & 0.19 & 11 & MW & $\rm 500._{-470.}^{+100.}$ & $\rm 2.0_{-1.3}^{+0.4}$ & $\rm 50_{-42}^{+3}$ & $\rm 11.5_{-0.06}^{+0.47}$ & $\rm 9.87_{-0.29}^{+1.41}$ & $\rm 11.5_{-0.06}^{+0.48}$ \\
2412 & $\rm 0.12_{-0.06}^{+0.06}$ & 1.35 & 0.17 & 13 & MW & $\rm 600_{-100}^{+0}$ & $\rm 3.0_{-0.1}^{+0.1}$ & $\rm 47_{-3}^{+3}$ & $\rm 10.0_{-0.53}^{+0.53}$ & $\rm 8.52_{-1.04}^{+0.38}$ & $\rm 10.1_{-0.65}^{+0.41}$ \\
2483 & $\rm 0.04_{-0.03}^{+2.53}$ & 1.40 & 0.16 & 11 & LMC & $\rm 10_{-0}^{+590}$ & $\rm 1.2_{-0.9}^{+1.8}$ & $\rm 45_{-3}^{+3}$ & $\rm 9.67_{-1.77}^{+3.38}$ & $\rm 9.24_{-1.73}^{+3.44}$ & $\rm 10.7_{-2.65}^{+2.52}$ \\
2885 & $\rm 1.00_{-0.38}^{+0.48}$ & 0.87 & 0.47 & 4 & SMC & $\rm 600_{-590}^{+100}$ & $\rm 0.7_{-0.4}^{+4.3}$ & $\rm 8_{-3}^{+30}$ & $\rm 11.9_{-0.17}^{+0.51}$ & $\rm 11.5_{-1.71}^{+0.02}$ & $\rm 12.0_{-0.28}^{+0.40}$ \\
      \noalign{\smallskip}\hline\end{tabular}
\tablefoot{$z_{\rm phot}$: Best fit photometric redshift; $\chi^{2}_{\rm min}/\nu$: reduced minimum~$\chi^2$ for  $\nu$ degrees of freedom; $P_{\chi^2}$: probability associated to the minimum $\chi^2$; ext.: extinction curve; age: age of the starburst; $\Theta$: starburst compactness factor; $\theta_{\rm view}$: viewing angle of the AGN torus; $\log[L_{\rm sb}]$:  luminosity contributed by the starburst component; $\log[L_{\rm agn}]$: luminosity contributed by the AGN component;  $\log[L_{\rm tot}]$: total luminosity.} 
\end{table}