\begin{table}%T5
\par
    \caption{\label{tab:silcatebreakfits}Best fit results for the 7 objetcs in Fig.~\ref{fig:silicatebreakSED} for candidate Silicate Break galaxies.}
    \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)             &  ($L_{\odot}$) &  ($L_{\odot}$) &  ($L_{\odot}$)  \\
      \noalign{\smallskip}\hline\noalign{\smallskip}
933 & $\rm 0.84_{-0.17}^{+0.17}$ & 2.44 & 0.00 & 11 & MW & $\rm 500_{-10}^{+10}$ & $\rm 2.2_{-1.9}^{+2.8}$ & $\rm 50_{-50}^{+40}$ & $\rm 10.9_{-0.12}^{+0.14}$ & $\rm 10.1_{-0.36}^{+0.19}$ & $\rm 10.9_{-0.14}^{+0.15}$ \\
1130 & $\rm 1.28_{-0.35}^{+0.17}$ & 2.08 & 0.03 & 8 & LMC & $\rm 600_{-10}^{+10}$ & $\rm 1.0_{-0.3}^{+2.8}$ & $\rm 40_{-32}^{+3}$ & $\rm 11.5_{-0.24}^{+0.22}$ & $\rm 10.4_{-0.00}^{+0.89}$ & $\rm 11.6_{-0.23}^{+0.29}$ \\
1549 & $\rm 1.46_{-0.60}^{+0.46}$ & 1.41 & 0.19 & 7 & SMC & $\rm 600_{-100}^{+0}$ & $\rm 1.0_{-0.5}^{+0.8}$ & $\rm 8_{-8}^{+83}$ & $\rm 11.4_{-0.15}^{+0.16}$ & $\rm 11.5_{-2.09}^{+0.00}$ & $\rm 11.7_{-0.33}^{+0.00}$ \\
1772 & $\rm 1.28_{-0.11}^{+0.13}$ & 2.13 & 0.01 & 12 & MW & $\rm 300_{-10}^{+100}$ & $\rm 2.0_{-0.1}^{+0.1}$ & $\rm 47_{-47}^{+43}$ & $\rm 12.2_{-0.14}^{+0.12}$ & $\rm 10.4_{-0.12}^{+1.36}$ & $\rm 12.2_{-0.13}^{+0.22}$ \\
1818 & $\rm 1.20_{-0.27}^{+0.30}$ & 0.85 & 0.54 & 8 & MW & $\rm 600_{-300}^{+0}$ & $\rm 2.0_{-1.6}^{+1.0}$ & $\rm 47_{-3}^{+42}$ & $\rm 11.2_{-0.16}^{+0.42}$ & $\rm 10.5_{-0.14}^{+0.09}$ & $\rm 11.3_{-0.15}^{+0.44}$ \\
2009 & $\rm 1.28_{-0.75}^{+0.94}$ & 4.72 & 0.00 & 9 & MW & $\rm 500_{-300}^{+100}$ & $\rm 3.0_{-1.6}^{+2.0}$ & $\rm 90_{-90}^{+0}$ & $\rm 11.3_{-0.72}^{+0.20}$ & $\rm 10.7_{-0.83}^{+0.97}$ & $\rm 11.4_{-0.71}^{+0.50}$ \\
2541 & $\rm 1.24_{-0.21}^{+0.18}$ & 1.03 & 0.40 & 7 & MW & $\rm 600_{-100}^{+0}$ & $\rm 2.6_{-0.1}^{+0.1}$ & $\rm 8_{-3}^{+40}$ & $\rm 11.4_{-0.21}^{+0.07}$ & $\rm 11.2_{-1.60}^{+0.14}$ & $\rm 11.5_{-0.29}^{+0.21}$ \\
3096 & $\rm 1.42_{-0.42}^{+0.25}$ & 0.95 & 0.47 & 8 & MW & $\rm 400_{-100}^{+200}$ & $\rm 1.6_{-1.1}^{+0.2}$ & $\rm 8_{-3}^{+42}$ & $\rm 11.6_{-0.33}^{+0.09}$ & $\rm 10.9_{-1.18}^{+0.39}$ & $\rm 11.7_{-0.41}^{+0.06}$ \\
3124 & $\rm 1.26_{-0.19}^{+0.85}$ & 2.49 & 0.01 & 8 & SMC & $\rm 600_{-100}^{+0}$ & $\rm 1.0_{-0.1}^{+0.4}$ & $\rm 7_{-7}^{+32}$ & $\rm 11.8_{-0.14}^{+0.28}$ & $\rm 9.71_{-0.00}^{+1.73}$ & $\rm 12.0_{-0.33}^{+0.13}$ \\
     \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.} 
%\vspace*{-2mm} 
\end{table}