\begin{table}%t3
\caption{Rest-frame properties inferred for the two sources dominated by stellar light.\label{tab3}      }
%\centerline
{\begin{tabular}{l c c c c }    
\hline\hline       
                      % To combine 4 columns into a single one 
Source  &  $L_{K}$ & $M_{\rm star}$ & $M_{\rm BH}^{\rm a}$ & $L/L_{\rm Edd}^{\rm b}$\\ 
        & $(L_{\odot})$ & $(M_{\odot})$ & $(M_{\odot})$ & \\ 
\hline                    
BPM16274\#069  & $\rm 8.3\times 10^{11}$ & $\rm 4\times 10^{11}$ & $\rm 2\times 10^9$ & 0.04 \\ 
Abell2690\#075 &  $\rm  1.7\times10^{12}$   & $8 \times 10^{11}$ & $\rm 3\times 10^9$ & 0.10 \\ 
\hline                  
\end{tabular}}
\par
\smallskip
Notes: $^a$ Inferred black hole mass assuming the $L_{\rm K}-M_{\rm BH}$ relation
obtained by \cite{marconi03} for local galaxies. $^b$ Eddington ratio assuming
a bolometric correction $L_{\rm bol}/L_{\rm X}=30$.
\end{table}