\begin{table}%t5
%
\par
\caption{\label{masses}\label{table3}Bolometric luminosities, black hole masses, and Eddington ratios.}
%\centerline
 {
\begin{tabular}{lrcccr}
\hline \hline
\noalign{\smallskip}
Source & $\log{L_{\rm{bol}}}$ & Ref. & $\log{M_{\rm{BH}}}$ & Ref. & $\log{\frac{L_{\rm{bol}}}{L_{\rm{Edd}}}}$ \\
&(${\rm erg}~{\rm s}^{-1}$)& & ($M_{\odot}$) & & \\
(1)&(2)&(3)&(4)&(5)&(6)\\
\hline
4C12.03      & $<$42.0 & 6     &   8.5 & 9     & $<$$-$4.6 \\
3C~015        & $<$42.8 & 1     &   8.8 & 4     & $<$$-$4.1 \\
3C~029        &      42.3 & 3     &   9.1 & 3     &      $-$4.9 \\
3C~040        & $<$41.5 & 3     &   7.9 & 2     & $<$$-$4.5 \\
3C~078        &      43.5 & 3     &   8.9 & 3     &      $-$3.5 \\
Fornax~A     & $<$41.1 & 5     &   8.4 & 1     & $<$$-$5.4 \\
3C~093        &      45.3 & 3     &   9.5 & 6     &      $-$2.3 \\
3C~098        & $<$41.5 & 1     &   7.9 & 8     & $<$$-$4.5 \\
3C~105        &      43.6 & 5     &   7.8 & 10    &      $-$2.3 \\
3C~120        &      45.3 & 4     &   7.4 & 8     &      $-$0.2 \\
3C~135        &      43.2 & 1     &   8.5 & 7     &      $-$3.4 \\
Pictor~A     &      44.3 & 3     &   8.7 & 6     &      $-$2.5 \\
3C~198        &      43.9 & 1     &   8.1 & 4     &      $-$2.3 \\
3C~227        &      44.9 & 3     &   8.9 & 6     &      $-$2.1 \\
3C~270        &      40.4 & 3     &   8.6 & 3     &      $-$6.3 \\
Centaurus~A  &      41.1 & 2     &   7.7 & 5     &      $-$4.7 \\
PKS1417$-$19 &      45.3 & 3     &   8.3 & 6     &      $-$1.1 \\
3C~317        &      42.4 & 3     &   9.5 & 3     &      $-$5.2 \\
3C~327        & $<$42.4 & 1     &   9.1 & 4     & $<$$-$4.8 \\
3C~353        & $<$41.4 & 1     &   7.6 & 4     & $<$$-$4.3 \\
PKS1839$-$48 &      44.5 & 5     &   8.7 & 10    &      $-$2.3 \\
3C~403        &      42.5 & 1     &   8.5 & 4     &      $-$4.1 \\
3C~403.1      & $<$42.0 & 6     &   8.1 & 10    & $<$$-$4.2 \\
3C~424        & $<$42.6 & 5     &   7.8 & 7     & $<$$-$3.3 \\
PKS2158$-$380& $<$42.0 & 6     &   8.6 & 2     & $<$$-$4.7 \\
3C~445        &      44.8 & 3     &   8.0 & 6     &      $-$1.3 \\
PKS2354$-$35 & $<$42.0 & 7     &   9.2 & 10    & $<$$-$5.3 \\
\hline
\end{tabular}}
\tablefoot {\textit{Columns~(2, 3)} Logarithm of bolometric luminosity from: 1~=~\cite{2004MNRAS.351..733M}, 2~=~\cite{2007AetA...471..453M}, 3~=~\cite{2007ApJ...658..815S}, 4~=~\cite{2002ApJ...579..530W}, 5~=~calculated from bolometric correction \citep{1994ApJS...95....1E, 2004MNRAS.351..733M} to optical nuclear luminosity \citep{1993MNRAS.263..999T, 2006AetA...447...97B}, 6~=~upper limit from spectral energy distribution fit in Fig.~\ref{allsedsLEG} and \ref{allsedsHEG}. \textit{Columns~(4, 5)} Logarithm of black hole mass from: 1~=~\cite{2006AetA...447...97B}, 2~=~\cite{2003AetA...399..869B}, 3~=~\cite{2004MNRAS.349.1419C}, 4~=~\cite{2004MNRAS.351..733M}, 5~=~\cite{2007ApJ...671.1329N}, 6~=~\cite{2007ApJ...658..815S}, 7~=~\cite{2005ApJ...631..762W}, 8~=~\cite{2002ApJ...579..530W}, 9~=~calculated from the velocity dispersion $\sigma$ \citep{2007AetA...470..531W} using the $M_{{\rm BH}}-\sigma$ correlation from \cite{2002ApJ...574..740T}, 10~=~calculated from B- or V-band absolute magnitudes \citep{1985MNRAS.216..173W, 1995ApJ...448..521Z} following the work of \cite{2004MNRAS.351..733M}. \textit{Column~(6)} Efficiency expressed in the logarithm of the bolometric to Eddington luminosity ratio.}
%\vspace*{3mm}
\end{table}