\begin{table}%t5
\caption{\label{tab:combLF}Combined binned local AGNLF, based on the SDSS broad line galaxy sample (faint end) and the Hamburg/ESO Survey (bright end).}
%\centerline
 {\small \begin{tabular}{rrrr}
\hline \hline \noalign{\smallskip} \noalign{\smallskip} 
$M_B$  & $\log \Phi(M_B)$  & $\log L_{\rm Bol}$ & $\log \Phi(L_{\rm Bol})$ \\ 
\noalign{\smallskip} \hline \noalign{\smallskip}
$-$14.2 & $\rm -2.60^{+0.11}_{-0.14}$ & 42.63 & $\rm -2.12^{+0.10}_{-0.15}$ \\ \noalign{\smallskip} 
$-$14.8 & $\rm -2.95^{+0.12}_{-0.18}$ & 42.83 & $\rm -2.48^{+0.13}_{-0.18}$ \\ \noalign{\smallskip} 
$-$15.4 & $\rm -3.00^{+0.08}_{-0.09}$ & 43.03 & $\rm -2.52^{+0.07}_{-0.1}$ \\ \noalign{\smallskip} 
$-$16.0 & $\rm -3.49^{+0.07}_{-0.09}$ & 43.24 & $\rm -3.02^{+0.07}_{-0.09}$ \\ \noalign{\smallskip} 
$-$16.6 & $\rm -3.63^{+0.08}_{-0.10}$ & 43.44 & $\rm -3.16^{+0.07}_{-0.10}$ \\ \noalign{\smallskip} 
$-$17.2 & $\rm -4.10^{+0.08}_{-0.09}$ & 43.65 & $\rm -3.64^{+0.08}_{-0.08}$ \\ \noalign{\smallskip} 
$-$17.8 & $\rm -4.26^{+0.08}_{-0.08}$ & 43.86 & $\rm -3.80^{+0.07}_{-0.08}$ \\ \noalign{\smallskip} 
$-$18.4 & $\rm -4.44^{+0.08}_{-0.09}$ & 44.07 & $\rm -3.98^{+0.07}_{-0.10}$ \\ \noalign{\smallskip} 
$-$19.0 & $\rm -4.69^{+0.07}_{-0.10}$ & 44.28 & $\rm -4.24^{+0.07}_{-0.10}$ \\ \noalign{\smallskip} 
$-$19.6 & $\rm -5.04^{+0.09}_{-0.10}$ & 44.49 & $\rm -4.59^{+0.08}_{-0.10}$ \\ \noalign{\smallskip} 
$-$20.2 & $\rm -5.46^{+0.06}_{-0.08}$ & 44.71 & $\rm -5.02^{+0.06}_{-0.08}$ \\ \noalign{\smallskip} 
$-$20.8 & $\rm -5.78^{+0.07}_{-0.08}$ & 44.93 & $\rm -5.34^{+0.06}_{-0.08}$ \\ \noalign{\smallskip} 
$-$21.4 & $\rm -6.36^{+0.09}_{-0.12}$ & 45.15 & $\rm -5.93^{+0.10}_{-0.11}$ \\ \noalign{\smallskip} 
$-$22.0 & $\rm -6.85^{+0.09}_{-0.11}$ & 45.38 & $\rm -6.42^{+0.09}_{-0.11}$ \\ \noalign{\smallskip} 
$-$22.6 & $\rm -7.19^{+0.08}_{-0.10}$ & 45.60 & $\rm -6.77^{+0.09}_{-0.10}$ \\ \noalign{\smallskip} 
$-$23.2 & $\rm -7.40^{+0.08}_{-0.09}$ & 45.82 & $\rm -6.98^{+0.08}_{-0.09}$ \\ \noalign{\smallskip} 
$-$23.8 & $\rm -7.87^{+0.10}_{-0.11}$ & 46.05 & $\rm -7.45^{+0.10}_{-0.11}$ \\ \noalign{\smallskip} 
$-$24.4 & $\rm -8.20^{+0.12}_{-0.16}$ & 46.28 & $\rm -7.78^{+0.12}_{-0.17}$ \\ \noalign{\smallskip} 
$-$25.0 & $\rm -8.76^{+0.20}_{-0.37}$ & 46.51 & $\rm -8.34^{+0.19}_{-0.38}$ \\ 
 \hline
\end{tabular} }
\medskip
The bolometric AGNLF has been computed using the bolometric corrections by \citet{Marconi:2004}.
\vspace*{2mm}
\end{table}