\begin{table}%t1
\caption{\label{SDSS_source}Properties of the SDSS type 2 AGN}
%\centerline
{
\small\begin{tabular}{c c c c c c}
\hline\hline
Name & log $M_{\rm BH}$$^{(a)}$ &log $L_{\rm OIII}^{(b)}$ &log $L^{\rm c}_{\rm OIII}$$^{(a)}$ & $F^{\rm obs}_{\rm X}$$^{(c)}$& log
$L^{\rm int}_{\rm X}$$^{(c)}$ \\
%(1)&(2)&(3)&(4)&(5)&(6)\\
&($M_{\odot}$)&(erg s$^{-1}$)&(erg s$^{-1}$)&(erg s$^{-1}$ cm$^{-2}$)&(erg s$^{-1}$)\\
\hline
SDSSJ075920.21+351903.4& 8.36 & 7.59&8.84&$1.3\times 10^{-14}$ &43.92   \\
SDSSJ083945.98+384319.0& 8.16 & 8.60&9.71 &$2.3\times 10^{-13}$ & 44.26    \\
SDSSJ084041.05+383819.9& 7.71 & 8.62& 9.48&$<$$4.4\times 10^{-14}$&$<$44.07   \\
SDSSJ092318.04+010144.7&8.53&8.94&9.31&$<$$4.0\times 10^{-14}$&$<$44.24\\ 
SDSSJ094820.38+582526.4& 7.01 & 7.89&9.08&$<$$4.2\times 10^{-14}$&$<$44.17   \\
SDSSJ133735.01-012815.6& 8.75 & 8.72&9.56&$<$$6.0\times 10^{-14}$&$<$44.25   \\
SDSSJ143027.66-005614.8& 7.61 & 8.36&9.23&$<$$8.6\times 10^{-14}$&$<$44.38   \\
SDSSJ143928.23+001538.0& 8.01 & 8.08&9.22&$6.6\times 10^{-14}$& 43.88\\
\hline
\end{tabular}} 
\medskip
\par
$^{(a)}$ From B06. $^{(b)}$ From Zakamska et~al (\cite{Zakamska2003}). $^{(c)}$ This work (see the Appendix).
%
%
%\caption{(1) SDSS name. (2) log of the black hole mass in units of M$_{\odot}$ from B06. (3) log of the [OIII] line luminosity in units of L$_{\odot}$ from Zakamska et~al (2003). (4) log of the extinction-corrected [OIII] line luminosity in units of L$_{\odot}$ from B06. (5) Observed \mbox{X-ray} flux in units of erg s$^{-1}$ cm$^{-2}$(see the Appendix).  (6) log of the de-absorbed \mbox{X-ray} luminosity in units of erg s$^{-1}$ (see the Appendix).
%($\ast$) Compton-thick source: L$^{int}_{X}$  is obtained assuming that the
%ratio between the reflected and the primary component is  0.05.
%  ($^{\dagger}$) this source has $z$=0.424 so the SDSS spectrum does not
%  cover the spectral range necessary to measure the H$\alpha$ line. The [OIII] line luminosity and the Balmer decrement measurements are obtained from observation collected with the  2.2 m telescope at the Centro Astron\'{o}mico Hispano Alem\'{a}n (CAHA) at
%Calar Alto. }
\end{table}