\begin{table}%t1
%\centering
\par
\caption{\label{lxlo_ho}LogX-ray vs. Log[OIII] luminosity relation in optically selected AGN.}
\begin{tabular}{lccccc}
\hline\hline
Sample & Number & Slope &  Intercept & $ \langle \log(L_{\rm x}/L_{\rm [OIII]})\rangle$ & Dispersion  \\
  \hline 
A. Seyfert-1 (Ho \& Heckman)& 28 & $0.84\pm0.09$  & $8.27\pm 3.87$ & 1.66 & 0.60 \\    
B. Seyfert-1 (Ho)           &  8 & $0.66\pm0.22$ & $15.31\pm8.84$ & 1.84 & 0.82 \\
C. Seyfert-1 (Heckman)      & 20 & $1.04\pm0.17$ & $-0.17\pm7.34$ & 1.59 & 0.48 \\
D. Seyfert-2  (Ho luminous+weak)      & 23 & $0.83\pm0.15$ & $7.3\pm6.1$ & 0.87 & 0.80 \\
E. Seyfert-2 (Ho luminous)  & 11  & $0.64\pm0.17$ & $15.34\pm7.15$ & 1.16 & 0.77 \\
F. Seyfert-2 (Ho weak)      & 12 & $0.59\pm0.29$ & $16.18\pm 11.48$ & 0.61 & 0.78 \\
G. Seyfert 1 + 2 (luminous)     & 17 & $0.65\pm0.14$ & $15.35\pm5.90$ & 1.44 & 0.84 \\  
\hline 
\end{tabular}
\end{table}