\begin{table}%t2
\caption{Multi-wavelength luminosities and $M_{\rm BH}$ of the total X-ray sample.}\label{x}
\footnotesize{
%\centering
\begin{tabular}{cccrrccrrrrr}
\hline
\hline
\multicolumn{1}{c}{Name} &
\multicolumn{1}{c}{Class}&
\multicolumn{1}{c}{Sat} &
\multicolumn{1}{r}{Log $F_{2-10 ~{\rm keV}}$}&
\multicolumn{1}{r}{Log $L_{2-10 ~{\rm keV}}$}&
\multicolumn{1}{r}{Ref.}&
\multicolumn{1}{r}{CThick}&
\multicolumn{1}{r}{Log $L_{\rm [OIII]}$}&
\multicolumn{1}{r}{Log $L_{\rm H\alpha}$}&
\multicolumn{1}{r}{Log $M_{\rm BH}$}&
\multicolumn{1}{c}{Method} &
\multicolumn{1}{r}{Ref.}\\
\multicolumn{1}{c}{(1)} &
\multicolumn{1}{c}{(2)} &
\multicolumn{1}{c}{(3)} &
\multicolumn{1}{c}{(4)} &
\multicolumn{1}{c}{(5)}&
\multicolumn{1}{c}{(6)} &
\multicolumn{1}{c}{(7)} &
\multicolumn{1}{c}{(8)} &
\multicolumn{1}{c}{(9)} &
\multicolumn{1}{c}{(10)} &
\multicolumn{1}{c}{(11)} &
\multicolumn{1}{c}{(12)} \\
\hline
NGC 676  &S2:    &X& --13.62 & 40.79	& 1 & $\surd$	  &	39.04	 &     38.62	 &  -	   & -  	& - \\  
NGC 1058 &S2     &C&$<$--14.42 &$<$37.55	& 2 & ? 	  &	37.90	 &     38.16	 &  4.88   &I$_{\sigma}$& 8  \\     
NGC 1068 &S1.9   &X& --11.31 & 42.84	& 1 & $\surd$	  &	41.91	 &     41.53	 &  7.20   & M  	& 1  \\     
NGC 1167 &S2     &A& --13.39 & 42.07	& 3 & $\surd$	  &	40.76	 &     40.81	 &  -	   &  - 	& -  \\  
NGC 1275 &S1.5   &X& --10.91 & 42.83		& 2 & $\times$    &	41.91	 &     42.07	 &  8.51   &I$_{\sigma}$& 2   \\ 
NGC 1667 &S2     &A&  --13.1 & 42.31	& 3 & $\surd$	  &	40.42	 &     40.17	 &  7.88   &I$_{\sigma}$& 2   \\    
NGC 2273 &S2     &A& --12.16 & 42.58	& 4 & $\surd$	  &	40.94	 &     40.92	 &  7.30   &I$_{\sigma}$& 2  \\  
NGC 2639 &S1.9   &A& --12.49 & 40.82		& 5 & ? 	  &	40.40	 &     40.56	 &  8.02   &I$_{\sigma}$& 9  \\       
NGC 2655 &S2     &A& --10.98 & 41.85		& 5 & $\times$    &	39.92	 &     40.03	 &  7.77   &I$_{\sigma}$& 9  \\     
NGC 2683 &L2/S2  &C& --13.62 & 38.21		& 2 & ? 	  &	38.58	 &     37.69	 &  7.51   &I$_{\sigma}$& 9  \\  
NGC 2685 &S2/T2: &X&:--12.53 & 39.94		& 1 & $\times$    &	38.96	 &     39.21	 &  7.15   &I$_{\sigma}$& 9   \\ 
NGC 3031 &S1.5   &X& --10.89 & 40.25		& 1 & $\times$    &	38.56	 &     38.94	 &  7.80   & S  	& 1   \\
NGC 3079 &S2     &C& --11.69 & 42.62	& 2 & $\surd$	  &	40.07	 &     40.89	 &  7.65   &I$_{\sigma}$& 3   \\ 
NGC 3147 &S2     &C& --11.39 & 41.89		& 2 & $\times$    &	40.07	 &     40.01	 &  8.79   &I$_{\sigma}$& 3  \\  
NGC 3185 &S2:    &X&  --13.7 & 40.79	& 1 & $\surd$	  &	39.90	 &     40.07	 &  6.06   &I$_{\sigma}$& 2   \\ 
NGC 3227 &S1.5   &X& --10.94 & 41.74		& 1 & $\times$    &	40.51	 &     40.20	 &  7.59   & R  	& 4  \\   
NGC 3486 &S2     &X& --12.93 & 38.86		& 1 & ? 	  &	37.99	 &     37.85	 &  6.14   &I$_{\sigma}$& 8  \\ 
NGC 3489 &T2/S2  &C&$<$--13.57 & $<$39.88	& 2 & $\surd$	  &	38.86	 &     38.48	 &  7.48   &I$_{\sigma}$& 5   \\
NGC 3516 &S1.2   &C& --10.87 & 42.29		& 2 & $\times$    &	40.50	 &     39.91	 &  7.36   & R  	& 1    \\
NGC 3608 &L2/S2  &C& --13.69 & 39.10		& 2 & $\times$    &	38.22	 &     38.23	 &  8.04   & S  	& 1   \\
NGC 3627 &T2/S2  &C&$<$--13.81 &$<$37.88	& 2 & ? 	  &	38.79	 &     39.35	 &  7.99   &I$_{\sigma}$& 5   \\ 
NGC 3941 &S2:    &X& --13.35 & 38.88		& 1 & $\times$    &	38.63	 &     38.78	 &  8.15   &I$_{\sigma}$& 7   \\
NGC 3982 &S1.9   &A& --13.28 & 41.18	& 2 & $\surd$	  &	40.50	 &     39.87	 &  6.09   &I$_{\sigma}$& 2  \\  
NGC 4051 &S1.2   &C&  --11.2 & 41.31		& 2 & $\times$    &	39.81	 &     39.68	 &  6.11   & R  	& 4  \\ 
NGC 4138 &S1.9   &X& --11.04 & 41.29		& 1 & $\times$    &	 38.74   &     38.69	 &  7.75   &I$_{\sigma}$& 9  \\ 
NGC 4151 &S1.5   &X&  --10.2 & 42.47		& 1 & $\times$    &	41.47	 &     40.94	 &  7.18   & R  	& 4 \\   
NGC 4168 &S1.9:  &X& --13.19 & 39.87		& 1 & $\times$    &	38.46	 &     38.93	 &  7.95   &I$_{\sigma}$& 6 \\    
NGC 4235 &S1.2   &A& --10.92 & 42.22		& 2 & $\times$    &	 40.41   &     40.97	 &  -	   &	-	& -  \\    
NGC 4258 &S1.9   &C& --10.91 & 40.86		& 2 & $\times$    &	39.07	 &     38.65	 &  7.61   & M  	& 1 \\     
NGC 4388 &S1.9   &C& --10.78 & 41.72		& 2 & $\times$    &	40.54	 &     40.26	 &  6.80   &I$_{\sigma}$& 3   \\  
NGC 4395 &S1     &X& --11.07 & 39.81		& 1 & $\times$    &	38.28	 &     38.53	 &  5.04  & S	       & 1   \\  
NGC 4472 &S2::   &C&$<$--13.18 &$<$39.32	& 2 & $\times$    & $<$37.81	 & $<$37.59	 &  8.80   &I$_{\sigma}$& 6   \\
NGC 4477 &S2     &X& --12.85 & 39.65		& 1 & $\times$    &	39.04	 &     39.06	 &  7.92   &I$_{\sigma}$& 9  \\
NGC 4501 &S1.9   &X& --12.91 & 39.59		& 1 & $\times$    &	39.23	 &     39.06	 &  7.90   &I$_{\sigma}$& 3  \\ 
NGC 4565 &S1.9   &X&  --12.6 & 39.43		& 1 & $\times$    &	38.69	 &     38.72	 &  7.70   &I$_{\sigma}$& 3  \\ 
NGC 4579 &S1     &C& --11.47 & 41.03		& 6 & $\times$    &	39.42	 &     39.72	 &  7.78   &I$_{\sigma}$& 3  \\  
NGC 4639 &S1.0   &X& --12.55 & 40.22		& 1 & $\times$    &	38.71	 &     39.90	 &  6.85   &I$_{\sigma}$& 8 \\  
NGC 4698 &S2     &X& --13.34 & 39.16		& 1 & $\times$    &	38.86	 &     38.74	 &  7.84   &I$_{\sigma}$& 9 \\  
NGC 4725 &S2:    &X&  --13.4 & 38.89		& 1 & $\times$    &	38.58	 &     38.24	 &  7.49   &I$_{\sigma}$& 3 \\   
NGC 5033 &S1.5   &X& --11.52 & 41.08		& 1 & $\times$    &	39.72	 &     40.42	 &  7.30   &I$_{\sigma}$& 3 \\  	      
NGC 5194 &S2     &C& --12.77 & 40.91	& 2 & $\surd$	  &	39.90	 &     39.87	 &  6.95   &I$_{\sigma}$& 2	  \\	
NGC 5273 &S1.5   &X& --11.13 & 41.36		& 1 & $\times$    &	39.03	 &     38.48	 &  6.51   &I$_{\sigma}$& 2	 \\  
NGC 5548 &S1.5   &X&  --10.5 & 43.25		& 2 & $\times$    &	41.16	 &     40.26	 &  8.03   &I$_{\sigma}$& 4   \\									      
NGC 6482 &T2/S2  &C& --13.33 & 40.16		& 2 & $\times$    &	-	 &     39.26	 &  8.75   &I$_{\sigma}$& 9\\	
NGC 6503 &T2/S2  &C& --14.39 & 37.10		& 2 & ? 	  &	-	 &     37.41	 &  5.56   &I$_{\sigma}$& 8\\	
NGC 7479 &S1.9   &X& --11.95 & 41.12		& 2 & ? 	  &	40.25	 &     40.67	 &  7.07   &I$_{\sigma}$& 9\\	
NGC 7743 &S2     &A& --13.14 & 41.47	& 5 & $\surd$	  &	40.21	 &     40.24	 &  6.59   &I$_{\sigma}$& 2 \\  	   
\hline						     
\end{tabular}												\\[1.5mm]					    				    	 				    
\scriptsize{Notes: Col. (1): galaxy name; Col. (2): optical classification;	    	 			     
Col. (3): Satellite used: "C''=Chandra, "X''=XMM-Newton,		    				    	 			    
"A''=ASCA; Col. (4): logarithm of the 2--10 keV flux in units of erg~cm$^{-2}$~s$^{-1}$, 
not corrected for Compton thick candidates. 
Col. (5): logarithm of the 2--10 keV luminosity, corrected for Compton thick
candidates. Col. (6):
X-RAY REFERENCES: (1) Cappi et~al. (\cite{cappi2006}); (2) this work; (3) Pappa et~al. (\cite{pappa2001}); 
(4) Guainazzi et~al. (\cite{guainazzi2005}); (5) Terashima et~al. (\cite{terashima2002}); (6) Eracleous et~al. (\cite{eracleous2002}); 
Col. (7):  Final classification: "$\surd$''=Compton thick candidates, "$\times$''=Compton thin candidate
and "?''=doubtful objects.; Col. (8): logarithm of the \oiii luminosity corrected for Galactic absorption
and NLR extinction; Col. (9): logarithm of the H${\alpha}$ (broad+narrow component) 
luminosity corrected for Galactic absorption
and NLR extinction; Col. (10): logarithm of the $M_{\rm BH}$ value in units of $M_{\odot}$; Col. (11):
$M_{\rm BH}$ measurement methods; M: maser kinematics;
G: gas kinematics; S: stellar kinematics; R: reverberation mapping; I$_{\sigma}$: 
inferred from the mass-velocity dispersion correlation; Col. (12): $M_{\rm BH}$ references:  
(1) Ho (\cite{ho2002}); (2) Woo \& Urry (\cite{woo2002}); (3) Merloni et~al. (\cite{merloni2003}); (4) Kaspi et~al. (\cite{kaspi2000});
(5) Pellegrini (\cite{pellegrini2005}); (6) Merritt \& Ferrarese (\cite{merritt2001}); (7) di Nella et~al. (\cite{diNella1995});
(8) Barth et~al. (\cite{barth2002}); (9) McElroy (\cite{mcElroy1995}).}
}			    	 		 \end{table}