\begin{table}%t11
\caption{\label{tab:flux}Fluxes and absorption-corrected luminosities calculated assuming the best fit
model. The last two columns list the ratio between the strength of the soft
excess  and the high energy power law component in the 0.5--2 and
0.5--10 keV band, respectively. }
%\centering
\par
\begin{tabular}{c c c c c c c }
\hline \hline 
   PG Name    &   
$F_{\rm 0.5-2\;keV}$   &    $F_{\rm 2-10\;keV}$   & $ L_{\rm 0.5-2\;keV}$   & 
  $L_{\rm 2-10\;keV}$  & $R^{\rm 0.5-2}_{\rm S/P}$ &  $R^{\rm 0.5-10}_{\rm S/P}$ \\ 
  &  (10$^{-12}$ erg cm$^{2}$ s$^{-1}$) & (10$^{-12}$ erg cm$^{2}$ s$^{-1}$)  & (10$^{44}$ erg s$^{-1}$)  & (10$^{44}$ erg s$^{-1}$)  &   &  \\ \hline  
0007$+$106	 & 3.7     & 7.2     & 0.87     & 1.4 &            0.160 &          0.072\\    
0050$+$124 	 &  9.15  &  8.44  &  1.39  &  0.78 &  		  0.360 &          0.212\\
0157$+$001 	 &  1.33  &  0.93  &  1.05  &  0.71 & 		  0.169	 &        0.126\\
0804$+$761 	 & 11.6     & 11.12  & 3.43     & 2.86 &     	  0.489	  &      0.238\\
0844$+$349 	 &      6.9  & 5.5  &  0.81  &  0.55 &  		  0.954	  &      0.444\\
0947$+$396 	 &  1.79  &  1.87  &  2.55  &  2.26  & 		  0.814	   &     0.336\\
0953$+$414 	 & 3.79 & 3.21 & 7.77 & 5.41		 & 	  0.836	 &       0.379\\
1001$+$054 	 & 0.03     & 0.12     & 0.10     &  0.13   &  	  $-$     &        $-$    \\
1048$+$342 	 & 1.24 & 1.46 & 1.07 & 1.10			 &   0.712 & 	       0.277\\
1100$+$772 	 & 2.48     & 3.83     & 8.97     & 11.19    &  	  0.650     &     0.318\\
1114$+$445 	 & 0.62 & 2.3     & 2.65     & 1.45    	 &   1.75         & 0.724\\
1115$+$080 	 &  0.23   &  0.36  &  42.1  &  65.3 &  		  $-$   &          $-$\\    
1115$+$407 	 & 2.13     & 1.27     & 1.67 & 0.85  &     	  0.787	 &       0.427\\
1116$+$215 	 &  5.2  &  3.3  &  5.0  &  3.1  	 & 	  0.473	 &       0.258\\
1202$+$281	 &  2.68  &  3.72  &  2.22  &  2.68 &  	 	  0.646	 &       0.226\\
1206$+$459       & 0.14 &  0.24  &  8.55  &  14.9 	 & 	  $-$     &        $-$    \\
1211$+$143 	 &  3.0  &  3.1  &  0.61  & 0.50 		 &   1.825 & 	       0.572\\
1216$+$069 	 & 1.08     & 1.38     & 4.69     & 4.8 	  &  0.948 & 	       0.351\\
1226$+$023	 & 43.81     & 78.74     & 31.75     & 51.05      &  0.310  &        0.103\\
1244$+$026 	 &  5.87  &  2.53  &  0.36  &  0.14  &  		  0.470   &       0.297\\
1307$+$085	 &  0.94  &  2.01  &  0.63  & 1.19  	 & 	  0.443	 &       0.118\\
1309$+$355 	 & 0.45     & 0.73     & 0.46     & 0.67  &    	  0.175	 &      0.077\\
1322$+$659 	 & 2.25 & 1.33 & 2.21 & 1.08			 &   0.650 & 	       0.367\\
1352$+$183 	 &  2.30  &  2.00  &  1.85  &  1.36 &  		  1.121	 &       0.464\\
1402$+$261 	 &  3.0  &  1.9  &  2.7  &  1.4 & 		  0.851	 &       0.427\\
1404$+$226 	 & 0.51     & 0.10     & 2.31     & 2.87 &     	  0.423	 &       0.246\\
1407$+$265 	 & 0.94     & 0.80     & 53.31     & 41.20 &        0.105	 &       0.058\\
1411$+$442 	 & 0.09  & 0.46     & 0.35     & 0.25 &     	  0.061   &      0.062\\
1415$+$451 	 &  1.4  &  1.1  &  0.5  &  0.4 &  		  0.696	 &       0.331\\
1427$+$480 	 &  1.2 	 &  1.1  &  2.0  &  1.6 &  		  0.634	 &       0.284\\
1440$+$356 	 &  5.9  &  3.9  &  1.0  &  0.58  &  		  2.432	 &       1.076\\
1444$+$407 	 &  0.9  &  0.6  &  2.6  &  1.3  & 		  3.009	 &       1.420 \\
1501$+$106	 & 17.2  & 16.2     &  0.57     &  0.49 &      	  0.761	 &       0.311\\
1512$+$370	 & 1.56  & 1.97     & 8.51     & 8.84 &      	  2.050   &       0.859\\
1613$+$658	 & 2.77     & 4.15     & 1.40  & 1.78 &      	  0.327	 &       0.121\\
1626$+$554 	 & 3.04     & 3.08     & 1.57     & 1.46 &     	  0.708	 &       0.354\\
1630$+$377 	 & 0.14 & 0.15 & 31.1 & 20.9 & 			  1.570   &       0.774\\
1634$+$706 	 & 	 1.0  & 1.16  &  141.6  &  127.9 &  	  0.591   &       0.335\\
2214$+$139 	 & 0.31     & 3.26     & 0.39 & 0.48   &    	  0.168	 &       0.111\\
2302$+$029 	 &  0.24  &  0.27  &  25.9  &  16.2  &    	  0.649  &       0.336\\
\hline
\end{tabular} 
\end{table}