\begin{table}%t10
\par
%\centering
\par
\caption{Spectral fit with absorbed compTT+power law. For the {\sc comp}TT component model, 
the soft photon temperature (${\it kT}^{\rm photon}_{1}$) is fixed to  $T$max (Col.~1 of Table~\ref{table:fitbb}). 
 ${\it kT}^{\rm plasma}$ is expressed in keV. 
$\tau$ corresponds to the plasma optical depth. 
The fits include the Galactic ($N^{\rm Gal}_{\rm H}$) and intrinsic ($N^{\rm in}_{\rm H}$) absorptions. 
Column densities are expressed in 10$^{20}$~cm$^{-1}$. 
The unabsorbed fluxes are expressed in 10$^{-12}$~erg~s$^{-1}$~cm$^{-2}$.
 In parentheses are reported the luminosities (expressed in 10$^{44}$~erg~s$^{-1}$). 
 The last column reports the flux ratio in the 0.3--2~keV and 0.3--10~keV energy bands. 
 ($^a$) one or two absorption edges are  added to the continuum model due to the presence of a WA.
($^b$) a Fe~K line is added (either a Gaussian line or a {\sc laor} line).
 \label{table:fitcomptt}}
\begin{tabular}{lcccccccc}
\hline\hline
\multicolumn{1}{c}{Source} &    $N^{\rm in}_{\rm H}$  &   $kT^{\rm plasma}$    &  $\tau_{1}$    &  $\Gamma$   &   $\chi^{2}$/d.o.f.   &   $F_{0.3-10}$ (L)   &   $F_{2-10}$ (L) & $\frac{\rm 0.3-2~\rm keV}{0.3-10~\rm keV}$ \\
\noalign {\smallskip}  
\hline
\noalign {\smallskip}            
  I~Zw1$^{(a,b)}$ &  10.5~$\pm$~2.6 & 0.22~$\pm$~0.05 & $\rm 14.7^{+2.2}_{-1.3}$ & 2.33~$\pm$~0.03 & 525.7/490 & 36.3 (2.8) & 8.6 (0.64) & 76$\%$\\
%\noalign {\smallskip}                       
PG~0804+761$^{(a,b)}$&  $\rm 3.9^{+7.2}_{-3.1}$& $\rm 2.8^{+3.1}_{-1.4}$& $\rm 3.5^{+2.1}_{-1.1}$ & $\rm 1.53^{+0.32}_{-0.17}$& 462.5/470 & 30.5 (6.1) & 11.4 (2.3) &63$\%$\\
%\noalign {\smallskip}                       
PG~0947+396$^{(a,b)}$& $<$3.3 & 0.32~$\pm$~0.06& $\rm 15.6^{+0.8}_{-2.0}$ & 1.76~$\pm$~0.07  &  440.1/479   & 4.6 (4.2)  & 1.8 (1.6) &61$\%$ \\ 
%\noalign {\smallskip}                       
PG~0953+414  & $<$2.0 &  $\rm 0.29^{+0.10}_{-0.06}$ & $\rm 13.8^{+0.5}_{-1.0}$ & 1.98~$\pm$~0.05  & 408.6/379  & 9.1 (11.9) & 3.0 (3.7) & 67$\%$  \\ 
%\noalign {\smallskip}                       
PG~1048+342$^{(b)}$  &  $<$1.8 & $\rm 0.25^{+0.09}_{-0.06}$ &  $\rm 16.6^{+0.8}_{-1.5}$& 1.82~$\pm$~0.06  & 417.4/383  & 3.2 (1.9) & 1.3 (0.74) & 60$\%$  \\
%\noalign {\smallskip}                       
PG~1114+445$^{(a,b)}$ &$\rm 5.2^{+2.5}_{-3.5}$ & $\rm 3.1^{+9.7}_{-2.2}$   &  $\rm 6.7^{+3.2}_{-4.0}$ & 1.51 (f)  & 214.6/236 & 3.3 (1.3) & 2.3 (0.92) & 30$\%$\\
%\noalign {\smallskip}                       
PG~1115+407$^{(a,b)}$ & $<$7.2 &  $\rm 0.17^{+0.08}_{-0.04}$  & $\rm 19.2^{+5.4}_{-3.4}$ & 2.40~$\pm$~0.06 &333.2/399 & 5.8 (3.1) & 1.2 (0.60) & 79$\%$ \\ 
%\noalign {\smallskip}                       
PG~1116+215$^{(a,b)}$ & $<$11.8 & $\rm 0.25^{+0.18}_{-0.07}$ & $\rm 13.1^{+3.7}_{-2.1}$ & 2.23~$\pm$~0.08 & 370.3/396 & 14.8 (11.0)&3.2 (2.1) & 78$\%$ \\
%\noalign {\smallskip}                       
PG~1202+281$^{(a)}$ &$<$6.7 & 0.24~$\pm$~0.07 & $\rm 21.2^{+1.8}_{-4.8}$& 1.68~$\pm$~0.04 &396.9/372 & 7.5 (4.2) & 3.6 (1.9) &52$\%$\\ 
%\noalign {\smallskip}                       
PG~1244+026$^{(b)}$ & $<$2.1 &0.18~$\pm$~0.02 & $\rm 28.7^{+2.5}_{-4.0}$&  2.40~$\pm$~0.08 &  426.8/400 & 12.4 (0.57) &  2.1 (0.098)  & 83$\%$ \\
%\noalign {\smallskip}                       
PG~1307+085$^{(a)}$ & 5.4~$\pm$~4.2& 0.10~$\pm$~0.02 & $>$44 &  1.46~$\pm$~0.03 &  350.1/337  & 3.4 (1.6) & 1.9 (0.87) & 44$\%$  \\
%\noalign {\smallskip}                       
PG~1309+355$^{(a,b)}$& $<$13.1 & $\rm 0.13^{+0.08}_{-0.03}$  & $>$23.4 & $\rm 1.78^{+0.09}_{-0.06}$ & 244.4/295 & 1.4 (1.0) & 0.72 (0.48)  & 49$\%$   \\
%\noalign {\smallskip}                       
PG~1322+659 & $<$4.3 & 0.17~$\pm$~0.05 & $\rm 22.4^{+1.7}_{-3.7}$  & 2.21~$\pm$~0.07 & 327.1/335  & 5.3 (3.4) & 1.3 (0.77) & 76$\%$      \\
%\noalign {\smallskip}                       
PG~1352+183$^{(a)}$ & $<$6.8  & 0.25~$\pm$~0.06   & $\rm 17.6^{+0.9}_{-3.0}$ & 1.90~$\pm$~0.08 & 476.0/455 & 5.7 (2.8) & 1.9 (0.88) & 67$\%$\\
%\noalign {\smallskip}                       
PG~1402+261$^{(b)}$  & $<$3.1 & $\rm 0.25^{+0.11}_{-0.06}$ & $\rm 14.2^{+0.6}_{-1.7}$ & 2.20~$\pm$~0.08 & 407.5/381 &  7.3 (4.4)   & 1.8 (1.0)  & 75$\%$  \\
%\noalign {\smallskip}                       
Mrk~1383$^{(b)}$ & $<$1.0 & 0.20~$\pm$~0.05 & $\rm 19.1^{+0.9}_{-1.2}$  & 2.02~$\pm$~0.05  & 438.8/457 & 23.2 (3.5) & 7.5 (1.1) &  68$\%$  \\
%\noalign {\smallskip}                       
PG~1427+480 & $<$4.8  & $\rm 0.27^{+0.08}_{-0.05}$ & $\rm 16.0^{+0.7}_{-2.4}$ & 1.86~$\pm$~0.05 & 494.9/487 & 2.7  (2.8)   & 1.0 (1.0)  &  63$\%$ \\ 
%\noalign {\smallskip}             
Mrk~478  &  $<$5.1 &  0.22~$\pm$~0.05 & 13.6~$\pm$~1.3  & 2.29~$\pm$~0.06  & 416.4/464 & 15.8 (2.0) & 2.7 (0.33) & 83$\%$\\
%\noalign {\smallskip}                       
PG~1512+370$^{(b)}$& $<$6.5 &  $\rm 0.44^{+0.72}_{-0.12}$ & $\rm 10.9^{+0.6}_{-2.4}$& 1.74~$\pm$~0.08 & 468.6/476 & 4.3 (13.5) &1.9 (5.4) &56$\%$ \\
%\noalign {\smallskip}                       
Mrk~876$^{(a)}$   &$<$4.0 & 0.14~$\pm$~0.06  & $>$37.4  & 1.86~$\pm$~0.06  & 327.4/320  & 11.8 (4.0)  & 5.1 (1.7)  & 57$\%$  \\
%\noalign {\smallskip}                       
PG~1626+554 &  $<$6.9 &   $\rm 0.52^{+7.84}_{-0.30}$  & $\rm 9.4^{+0.7}_{-2.2}$ & 1.85~$\pm$~0.17   &  385.9/387 & 8.0 (2.9)& 3.1 (1.1) & 61$\%$\\
\hline
\end{tabular}
\end{table}