\begin{table}%t4
%\centering
\par
\caption{Spectral fits with an absorbed power law continuum in two energy bands
 (2--5~keV and 0.3--2~keV). 
Galactic absorption ($N_{\rm H}^{\rm Gal}$) 
 and intrinsic absorption ($N^{\rm in}_{\rm H}$) of the QSO in its rest frame
 are expressed in 10$^{20}$~cm$^{-1}$.
 ($^a$) absorption edge(s) added to the continuum model 
(see parameter values in Table~\ref{tab:WA}).
\label{table:fits}}
\begin{tabular}{l|c|ccc|cccc}
\hline
\hline
%                   &            &  \multicolumn{3}{c}{2 -- 5 keV}   &  \multicolumn{4}{c}{0.3 -- 2 keV} \\
Source        &   $N_{\rm H}^{\rm Gal}$& $\Gamma_{2-5}$ & $\chi^{2}$/d.o.f.  & P($\chi^{2}$)&  $N^{\rm in}_{\rm H}$&  $\Gamma_{0.3-2}$    & $\chi^{2}$/d.o.f.&  P($\chi^{2}$) \\
\hline
I~Zw1& 4.94 & 2.30~$\pm$~0.05 & 167.4/132 & 2.0 &$^{(a)}$7.8~$\pm$~1.0 & 2.63~$\pm$~0.06 & 352.8/324& 13.0\\ 
%\noalign {\smallskip}           
PG~0804+761 & 3.01   &2.19~$\pm$~0.09   &161.5/196 & 96.6&  $^{(a)}$2.3~$\pm$~1.1  & 2.51~$\pm$~0.08 & 248.6/220   & 9.0 \\  
%\noalign {\smallskip}                       
PG~0947+396  & 1.55 &1.81~$\pm$~0.12 & 128.3/122 & 33.1  &$^{(a)}$2.1~$\pm$~1.4& 2.52~$\pm$~0.09&  285.1/312 & 86.0\\ 
%\noalign {\smallskip}                       
PG~0953+414  & 0.82 & 2.04~$\pm$~0.11 & 55.7/75 & 95.2 & $<$0.4 & 2.59~$\pm$~0.03 & 337.0/278 & 0.9 \\ 
%\noalign {\smallskip}    
PG~1048+342  &  1.94   & 1.83~$\pm$~0.12 & 85.8/81 & 33.7  & $<$0.8 & $\rm 2.40^{+0.06}_{-0.02}$  & 239.3/267 & 8.5 \\
%\noalign {\smallskip}                       
PG~1114+445 & 1.62 &  1.38~$\pm$~0.08 &  123.3/131& 67.2 & $^{(a)}$$<$2.0  & $\rm 1.56^{+0.12}_{-0.03}$  &  267.9/213   & 0.6 \\
%\noalign {\smallskip}                       
PG~1115+407 &  1.91  &2.27~$\pm$~0.15 & 58.9/81 &96.9&$^{(a)}$$\rm 2.1^{+1.7}_{-1.3}$ & 2.92~$\pm$~0.09 & 268.0/300  & 90.8 \\ 
%\noalign {\smallskip}                       
PG~1116+215  &  1.29 & 2.26~$\pm$~0.16 & 98.6/80  & 7.8  & $<$0.5  & 2.71~$\pm$~0.04 & 263.6/294 &89.8   \\
%\noalign {\smallskip}                       
PG~1202+281 & 1.70 & 1.65~$\pm$~0.11 & 68.9/78 & 76.0 & $^{(a)}$$<$0.3 & 2.28~$\pm$~0.03 & 309.9/264 & 2.7\\
%\noalign {\smallskip}                       
PG~1244+026  &   1.78  & 2.52~$\pm$~0.18 & 96.5/79 & 8.8&11.5~$\pm$~0.1  & 3.72~$\pm$~0.09  & 407.6/296 & 0 \\
%\noalign {\smallskip}                       
PG~1307+085  &  2.10   &  1.40~$\pm$~0.16 & 74.5/81 & 68.3 & $^{(a)}$$<$0.3 & 2.22~$\pm$~0.05 & 268.8/219  & 1.2 \\
%\noalign {\smallskip}                       
PG~1309+355&1.02 & 1.76~$\pm$~0.18& 51.8/62&81.8&$^{(a)}$$<$0.5 & 2.26~$\pm$~0.05 & 197.8/212  & 75.0 \\
%\noalign {\smallskip}                      
PG~1322+659  &  2.00  & 2.23~$\pm$~0.20 &52.8/57 &63.2  &  $<$0.7 &   $\rm 2.99^{+0.05}_{-0.03}$ &275.6/257 & 20.3    \\
%\noalign {\smallskip}                       
PG~1352+183  & 2.05   & 1.95~$\pm$~0.15 & 126.2/107 & 9.9 &   $^{(a)}$$<$2.3  &  $\rm 2.69^{+0.10}_{-0.08}$& 311.9/299  & 29.2    \\
%\noalign {\smallskip}                       
PG~1402+261  & 1.47  &  2.31~$\pm$~0.16    & 75.5/73 &39.8  & $<$1.5 & $\rm 2.83^{+0.10}_{-0.03}$  &319.4/288 & 9.8  \\
%\noalign {\smallskip}   
Mrk~1383 & 2.85 & 1.95~$\pm$~0.13 & 92.9/110 & 87.9 & $<$0.8 & $\rm 2.62^{+0.06}_{-0.02}$  & 321.2/313 & 36.2 \\      
%\noalign {\smallskip}                       
PG~1427+480  &  1.86  & 1.90~$\pm$~0.12 & 104.3/123 & 90.0 &  $<$1.4   & $\rm 2.52^{+0.08}_{-0.03}$ & 344.1/311   & 9.5  \\
%\noalign {\smallskip}                       
Mrk~478 & 1.04 & 2.45~$\pm$~0.13   & 90.9/115 & 95.2& 0.9~$\pm$~0.8  & $\rm 3.12^{+0.07}_{-0.06}$& 322.7/319  & 43.2 \\ 
%\noalign {\smallskip}  
PG~1512+370   &  1.35  & 1.72~$\pm$~0.13  & 125.0/124 &45.8& $<$0.8 & 2.31~$\pm$~0.04 & 301.4/305  & 54.7 \\
%\noalign {\smallskip} 
Mrk~876     &  2.85  & 1.92~$\pm$~0.20 & 47.2/61 & 90.2 & $^{(a)}$$<$2.3 & $\rm 2.45^{+0.15}_{-0.04}$ & 254.2/230  & 13.1 \\
%\noalign {\smallskip} 
PG~1626+554   &   2.02 &  2.03~$\pm$~0.21  &  61.2/82 & 95.8 &  $<$0.7 & $\rm 2.00^{+0.19}_{-0.13}$ &  96.9/122  & 95.4    \\
\hline
\end{tabular}
\end{table}