\begin{table}%t8
%\centering
\par
\caption{Fit results, in the 2--12~keV energy band, of a 
 disk reflection model assuming a {\sc lamppost} geometry for I~Zw1, 
PG~0804+761, PG~1114+445, PG~1116+215 and PG~1309+355, 
i.e. we assume a height of 10~$R_{\rm g}$, a ratio of X-ray to disk flux of 0.2 
 (with solar iron abundance).
For PG~1402+261, a lower height above the AD of about 2.5~$R_{\rm g}$, 
an iron abundance of 5 relative to solar abundance are required. 
Its spectrum is dominated by reflection. \label{tab:lamppost}
}
\begin{tabular}{ccccc}
\hline
\hline
\noalign {\smallskip}  
Object &  $\Gamma$  & $\theta$ (deg) & $r_{\rm in}$ ($r_{\rm g}$) & $\chi^{2}$/d.o.f. \\  
\noalign {\smallskip}  
\hline
\noalign {\smallskip}  
 I~Zw1      &  2.28~$\pm$~0.03    & $\rm 42^{+23}_{-19}$ & $\rm 16^{+17}_{-10}$& 598.7/590 \\
\noalign {\smallskip}  
PG~0804+761 & 2.07~$\pm$~0.06     & 42~$\pm$~21  &$<$14  & 212.2/250\\
\noalign {\smallskip}  
PG~1116+215 & 2.12~$\pm$~0.09 & 30~$\pm$~22 & $<$13 & 124.6/104 \\ 
\noalign {\smallskip}  
PG~1309+355 & 1.74~$\pm$~0.09 & $<$27 &$<$30 & 62.9/86 \\
\noalign {\smallskip}  
PG~1402+261 & 2.13~$\pm$~0.10 & $>$60 & $<$5 & 85.9/92\\
\noalign {\smallskip}  
\hline
\end{tabular}
\end{table}