\begin{table}%t5
%\centering
\par
\caption{\label{TFITL} Spectral fits of the emission line of PG~1535+547.
The corresponding continuum fits are provided in Table \ref{TFITS}.
Fits labeled with $\dagger$ were performed over the 2--10 keV energy range for MOS and the
2--12~keV energy range of pn, respectively.
(1)~The following two models are used:
$ga$: Gaussian line at  redshift of source (XSPEC: zgauss),
$la$: relativistic disk line after Laor (XSPEC: laor, \cite{Laor1991});
Parameters: 
 (a)~energy of line in rest frame of quasar; 
 (b) line width~($\sigma$);
 (c) total photons in line; 
 (d) inclination angle  
}
\begin{tabular}{llcccrrc}
\hline \hline 
Fit & Emission   &  Energy$^{(a)}$   & Width$^{(b)}$ & Norm$^{(c)}$ & $R$(in) & $R$(out) & Inclination$^{(d)}$ \\ 
    & line model &  [$\rm keV$]  & [$\rm keV$] & [$\rm cm^{-2}\;s^{-1}$]  & [$\rm G\;M\;c^{-2}$]      &   [$\rm G\;M\;c^{-2}$]     & [$\rm degree$]    \\  
\hline 
11   & la            & 6.4 (fixed)          &       &  $\rm 5.38_{-0.68}^{+0.49} \;10^{-5}$     & 
                      $\rm 1.77_{-0.77}^{+0.22}$  & $\rm 7.83_{-0.66}^{+1.40}$ 
                    & $\rm 31.85_{-1.45}^{+2.40}$ \\
12   & ga            &  $\rm 6.00_{-0.21}^{+0.14}$  & $\rm 0.26_{-0.11}^{+0.21}$ & $\rm 7.16_{-2.70}^{+2.69} \;10^{-6}$ 
                    &       &     \\
13$^\dagger$  & ga     &  $\rm 6.06_{-0.14}^{+0.14}$  & $\rm 0.19_{-0.08}^{+0.14}$ & $\rm 5.22_{-2.71}^{+3.16} \;10^{-6}$ 
                  &       &     \\
14   & la       & 6.4 (fixed)          &       & $\rm 1.63_{-0.42}^{+0.42} \;10^{-5}$     & 
                      $\rm 5.67_{-1.32}^{+2.16}$  & $\rm 9.47_{-2.08}^{+1.59}$ 
                    & $\rm 28.38_{-2.28}^{+4.36}$ \\
15$^\dagger$  & la       & 6.4 (fixed)          &       & $\rm 1.28_{-0.44}^{+0.49} \;10^{-5}$     & 
                      $\rm 7.00_{-2.57}^{+0.96}$  & $\rm 8.16_{-0.75}^{+3.06}$ 
                    & $\rm 28.63_{-2.18}^{+4.43}$ \\
\hline 
\end{tabular}
\end{table}