\begin{table}%t3
\par
\caption{\label{tab:para}{Best-fit spectral parameters over all our {\emph {INTEGRAL}} observations.}}
%\centerline
{
\small\begin{tabular}{ccccccccc}
\hline \hline
Time    & Observations & Disc Norm.$^a$       & $kT_{\rm in}$ & $\Gamma$ & $E_{\rm Fe}$ line    & \kir             & $F_{\rm total}^b$                      & $F_{\rm bolometric}^c$\\
(MJD)   &              &                      & (keV)         &          & (keV)                & (d.o.f.)            & (10$^{-10}$~erg~cm$^{-2}$~s$^{-1}$) & (10$^{-8}$~erg~cm$^{-2}$~s$^{-1}$)\\
\hline
53599.8 & Rev. 347     & $\rm 1320_{-112}^{+90}$  & 0.640$\pm$0.008      & $\rm 2.44_{-0.07}^{+0.08}$ & 
$\rm 6.0^{+0.05}$ & 1.39~(57) &~81 $\pm$ 3 & 5.96\\
53602.5 & Rev. 348     & $\rm 1990_{-107}^{+21}$   & 0.59$\pm$0.01         & $\rm 2.21_{-0.04}^{+0.04}$ & $\rm 6.0^{+0.06}$ & ~~1.49~(136) & ~63 $\pm$ 1 & 4.19\\
53605.5 & Rev. 349     & $\rm 1160_{-34}^{+110}$   & 0.624$\pm$0.008      & $\rm 2.34_{-0.08}^{+0.05}$ & $\rm 6.0^{+0.04}$ & 1.69~(57)    & ~59 $\pm$ 2 & 3.92\\
53607.8 & Rev. 350     & $\rm 1090_{-85}^{+100}$   & 0.614$\pm$0.007      & $\rm 2.37_{-0.06}^{+0.07}$ & $\rm 6.0^{+0.04}$ & 1.10~(48)    &~52 $\pm$ 2 & 3.08\\
53611.1 & Rev. 351     & $\rm 1730_{-130}^{+140}$ & 0.55$\pm$0.007          & $\rm 2.32_{-0.10}^{+0.09}$ & $\rm 6.0^{+0.05}$ & 1.51~(48)    & ~39 $\pm$ 1 & 2.20 \\
53618.5 & Rev. 353     & $\rm 2260_{-170}^{+230}$ & 0.51$\pm$0.01          & $\rm 2.30_{-0.21}^{+0.29}$ & $\rm 6.0^{+0.07}$ & 0.73~(41)    &~27 $\pm$ 2 & 2.40\\
53619.8 & Rev. 354    & $\rm 2270_{-180}^{+230}$  & 0.502$\pm$0.006      & $\rm 2.82_{-0.32}^{+0.58}$ & $\rm 6.0^{+0.18}$ & 1.08~(41)    &~25 $\pm$ 1 & 2.33\\
53621.7 & First min.$^d$   & $\rm 2160_{-140}^{+290}$  & 0.50$\pm$0.01          & $\rm 2.45_{-0.28}^{+0.45}$ & $\rm 6.0^{+0.07}$ & 1.41~(41)    & 23.3 $\pm$ 0.5 & 2.20\\
53631.2 & Second. max$^d$. & $\rm 2440_{-206}^{+170}$ & ~0.511$\pm$0.005    & $\rm 2.30_{-0.78}^{+0.70}$ & $\rm 6.0^{+0.14}$ & 1.08~(42)    & 28.0 $\pm$ 0.5 & 2.29\\
53699.8 & Last obs.$^d$    & $<$ 20 000            & 0.27$\pm$0.06             & $\rm 2.28_{-0.24}^{+0.28}$ & ---           & 1.11~(40)    & ~1.5 $\pm$ 0.1 & 0.92\\
\hline
\end{tabular}}
\medskip
\par
Notes:\\
Model applied in {\tt XSPEC} notations: {\sc constant}*{\sc
wabs}*({\sc ezdiskbb}+{\sc gaussian}+{\sc powerlaw}) with $N_{\rm H}$ fixed to
5.4~$\times$~10$^{21}$ cm$^{-2}$. Errors are given at the 90\% confidence level
($\Delta \chi^2=2.7$).\\
$^a$ Disc normalization $K$ is proportional to $(R/D)^{2}\cos\theta$, where $R$ is the
inner disc radius in km, $D$ is the distance to the source in kpc and $\theta$
the inclination angle of the disc.\\
$^b$ Computed in the 2--20~keV range.\\
$^c$ Extrapolated in the 0.001~keV--10~MeV range.\\
$^d$ Based on the \rxte/PCA light curve.\\
\end{table}