\begin{table}%t1
%\centering
\par
\caption{\label{t1}Spectral fitting results for Cygnus~X-2: 90\% confidence errors are shown.}
\begin{tabular}{lrrrrlrrr}
\hline \hline
\noalign{\smallskip}
$\;\;$spectrum&$N_{\rm H}$&$kT$&$norm_{\rm BB}$&$R_{\rm BB}$&$E_{\rm
CO}$&$norm_{\rm CPL}$&$\chi^2$/d.o.f.\\
&&(keV)&&(km)&(keV)\\
\hline
Horizontal Branch\\
1&$1.5\pm 0.6$  &$2.31\pm 0.20$  &$1.96\pm 0.33$ &$2.1\pm 0.4$  &$7.29\pm 0.69$  &$3.93\pm 0.41$  &66.7/69\\
2&$2.0\pm 0.5$  &$2.37\pm 0.16$  &$1.74\pm 0.24$  &$1.9\pm 0.3$  &$7.00\pm 0.45$  &$4.50\pm 0.34$  &77.6/68\\
3&$2.2\pm 0.5$  &$2.20\pm 0.14$  &$1.67\pm 0.20$ &$2.1\pm 0.3$  &$6.90\pm 0.27$  &$5.16\pm 0.33$  &64.3/68\\
4&$2.3\pm 0.5$  &$2.20\pm 0.15$  &$1.76\pm 0.20$ &$2.2\pm 0.3$  &$6.70\pm 0.30$  &$5.52\pm 0.39$  &82.8/68\\
5&$2.6\pm 0.5$  &$1.99\pm 0.16$  &$1.51\pm 0.30$ &$2.4\pm 0.5$  &$6.68\pm 0.24$  &$6.15\pm 0.45$  &73.4/65\\
%\noalign{\smallskip}
Hard Apex\\
6&$2.7\pm 0.5$  &$1.92\pm 0.15$  &$1.60\pm 0.35$ &$2.7\pm 0.5$   &$6.43\pm 0.22$  &$6.71\pm 0.50$  &52.6/55\\
%\noalign{\smalls kip}
Normal Branch \\
7&$2.6\pm 0.5$  &$1.65\pm 0.12$  &$1.43\pm 0.50$ &$3.5\pm 0.7$   &$5.95\pm 0.16$  &$7.28\pm 0.60$  &78.4/68\\
8&$2.4\pm 0.5$  &$1.46\pm 0.08$  &$1.56\pm 0.60$ &$4.7\pm 1.0$   &$5.68\pm 0.18$  &$7.23\pm 0.72$  &56.8/58\\
%%%%9(Hexte bad)&1.7$\pm 0.6$  &1.26$\pm 0.04$  &2.86$\pm 0.70$ &8.4$\pm 1.2$   &5.71$\pm 0.26$  &6.00$\pm 0.75$  &11\
%0.0/70 \\
9   &$1.9\pm 0.6$  &$1.26\pm 0.05$  &$2.54\pm 0.75$ &$7.9\pm 1.3$   &$5.59\pm 0.26$   &$6.35\pm 0.85$ &60.3/51 \\
10&$1.6\pm 0.6$    &$1.20\pm 0.04$  &$2.93\pm 0.75$ &$9.5\pm 1.3$   &$5.45\pm 0.30$   &$6.1\pm 0.9$  &74.1/70\\
%\noalign{\smallskip }
Soft Apex \\
11&$0.9\pm 0.6$    &$1.19\pm 0.03$  &$4.55\pm 0.70$ &$12.0\pm 1.1$  &$5.41\pm 0.30$  &$4.97\pm 0.85$  &53.6/63\\
%\noalign{\smallskip }
Flaring Branch\\
12&$0.9\pm 0.9$    &$1.22\pm 0.04$  &$4.80\pm 1.30$ &$11.9\pm 1.0$  &$5.53\pm 0.60$  &$5.05\pm 1.50$  &47.9/47 \\
13&$0.9\pm 0.9$    &$1.31\pm 0.03$  &$5.46\pm 0.6$  &$10.9\pm 0.8$  &$5.72\pm 0.26$  &$4.87\pm 0.50$  &58.5/56\\
\hline
\end{tabular}
\tablefoot{Column densities are in units of 10$^{22}$~atom~cm$^{-2}$; the normalization of the blackbody is in units of $\rm {10^{37}}$~erg~s$^{-1}$ for a distance of 10~kpc, the cut-off power law normalization is in units of photon~cm$^{-2}$~s$^{-1}$~keV$^{-1}$ at 1~keV.}
%\vspace*{3mm}
\end{table}