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Table 2:

Spectral fitting results: 90% confidence errors are shown.
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    
Horizontal branch              
1 $6.1\pm 0.5$ $2.08\pm 0.10$ $7.6\pm 0.7$ $5.1\pm 0.5$ $5.9\pm 0.3$ $19.5\pm 1.4$ 32/58
2 $6.3\pm 0.5$ $1.98\pm 0.10$ $7.2\pm 0.8$ $5.4\pm 0.6$ $5.8\pm 0.2$ $21.2\pm 1.5$ 24/58
3 $6.5\pm 0.4$ $1.93\pm 0.08$ $7.4\pm 0.8$ $5.8\pm 0.5$ $5.6\pm 0.2$ $23.4\pm 1.5$ 46/58
Hard apex              
4 $6.8\pm 0.5$ $1.87\pm 0.09$ $7.2 \pm 0.1$ $6.07\pm 0.6$ $5.6\pm 0.2$ $25.3\pm 1.8$ 38/58

Normal branch
             
5 $6.6\pm 0.4$ $1.77\pm 0.07$ $6.6\pm 1.1$ $6.5\pm 0.5$ $5.4\pm 0.1$ $25.5\pm 1.7$ 37/58
6 $6.5\pm 0.5$ $ 1.70\pm 0.10$ $5.6\pm 0.6$ $6.5\pm 0.8$ $5.1\pm 0.1$ $26.9\pm 0.8$ 41/58
7 $6.4 \pm 0.5$ $1.54 \pm 0.07$ $5.0 \pm 0.1$ $7.5 \pm 0.7$ $ 4.9\pm 0.1$ $26.1 \pm 2.0$ 40/58
8 $6.2 \pm 0.5$ $ 1.41 \pm 0.06$ $4.8\pm 0.2$ $8.9\pm 0.8$ $4.7\pm 0.1$ $24.4\pm 2.3$ 38/58

Soft apex
             
9 $5.7\pm 0.7$ $1.31\pm 0.05$ $6.0\pm 0.2$ 11.3+1.4-0.7 $3.7\pm 0.1$ $25.1\pm 3.3$ 74/58

Flaring branch
             
10 $5.8\pm 0.7$ $1.39\pm 0.06$ $8.6 \pm 0.2$ $12.0 \pm 1.0$ $3.6 \pm 0.2$ $25.6 \pm 3.8$ 48/58
11 $5.9 \pm 0.7$ $1.46 \pm 0.05$ $11.6 \pm 0.1$ $12.7 \pm 0.8$ $3.5 \pm 0.2$ $27.2 \pm 4.0$ 40/58
Column densities are in units of 1022 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 normalization of the cut-off power law is in units of photon cm-2 s-1 keV-1 at 1 keV.

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