Table 4: Best-fit parameters of the seven spectra extracted from the November 14, 2002 observation and from the flaring section of the December 1st, 2002 observation, modelled with an absorbed power law.
Section $\alpha $ ka $F_{0.6-10 ~\rm keV}$b $\chi^2_r/\rm d.o.f.$
      ( $\times10^{-10}$)  
14 November 2002, Obs. Id. 0136540701
1 $1.20 \pm 0.01$ $0.199\pm 0.002$ 7.44 1.28/125
2 1.16+0.01-0.02 $0.211\pm 0.001$ 8.12 1.73/125
3 $1.10\pm0.01$ $0.250\pm 0.002$ 10.1 1.70/125
4 $1.03\pm0.01$ $0.312\pm0.002$ 13.4 1.72/125
5 $1.17\pm0.01$ $\rm0.269^{+0.001}_{-0.002}$ 10.3 1.35/125
6 $1.24\pm0.01$ $\rm0.222^{+0.001}_{-0.002}$ 8.04 1.39/125
7 $1.23\pm0.01$ $0.197\pm0.002$ 7.16 1.31/125
1 December 2002, Obs. Id. 0136541001
1 $1.597\pm 0.006$ $0.1027\pm0.0004$ 2.95 1.02/977
2 $\rm 1.574^{+0.006}_{-0.007}$ $\rm0.1057^{+0.0003}_{-0.0004}$ 3.08 0.96/998
3 $1.557\pm 0.006$ $\rm0.1113^{+0.0003}_{-0.0004}$ 3.27 1.15/1029
4 $\rm 1.517^{+0.007}_{-0.006}$ $\rm0.115^{+0.0003}_{-0.0005}$ 3.46 1.02/1026
5 $1.518\pm0.006$ $\rm0.1118^{+0.0003}_{-0.0004}$ 3.36 1.09/1049
6 $1.535\pm0.006$ $0.1066\pm0.0004$ 3.17 1.06/1038
7 $\rm 1.542^{+0.006}_{-0.007}$ $0.1029\pm0.0004$ 3.05 1.07/1033
a Power law normalization (cts cm-2 s-1 keV-1); b erg cm-2 s-1.

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