Table 2: Best-fit parameters of the absorbed power-law, broken power-law and parabolic models. We added a systematic error of 3% to the imaging mode data (exp. 0136540301, 0136540401 and 0136540701) and a systematic error of 1.5% to the Timing mode data (0136541001).
Obs.Id. $\alpha_1$ $E_{\rm b}$ $\alpha_2$ $F_{1 ~\rm keV}$ $F_{0.6-2 ~\rm keV}^a$ $F_{2-10 ~\rm kev}^a$ $\chi^2_r/\rm d.o.f.$
    (keV)   ($\mu$Jy) ( $\times10^{-10}$) ( $\times10^{-10}$)  
0136540301 $1.53\pm0.01$     123.8 3.34 2.25 1.21/125
0136540301 $\rm 1.31^{+0.1}_{-0.16}$ $\rm 1.00^{+0.25}_{-0.12}$ $\rm 1.57^{+0.01}_{-0.02}$ 128.3 3.35 2.21 0.98/123
0136540401 $1.41\pm0.01$     154.8 4.20 3.31 1.40/125
0136540401 $\rm 1.27^{+0.07}_{-0.09}$ $\rm 1.14^{+0.24}_{-0.16}$ $1.45\pm0.02$ 157.1 4.21 3.25 1.20/123
0136540701 $1.15\pm0.01$     153.9 4.25 4.82 1.81/125
0136540701 $1.13\pm0.01$ $\rm 6.56^{+0.20}_{-0.16}$ $\rm 2.26^{+0.17}_{-0.23}$ 153.6 4.24 4.67 1.14/123
0136541001 $1.535\pm0.003$     71.1 1.92 1.28 1.68/125
0136541001 $ 1.521\pm0.004$ $\rm 4.50^{+0.35}_{-0.27}$ $1.70\pm0.03$ 71.0 1.91 1.27 0.61/123
Parabolic model
Obs.Id. $\alpha $   $\beta$ $F_{1 ~\rm keV}$ $F_{0.6-2 ~\rm keV}^a$ $F_{2-10 ~\rm kev}^a$ $\chi^2_r/\rm d.o.f.$
        ($\mu$Jy) ( $\times10^{-10}$) ( $\times10^{-10}$)  
0136540301 $\rm 1.45^{+0.03}_{-0.02}$   $\rm0.16^{+0.03}_{-0.05}$ 124.8 3.35 2.18 0.95/124
0136540401 $\rm 1.34\pm0.02$   $\rm0.14^{+0.03}_{-0.04}$ 155.6 4.21 3.22 1.13/124
0136540701 $\rm 1.16\pm0.02$   $\rm0.02\pm0.01$ 153.9 4.25 4.83 1.81/124
0136541001 $\rm 1.503^{+0.005}_{-0.003}$   $0.054\pm0.04$ 71.2 1.92 1.27 1.24/124
a erg cm-2 s-1.

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