Table 2: Results for the broken power law fits assuming galacticabsorption ( $N_{\rm H} = 1.66\times 10^{20}$ cm-2).

Orbit		 $\Gamma _{\rm soft}$ $E_{\rm brk}$ $\Gamma _{\rm hard}$ Norm $\chi^2_{\rm red}$/d.o.f.
    (keV)   (1)  

084		 $2.257\pm0.001$ $4.00\pm0.17$ $2.354\pm0.009$ 0.182 1.22/1584
546 $2.400\pm0.009$ $3.37\pm0.42$ $2.620\pm0.006$ 0.108 1.69/1671
807 $1.969\pm0.001$ $4.63\pm0.19$ $2.027\pm0.006$ 0.316 1.58/1900

 (1): Normalization at 1 keV in ph/keV/cm2/s.


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 The XMM-Newton observations
3 Cross-correlation analysis
4 Time-resolved spectroscopy
5 Discussion
6 Conclusions
References
List of tables
List of figures