Table 5: The best fit results for a model with three xabs components fitting all elements but iron, which was fit separately with a slab model (model C). To fit the full blend we froze the velocity broadening to 200 km s^-1 and the outflow velocity to -530 km s^-1.
Comp. A B C

LETGS:

log $N_{\rm H}$ (m^-2) <25.9 <25.8 24.56 $\pm$ 0.09

log $\xi$ (10^-9 W m) <5 2.1 $\pm$ 0.6 0.8 $\pm$ 0.1

LETGS, HEG and MEG:

log $N_{\rm H}$ (m^-2) <28 25.43 $\pm$ 0.06 24.55 $\pm$ 0.08

log $\xi$ (10^-9 W m) <5 2.17 $\pm$ 0.05 0.80 $\pm$ 0.09

**Table 5:** The best fit results for a model with three *xabs* components fitting all elements but iron, which was fit separately with a *slab* model (model C). To fit the full blend we froze the velocity broadening to 200 km s^-1 and the outflow velocity to -530 km s^-1.
Comp.	A	B	C
LETGS:
log $N_{\rm H}$ (m^-2)	<25.9	<25.8	24.56 $\pm$ 0.09
log $\xi$ (10^-9 W m)	<5	2.1 $\pm$ 0.6	0.8 $\pm$ 0.1
LETGS, HEG and MEG:
log $N_{\rm H}$ (m^-2)	<28	25.43 $\pm$ 0.06	24.55 $\pm$ 0.08
log $\xi$ (10^-9 W m)	<5	2.17 $\pm$ 0.05	0.80 $\pm$ 0.09

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observation and data reduction
	3 Spectral data analysis
	4 Timing analysis
	5 Discussion
	6 Ionization structure
	7 The outflow
	8 Summary and conclusions
	References
	Online Material
	Appendix A
	Appendix B
	Appendix C