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Table 3:

The XIS 1-10 keV spectra of the six time-intervals.

Interval 		$\Gamma$ log $\xi$a $N_{\rm W}$b $F_{\rm 2-10}$c
1 $1.50\pm 0.07$ $1.6\pm 0.1$ $1.6\pm 0.2$ 4.8
2 $1.67\pm 0.06$ $1.7\pm 0.1$ $1.2\pm 0.2$ 5.2
3 $1.32\pm 0.08$ $1.3\pm 0.1$ $2.0\pm 0.2$ 3.3
4 $1.08\pm 0.06$ $1.0\pm 0.1$ $2.4\pm 0.2$ 2.6
5 $1.16\pm 0.06$ $1.0\pm 0.1$ $2.4\pm 0.2$ 4.9
6 $1.58\pm 0.06$ $1.6\pm 0.1$ $1.3\pm 0.2$ 5.6
$\Gamma$ - $1.47\pm 0.04$ $1.40\pm 0.04$  
log $\xi$a $1.5\pm 0.1$ - $1.2\pm 0.1$  
$N_{\rm W}$b $2.2\pm 0.3$ $2.2\pm 0.1$ -  
$\chi^2$/d.o.f. 671.8/676 707.2/676 698.1/676  

Notes. Results of fitting a single warm absorber model to the 1-10 keV XIS spectra from the six time-intervals are presented. One of the three parameters, $\Gamma$, $\xi$, and $N_{\rm W}$, is a free parameter when fitting the six spectra, besides the normalizations of the power-law continuum. The other two are tied together between the spectra and reported below. Observed 2-10 keV flux is also given. (a) In unit of erg s-1 cm. (b) In unit of 1022 cm-2. (c) The 2-10 keV flux in unit of 10-12 erg cm-2 s-1.


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