Table 1: The results of fitting different continuum models to the PN data in the 2-12 keV energy range. The fluxes correspond to the 2-10 keV band and are corrected for absorption. The units are 10^-10 erg cm^-2 s^-1.
Models ${\cal N}_{\rm H}$ kT (keV) $\chi^{2}$ /d.o.f. Flux

(10²³ cm^-2) or $\Gamma$ (2-10 keV)

pow $2.02\pm0.04$ $1.83\pm0.05$ 1111/1141 $2.40\pm0.23$

bb $1.31\pm0.03$ $1.93\pm0.03$ 1206/1141 $1.52\pm0.02$

diskbb $1.69\pm0.03$ $3.4\pm0.1$ 1099/1141 $1.89\pm0.21$

**Table 1:** The results of fitting different continuum models to the PN data in the 2-12 keV energy range. The fluxes correspond to the 2-10 keV band and are corrected for absorption. The units are 10^-10 erg cm^-2 s^-1.
Models	${\cal N}_{\rm H}$	kT (keV)	$\chi^{2}$ /d.o.f.	Flux
	(10²³ cm^-2)	or $\Gamma$		(2-10 keV)
pow	$2.02\pm0.04$	$1.83\pm0.05$	1111/1141	$2.40\pm0.23$
bb	$1.31\pm0.03$	$1.93\pm0.03$	1206/1141	$1.52\pm0.02$
diskbb	$1.69\pm0.03$	$3.4\pm0.1$	1099/1141	$1.89\pm0.21$

Source LaTeX | All tables | In the text