Table 1: Spectral fit parameters. The given fluxes are corrected for an encircled energy fraction of 85%. The errors are the 1 $\sigma$ confidence level.
Power-law Model

$N_{\rm H}$ $\rm 21_{-1}^{+4}\times 10^{22}$ cm^-2

$\Gamma$ $\rm 1.6_{-0.1}^{+0.2}$

$\chi^2$ 55.9 (69 d.o.f.)

2-10 keV unabsorbed flux $1.7\times 10^{-11}$ erg/s/cm²

Comptt

$N_{\rm H}$ $14\pm2\times 10^{22}$ cm^-2

$kT_{{\rm seed}}$ $\rm 1.6_{-0.3}^{+0.5}$ keV

$kT_{{\rm e}}$ 10 keV fixed

$\tau$ $\leq$ 3.35 (3 $\sigma$ )

$\chi^2$ 56.2 (68 d.o.f.)

2-10 keV unabsorbed flux $1.1 \times 10^{-11}$ erg/s/cm²

**Table 1:** Spectral fit parameters. The given fluxes are corrected for an encircled energy fraction of 85%. The errors are the 1 $\sigma$ confidence level.
Power-law Model
$N_{\rm H}$	$\rm 21_{-1}^{+4}\times 10^{22}$ cm^-2
$\Gamma$	$\rm 1.6_{-0.1}^{+0.2}$
$\chi^2$	55.9 (69 d.o.f.)
2-10 keV unabsorbed flux	$1.7\times 10^{-11}$ erg/s/cm²
Comptt
$N_{\rm H}$	$14\pm2\times 10^{22}$ cm^-2
$kT_{{\rm seed}}$	$\rm 1.6_{-0.3}^{+0.5}$ keV
$kT_{{\rm e}}$	10 keV fixed
$\tau$	$\leq$ 3.35 (3 $\sigma$ )
$\chi^2$	56.2 (68 d.o.f.)
2-10 keV unabsorbed flux	$1.1 \times 10^{-11}$ erg/s/cm²

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