Table 5: Results for power law fits and galactic absorption ( $N_{\rm H}^{\rm gal}=1.67\times 10^{20}$ cm^-2) for Q 0000-263 in the energy band 0.2-9.0 keV.
Detector $\Gamma$ Normalization $\chi^2_{\rm red}$ /d.o.f.

(1)

PN $2.19\pm0.12$ $1.31\pm0.14$ 0.91/64

MOS1 $1.98\pm0.40$ $1.58\pm0.19$ 0.67/21

MOS2 $1.82\pm0.23$ $1.46\pm0.23$ 0.52/23

PN+MOS $2.10\pm 0.11$ (a) 0.85/110

The errors given are at the 90% level.
⁽¹⁾ Normalization at 1 keV in 10^-5 ph/keV/cm²/s.
^(a) Different normalizations for the individual detectors.

**Table 5:** Results for power law fits and galactic absorption ( $N_{\rm H}^{\rm gal}=1.67\times 10^{20}$ cm^-2) for Q 0000-263 in the energy band 0.2-9.0 keV.
Detector	$\Gamma$	Normalization	$\chi^2_{\rm red}$ /d.o.f.
		(1)
PN	$2.19\pm0.12$	$1.31\pm0.14$	0.91/64
MOS1	$1.98\pm0.40$	$1.58\pm0.19$	0.67/21
MOS2	$1.82\pm0.23$	$1.46\pm0.23$	0.52/23
PN+MOS	$2.10\pm 0.11$	(a)	0.85/110

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