Table 4: Results for power law fits for PKS 2126-158.
Detector $N_{\rm H}$ $\Gamma $ Normalization $\chi^2_{\rm red}$/d.o.f.
  (1)   (2)  

PN(a)		 $1.12\pm0.06$ $1.51\pm0.02$ $0.99\pm0.02$ 0.98/492
PN(a) galactic $1.30\pm0.01$ $0.77\pm0.01$ 1.85/493
PN(b) $0.49\pm8.28$ $1.50\pm0.20$ $1.00\pm0.49$ 1.00/132
PN(b) galactic $1.50\pm0.07$ $1.00\pm0.12$ 0.99/133
PN(c) $3.10\pm1.99$ $1.49\pm0.41$ $0.87\pm0.33$ 0.87/196
PN(c) galactic $1.43\pm 0.04$ $0.88\pm0.04$ 0.88/197
MOS1(a) $1.29\pm0.09$ $1.35\pm0.03$ $1.74\pm0.06$ 1.26/229
MOS1(a) galactic $1.11\pm0.01$ $1.31\pm0.02$ 2.36/230
MOS2(a) $1.13\pm0.09$ $1.34\pm0.03$ $1.71\pm0.06$ 1.22/233
MOS2(a) galactic $1.14\pm0.02$ $1.36\pm0.02$ 1.90/234
The errors given are at the 90% level.
(1) In units of 1021 cm-2; $N_{\rm H}^{\rm gal}=4.90\times 10^{20}$ cm-2.
(2) Normalization at 1 keV in 10-3 ph/keV/cm2/s.
(a) Energy band 0.2-10.0 keV.
(b) Energy band 3.0-10.0 keV.
(c) Energy band 2.0-10.0 keV.


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