Table 3: Best fit parameters for the 0.3-10 keV PN spectra of XMMU J004303+4115a. Numbers in parentheses represent 90% confidence uncertainties on the last digit.
Obs. $N_{\rm H}$ $\alpha$ Lb $\chi^2$/d.o.f.
x1 0.6(2) 2.15(15) 3.0(2) 37/34
x2 1.0(2) 1.91(15) 4.4(3) 36/34
x3 1.1(2) 1.98(15) 3.3(2) 16/18
x4 1.4(2) 1.89(15) 12.0(7) 17/34
a An absorbed power law model was used, with line-of-sight absorption $N_{\rm H}$
(in units of 1021 atom cm-2) and spectral index $\alpha$.
b 0.3-10 keV luminosity/1037 erg s-1.

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