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Table 1:

Best fit parameters for the baseline model, for E>4 keV.
  $\Gamma$ $N_{\rm H}$ R $E_{\rm line}$ $F_{\rm line}$ EW $\chi^2_r$/d.o.f. Flux (XIS0; 4-10 keV)
    (1023 cm-2)   (keV) 10-5 ph cm-2 s-1 (eV)   10-12 erg cm-2 s-1
Total $1.87\pm0.18$ $\rm 3.30^{+0.22}_{-0.23}$ $\rm 2.0^{+1.7}_{-0.9}$ $6.398\pm0.009$ $\rm 4.34^{+0.55}_{-0.53}$ $206\pm 26$ 0.91/150 4.26
Low $1.90\pm0.33$ $\rm 3.23^{+0.51}_{-0.66}$ $\rm 3.0^{+9.8}_{-2.1}$ $\rm 6.389^{+0.018}_{-0.024}$ $\rm 3.90^{+0.91}_{-0.86}$ $228\pm 53$ 1.00/62 3.53
High $1.87 \pm0.22$ $\rm 3.26^{+0.29}_{-0.28}$ $\rm 1.6^{+1.9}_{-0.9}$ $\rm 6.404^{+0.010}_{-0.015}$ $\rm 4.65^{+0.76}_{-0.72}$ $200\pm 33$ 0.99/111 4.77
Note: from left to right: the index of the power-law ($\Gamma$); the column density of the intrinsic absorber; the relative normalization of the Compton reflection component, R; the centroid energy, $E_{\rm line}$, flux, $F_{\rm line}$, and equivalent width (EW) of the iron line; the reduced $\chi^2$ and the d.o.f.

Source LaTeX | All tables | In the text

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