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Table 3:

Spectral fits of the May 2007 EPIC spectra of PG 2112+059: Continuum properties.

Fit
Modela Absorber Continuum Distant Statistic
    neutral power-law Reflection  
    $N_{\rm H}$b cfc $\xi$d $\Gamma$e Normg Normg $\chi^2$ dh
    [ $\rm 10^{22}~cm^{-2}$]   [$ \log$]   $[\rm keV^{-1}~cm^{-2}~s^{-1}]$ $[\rm keV^{-1}~cm^{-2}~s^{-1}]$    

1
i * (p + d) $\rm 18.3_{-1.9}^{+2.7}$ $\rm0.94_{-0.02}^{+0.01}$ $\rm 1.10_{-0.52}^{+0.45}$ $\rm 2.08_{-0.13}^{+0.16}$ $\rm 8.74_{-2.51}^{+2.29}\; 10^{-5}$ $\rm 9.24_{-5.14}^{+8.03}\; 10^{-5}$ 93.2 99
2 i * (p + k(r) + d) $\rm0.12_{-0.02}^{+0.39}$ $\rm 1.00_{-0.14}^{+0.00}$ $\rm -1.36_{-0.31}^{+3.04}$ $\rm 1.53_{-0.10}^{+0.16}$ $\rm 3.58_{-0.89}^{+0.74}\; 10^{-6}$ $\rm 1.45_{-0.95}^{+1.17}\; 10^{-5}$ 96.7 93

Notes. Explanation of labels: (a) the spectral models described in Table 2; (b) equivalent column density; (c) covering fraction; (d) ionisation level of absorbing material $\xi=L/nr^{2}$, as defined in XSPEC; (e) photon index of power-law continuum; (g) normalisation of photon flux at 1 keV; (h) degrees of freedom. The best-fit parameters for the ionised reflector, the disk, and the black hole are provided in Table 4. All errors are provided at the 90% confidence level.


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