Characterization of the emitting and absorbing media around the nucleus of the active galaxy UGC 11763 using XMM-Newton data

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Table 4:

EPIC-pn fit model parameters for the 2-10 keV energy range.
Model component	Parameter	Value
powerlaw	$\Gamma$	$\rm 1.65_{-0.05}^{+0.06}$
	$K_{\rm pwlw}$	$\rm 8.3_{-0.6}^{+0.6}$
statistic	$\chi^{2}_{\nu}$	1.07
	d.o.f.	112
powerlaw	$\Gamma$	$\rm 1.69_{-0.06}^{+0.06}$
	$K_{\rm pwlw}$	$\rm 8.6_{-0.3}^{+0.4}$
Gaussian	$E_{\rm rest}$	$\rm 6.35_{-0.34}^{+0.16}$
	$\sigma$	$\rm0.26_{-0.11}^{+0.52}$
	$K_{\rm line}$	$\rm0.9_{-0.5}^{+1.1}$
statistic	$\chi^{2}_{\nu}$	0.99
	d.o.f.	109

The galactic $N_{\rm H}$ is fixed to $4.67 \times 10^{20}$ cm^-2. The line energy in the rest frame of the source ( $E_{\rm rest}$ ) and $\sigma$ of the Fe-K $\alpha$ emission line are given in keV; power-law normalizations ( $K_{\rm pwlw}$ ) in units of 10^-4 ph keV^-1 cm^-2 s^-1 at 1 keV; and line normalization $K_{\rm line}$ in units of 10^-5 ph cm^-2 s^-1. Errors quoted are at 90% confidence level.

Source LaTeX | All tables | In the text

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