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 7:

Model $\mathcal{C}$ parameters for the narrow emission lines.
Line	$E_{\rm lab}$	$E_{\rm rest}$	$\lambda_{\rm rest}$	$\sigma$	$K_{\rm line}$
O VII (f)	0.5610	0.564^(a)	21.97^(a)	0 (frozen)	$\rm 16_{-14}^{+14}$
O VII (r)	0.5740	0.579^(a)	21.41^(a)	0 (frozen)	$\rm 5_{-3}^{+3}$
Fe XVIII	0.7035	$\rm0.708_{-0.004}^{+0.005}$	$\rm 17.50_{-0.09}^{+0.11}$	$\rm0.004_{-(a)}^{+0.004}$	$\rm 3_{-3}^{+1}$
Ne IX K $\alpha$	blend	$\rm0.917_{-0.015}^{+0.007}$	$\rm 13.52_{-0.22}^{+0.10}$	0.0001^(a)	$\rm 2_{-1}^{+2}$

$E_{\rm lab}$ is the laboratory energy of the lines. $E_{\rm rest}$ and $\lambda_{\rm rest}$ are the energy and wavelength of the lines given in the rest frame of the object. $E_{\rm lab}$ , $E_{\rm rest}$ and $\sigma$ are given in keV, $\lambda$ in Å and $K_{\rm line}$ in 10^-5 ph cm^-2 s^-1. ^(a) Unconstrained parameter, see text. Errors quoted are at 90% confidence level.

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