X-ray view of dissipative warm corona in active galactic nuclei

Open Access

Fig. A.1.

Scatter plot showing the best fitted hydrogen column density, $N_{H}^{CL}$ $N^{\mathrm{CL}}_{\mathrm{H}}$ , against ionization parameter, ξ_CL, of CLOUDY model. The distribution of their values is shown as grey histograms. Different symbols associated with sources are the same as in Fig. 6.

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