Fig. 7
Mrk 509 RGS data and best fit for the complete ISM model (see Sect. 4.2.2). All the absorption and emission lines intrinsic to the AGN have been subtracted through the AGN slab model of Detmers et al. (2011). The flux is normalized to the AGN continuum emission. Color code of the labels: red for the hot phase, purple for the warm phase and blue for the cold phase.
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