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Fig. 12.


Panel a: 3–5 keV emission (green) together with Hα emission (red) from MUSE. Panel b: radial profile of the surface brightness in the energy range 3–5 keV (black) versus the simulated PSF of the nucleus (red) from the brightest, less obscured state of the AGN (ObsID 6870); the level of the background is also reported (blue).

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