Fig. D.1.
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Spatially resolved maps of visual extinction and electron density in the circumnuclear region of NGC 1365 obtained from the MUSE data, zoomed in the MIRI FoV. Top panel: visual extinction computed from the Balmer decrement. Bottom panel: ionized gas electron density obtained from the [S II]λ6716/[S II]λ6731 line ratio. Contours represent arbitrary flux levels of [Ne V]λ14#x03BC;m. The black circle marks the 1.5″radius aperture used to extract integrated fluxes for the HOMERUN code (see Section 3.5). The star indicates the nucleus position.
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