Fig. 5.

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Illustration of different data products derived from the methodology described in Sect. 3. We display the sum of the original MUSE fluxes between 4800 and 5800 Å (top row), and the derived representative MD (bottom row, left) and the ND data (bottom row, right), which is the result of subtracting the representative MD from the original data cube. For the representative MD, it is possible to notice the exponential increase in flux towards the centre. All data cubes were masked for AGN contributions with AON ≥ 20.
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