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Fig. 6.

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Examples of the maps of the stellar population properties of TNG501725 obtained from the spatially resolved SED fitting on the three data cubes: G + L + E (a), L + E (b), and E (c). The maps derived from the analysis with the L + E and E data cubes alone have a high spatial resolution and reveal detailed spatial variation in the physical properties compared to those obtained from the analysis with the G + L + E data cubes.

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