Fig. 9.
Maps of the light-weighted stellar population content of the galaxy NGC 1433, as derived from full-spectral fitting. Displayed are age (left panel), [M/H] (centre panel), and [α/Fe] (right panel). The limits of the colour bar are stated in the lower right of each panel. Isophotes are based on reconstructed intensities from the MUSE cube and displayed in steps of 0.5 mag. North is up; east is to the left.
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