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Fig. 1.

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Maps of stellar properties derived with the GIST Pipeline run on the MUSE WFM datacube. Left: stellar velocity map; zero velocity corresponds to a radial velocity of 1313 km s−1. Middle: map of the weighted mean stellar age of the best-fit templates. Right: map of the weighted mean metallicity of the best-fit templates. These maps were derived using GIST Pipeline over a wavelength range of 5050−6000 Å, with Voronoi binning used to obtain a S/N ≥ 300 in each bin. All spaxels with significant jet emission were masked in the datacube to avoid confusion.

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