Fig. 3.
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Comparison between the stellar masses derived using different methods and the pPXF stellar population mass for galaxies in the sample. Left panel: Galaxies within the MUSE-Wide footprint. Right panel: MAGIC galaxies. The dashed line is the one-to-one relation. The black-solid line is a linear fit to the derived masses. Symbols are coloured according to the integrated galaxy’s S/N.
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