Fig. 7.
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Enclosed mass profiles for the stellar component (red), dark matter component (black), and their combination (blue) for the different DYNAMITE modelling runs of FCC 47. The left panel shows the profiles over the full FoV of the MUSE observations and the right panel only shows the central 10 arcsec in logarithmic scales. The central mass profile is clearly dominated by stellar mass. The shaded regions indicate the 1σ uncertainties of the mass profiles. The spatial resolution of the SINFONI observations is 0.14″ (FWHM). The purple line visualises the effective radius of FCC 47.
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