Fig. 10.
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Comparison of DM velocity profiles for the three galaxies shown in Fig. 9. The green curves show the profiles modelled with GALPAK3D assuming a DC14 halo, while the purple curves are obtained by subtracting the baryonic contributions obtained with vcdisk from the MUSE-derived vc(r). The green shaded regions indicate the 95% confidence intervals from the 3D disk–halo decomposition fits.
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