Fig. 11.

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Intrinsic circular velocity and rotation velocity profiles of C05-NW for the best-fit model of DYSMALpy. From top to bottom, we show as solid lines the intrinsic circular velocity of total mass distribution (baryon + dark matter component; navy), the intrinsic circular velocity of the baryons (gas + stars, cyan), the rotation velocity curve of the total mass distribution (baryon + dark matter; blue), and the intrinsic circular velocity of the dark matter mass distribution (dark violet). All the curves are corrected for inclination. As a reference, the intrinsic velocity dispersion is plotted as dotted black lines. The symmetrized rotation curve, the same as Figure 10, is plotted as navy circles, and the white diamonds show the best-fit model. None of rotation curves is corrected for inclination.
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