Fig. B.3.
Radial dependence on the projected velocity dispersion measurement for different cored components (38) on top of a PEMD profile approximating a pure MST, with normalization λc and core radii, Rc. The projected radius from the center of the galaxy is extended to 5 arcsec to visibly see the impact on the kinematic of larger cored components (https://github.com/TDCOSMO/hierarchy_analysis_2020_public/blob/6c293af582c398a5c9de60a51cb0c44432a3c598/MST_impact/anisotropy_ifu.ipynb).
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