Fig. B.1

image

One-dimensional version of the kinematic maps for the HDFS galaxies. Each line corresponds to one galaxy, indicated by the ID number on the right panel. The left column shows the LOS velocity, V, and the right column shows the LOS velocity dispersion, σ. Each point corresponds to a spatial bin of the MUSE sub-cubes and the radius is the distance from the center (i.e.  not interpolated either cut along the major axis). Blue points are for the stellar component and orange points are for the gas.

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