Fig. A.1.
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Disc kinematic best-fit of the total flux, velocity, and velocity dispersion of GS_4891 (first to third rows). The analysis was performed with 3D-BAROLO (Di Teodoro & Fraternali 2015) on the kinematics maps obtained from a spaxel-by-spaxel emission-line fitting (see Section 3.3 and Figure 11). The black and green lines identify the major axis and the zero-velocity curve, respectively.
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