Fig. C.1.
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Distribution of the half-mass radius (left) and f5 (right) of the post-merger galaxy on the 3D-2D plane. Each solid line represents a simulation in the suite, spanning from the 16%-th to the 84%-th percentiles. The dashed lines in the two panels are the plane bisectors. The 3D half-mass value is multiplied by 3/4 to account for the projection, as reported by Wolf et al. (2010).
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