Fig. E.1.
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Velocity widths vs. impact parameter in the simulated galaxies at z = 2.55 compared to the data obtained from observations in emission by Christensen et al. (2014) (orange triangles) and Møller & Christensen (2020) (green diamonds). The highlighted symbols correspond to the systems studied in Velichko et al. (2024) (see Table 1).
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