Fig. 1.

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Distributions of the physical properties of the KMOS3D parent and selected sample, arranged from top-left to bottom-right: inclinations, stellar masses, effective radii, and redshifts. The dark blue histogram represents all Hα datacubes with confirmed spectroscopic redshift. The blue histogram shows Hα-detected galaxies with Flag-0 or Flag-1 in Table-6 of Wisnioski et al. (2019). We further select galaxies with inclination angles between 25° ≤θi ≤ 75°, shown in the sky-blue histogram. Lastly, we narrow our focus to galaxies with a signal-to-noise ratio greater than 3, depicted by the yellow hatched histogram. This selection criteria allowed us to perform the robust kinematic modeling of these high-z galaxies.
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