Distributions of the physical properties of galaxies after kinematic modeling, arranged from top-left to bottom-right: inclinations, stellar masses, effective radii, and redshifts. These distributions are presented for the KMOS^3D (in red), KGES (in green), and KROSS (in blue) samples. In total, we use 73 KMOS^3D, 21 KGES, and 169 KROSS galaxies to estimate the DM fraction at high-z. The distribution of R_e > PSF galaxies (within final sample) is shown by black hatched histograms. For detailed information on sample selection following kinematic modeling, we refer the reader to Section 3.2.