Impact of the pressure gradient on the circular velocity of galaxies computed at R_out. The KMOS^3D, KGES, and KROSS samples are denoted by red circles, green cross, and blue stars, respectively. The interior of each data point is color-coded for rotation-to-dispersion ratio computed before pressure support correction ($V_{\mathrm{Rout}}^{\mathrm{int}}/\sigma$). The black dashed line represents the one-to-one relation between the two measurements. We observe that galaxies with higher velocity dispersion require large pressure corrections.