Velocity dispersion of the integrated spectrum (σ_v, intspec) from Beverage et al. (2025) against the inferred integrated line-of-sight velocity dispersion (σ_v, re) within 1 r_e for the galaxies in our sample. The dashed line indicates a one-to-one ratio. The pink squares indicate galaxies for which only lower limits to the rotational velocity could be obtained. The median offset between the integrated velocity dispersion and the velocity dispersion within 1 r_e is ${33}_{-34}^{+47}$ km s⁻¹.