Observed kinematics and best-fit models for the ten distant quiescent galaxies for which we can constrain rotational velocities. In the left panels, we show the observed velocities (dispersions) as the black (orange) data points, and the best-fit models are represented by the corresponding lines. In the top right panels we show NIRCam RGB imaging (Casey et al. 2023) where available, or HST F814W imaging otherwise (Scoville et al. 2007). In the bottom right panels we show the inferred 2D line of sight velocity fields. We overlay the MSA microshutter positions in both panels on the right.