Sample distribution in the parameter space of the stellar mass, SFR, and emission line half-light radius, colour-coded by redshift. We compare this with a selection of ground-based near-infrared spectroscopic surveys that used the Hα and [OIII] lines to measure galaxy kinematics at z ∼ 1 − 4 (Turner et al. 2017; Förster Schreiber et al. 2018; Wisnioski et al. 2019; Price et al. 2020). We used UV+IR SFRs from Whitaker et al. (2014) where available for the Turner et al. (2017) sample. We note that all objects at z > 1 from KMOS3D are shown in this figure, but not all objects were used in the kinematic studies because the S/N was low or the objects were too small. The sample selected from JADES (hexagons) probes a very different regime: JADES targets are at higher redshift and lower stellar mass than ground-based facilities have probed thus far.