Left: RCs (using the URC model, Sect. 2.1) of our sample of intermediate-z SFGs, colour-coded by stellar mass. The dotted black line shows the physical extent of 1 MUSE spaxel at z ∼ 1, namely 1.65 [kpc]. Right: Inner RC slopes, S (corrected for inclination), as a function of the stellar mass surface density. The data points are colour-coded according to their z. The error bars on the y-axis show the 95% confidence intervals from our 3D kinematic modelling, while the x-axis shows the 1σ uncertainties in Σ_M★.