Relation between SFR and cores. Left: α, β, γ parameters as a function of log M_⋆/M_vir. The curves show the parameterisation of DC14 for α, β, γ and the solid symbols represent our SFGs, excluding ID919 and 943. Middle: DM inner slope γ as a function of the SFR surface density Σ_SFR, scaled to z = 1.5. Right: DM inner slope γ as a function of the logarithmic offset from the MS, δ(MS), using the Boogaard et al. (2018) MS. DM cores are present in galaxies with higher SFR and SFR surface-densities.