The resolved Kennicutt-Schmidt relation for the sub-sample of galaxies in the VERTICO sample with inclinations i ≤ 80°, represented as Σ_SFR as a function of Σ_mol. All data points are convolved to a common working resolution of 720 pc. Each data point is color-coded by the distance to the galaxy center. The diagonal dashed, grey lines show constant depletion times of 0.1, 1 and 10 Gyr, respectively. For a fixed molecular gas mass, there are clear galaxy-to-galaxy variations in the KS relation. OLS weighted fits to the line-of-sight measurements are the solid blue lines shown in Table A.1. Note that values for Σ_SFR and Σ_mol have been corrected via cos i. The rest of the panels can be found in Fig. A.1.