SFR per area vs. stellar mass surface density for different regions in the disc of UGC 10214. Upper row: SFR derived from the FUV and 24 μm emissions, SFR_FUV, and lower row: SFR derived from the Hα and 24 μm emission, SFR_Hα. The pixels in the separate panels correspond to the different regions shown in Fig. 1. The colour of the markers of the different regions indicates the distance to the galaxy centre. For comparison, the pink ellipse shows the location of the resolved MS from Ellison et al. (2018).