Resolved [CII]-SFR relation for galaxies at z ∼ 5. The grey contours show the individual pixel distribution for the whole sample. Each pair of coloured points represents a high- and low-[CII] density average region for each galaxy of the sample following B23 methodology. The orange line and shaded region shows our best-fit power-law model from the tailored likelihood-based approach with the parameters in the top left corner (where log₁₀(C₀) is the value at g₀ = 10^7.5 L_⊙ kpc⁻²). The dashed black line presents the extrapolation of the relation derived from a spatially resolved sample of 46 nearby galaxies by Herrera-Camus et al. (2015). We represented the typical errors bars for the individual pixels across the sample with three black squares.