From left to right: Restframe-UV absolute M_AB1600 magnitudes, attenuated and intrinsic (unattenuated), dust column density, and projected stellar density maps of a sample of four CoDa III galaxies with dark matter halo masses M_DM = 5 × 10¹¹ − 10¹² M_⊙ at z = 5–7. In the left panel, for each galaxy, symbols mark the positions of maximum attenuated UV flux (green ‘x’), maximum NIR flux – approximated by the maximum projected stellar density (green ‘+’) – and maximum dust column density (green ‘Y’). For the two leftmost plot columns, the colour indicates the absolute magnitude (attenuated or intrinsic) of each cell. The dust column density and projected stellar density are given in log₁₀(M_⊙/pkpc²).