Examples of ALMA-detected galaxies in our sample. The HST F160W image is shown in the background, smoothed by a 0.3″ FWHM Gaussian to reveal extended features. The white contours show the extent of the ALMA emission (3, 5, 10 and 17σ) after applying tapering. The size and orientation of the ALMA clean beam is given with a yellow hatched region (FWHM). The CANDELS ID of each target is given at the top of each cutout, together with the S/N of the integrated ALMA flux.