Fig. 1

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Millimetre continuum images for the REASONS resolved sample of 74 belts, ordered by source RA. North is up and east is left. Bars indicate a physical scale of 50 au, and ellipses represent the synthesised beam of the observations. Images were obtained with the CLEAN algorithm as described in Sect. 3, with weighting parameters, resulting RMS noise levels, and beams listed in the observational log tables (available on ZENODO). All images are in a linear scale, stretching from 0 (black) to the maximum intensity of the image, except in a few cases where the maximum was set to a lower value to highlight emission from a belt with respect to the star or a contaminating source.
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