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Fig. 1

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Gallery of the ten ARKS systems with evidence of asymmetric or offset emission, and their respective observational asymmetry type. The arrows indicate systems that host a major or minor axis with the directionality pointing towards the brighter side. All systems are shown with different contour levels to accentuate their asymmetric features. We present the synthesised beams in the lower left of each panel, as well as 50 au scale bars in the lower right. For systems with significant offsets, we show insets zoomed into their central regions, denoting their phase (stellar) centres as orange stars and best-fit disc centres as blue dots. In all panels north is up and east is left. From left to right, then top to bottom, the images are cropped to fields of view that in both axes are ±7.5″, ±8″, ±0.875″, ±2.5″, ±1″, ±1.125″, ±9″, ±8″, ±3″, and ±4″, respectively.

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