Fig. 1

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SMA 868 μm (345 GHz) images of all 10 PILS-Cygnus sources (N53 and N54 are both featured in the middle right panel) contoured in red at 10, 40, and 70% of the maximum flux. The cyan ellipses in the upper right corners show the FWHMa of both axes and positionangle of the synthesised SMA beam, and the line segments alone the bottoms of each panel show how long 10 000 AU and its corresponding angular length appears at the adopted distance to each object. We note the change of scale for S26. All images are normalised to their peak flux densities, which are given in Table 1.
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