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Fig. 2.

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Colour-composite images from the DESI Legacy Imaging Surveys of the RC non-detected CHILLING sample, showing more compact emission, with overlaid 2.1 GHz ATCA radio emission contours starting at 3σ and increasing by a factor of 2 $ \sqrt{2} $. The scale in the top left corner is calculated using the distance to the source. The beam is shown in the bottom left corner. The noise level σ2.1 GHz can be taken from Table 3.

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