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Fig. 11


Positional offsets between the ALMA detections and the nearest optical/NIR detections. We find good agreement between the positions of the sources in the FIR and in the optical rest-frame. The high-significance continuum detections demonstrate that the astrometric consistency between the HST and ALMA reference frames appears robust to 0.̋1 and that the NIR and FIR/mm emission are nearly co-spatial for most of the cases.

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