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Fig. 1


HST/WFC3 lens-subtracted F160W images (brightness scale in μJy arcsec−2, left panel) and Chandra 0.5/7 keV images (right panel) of SDP.9 and SDP.11, overlaid with signal-to-noise ratio (S/N) contours at 880 μm from the SMA (in steps of 3, 6, and 9, Bussmann et al. 2013; Negrello et al. 2014).

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