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Fig. B.1.
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(a) JWST/NIRCam F444W image of the A28/A43 group. The ALMA 1.17 mm continuum is overlaid as white contours in levels of 2, 4, 8, 16, 32…×RMS. (b) VLT/MUSE spectra of A28, A43, and another group member. The horizontal dashed line indicates zero flux.
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