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Fig. E.4.

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Multiwavelength view of the CRISTAL galaxies including from left to right: integrated [C II] line emission, [C II]-based velocity field, dust continuum emission, [C II] and dust continuum emission overlaid on a composite image based on HST/WFC3 and JWST/NIRCam observations. The redshift, stellar mass, and SFR are listed in the top left corner of the second panel. S/N contours correspond to 3, 4, and 5σ and then increase in steps of 2σ.

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