Fig. 2.
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Example of GALFIT fitting of a galaxy from our sample (HELP-J095953.305+014250.922) with its modeled light profiles (second column) and its subsequent residuals (third column) at two different wavelengths shown from top to bottom. Top: HSC-Y band detection. Middle: ALMA band 6 detection. The left side of each row shows the scientific primary-beam-corrected image, with the beam size and the corresponding 1 arcsecond scale.
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