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Fig. A.1.

image

CL1604 sample of galaxies introduced in Sect. 3 and presented in the same order as in Table A.1. The first and second columns show the original HST-F814W or HSC-z-band images centered on the targets and their residuals after subtracting the 2D model of the galaxies. The pixel scale in the first column corresponds to 0.05″ pix−1 for HST images and 0.2″ pix−1 for HSC images. The third column presents the synthetic velocity field after fitting the simulated rotation curve to the observed curve (assuming the pixel scale of OSIRIS, i.e., 0.25″ pix−1). The solid black parallel lines depict the edges of the slit. The fourth column displays the observed (black dots) and modeled (red line) rotation curve.

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