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Fig. 1.

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The galaxy clusters of our sample. The background images are from the HST and JWST optical/infrared passbands. The blue circles represent the positions of the multiple images employed in the strong-lensing studies by Caminha et al. (2019, 2023) and Bergamini et al. (2019, 2023). The red circles show the area surrounding the multiple images that we considered for the measurement of the projected total mass profiles. The red crosses indicate the centers of the red circles and the origin point of each projected total mass profile. The green lines represent the radii of the red circles, whose length is shown near them.

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