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Fig. 6.

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Projected maps along a cylinder of length 23 Mpc, with radius r200c and centred on a random sample of our galaxy clusters, ordered by their M2D/M (over-plotted above each map) values decreasing from left to right. The pixel red, green, and blue channels are used as follows: the red channel maps the gas projected mass, the green channel maps the dark matter projected mass, and the blue channel maps the stellar projected mass. Columns widths are proportional to the cluster radii.

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