Intracluster light in clusters of galaxies at redshifts 0.4 < z < 0.8

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Fig. 10

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Relation between the cluster M₂₀₀ mass computed from velocity dispersions from Table 1 and the amount of diffuse light in the F814W-band. The red line has a slope of − 1.85. This figure does not show the two low-redshift clusters seen in Fig. 12.

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