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Fig. 11


Mass distribution (left) and size distribution (right) of log M/M> 10.7 galaxies of high-redshift (blue) or Coma (red) cluster galaxies. Sizes are not corrected for PSF blurring effects. To account for the different richness of compared samples, we matched the number of galaxies with masses in the lowest mass bin. The outlier with smallest effective radius reduced to log M/M = 11 is the peculiar BCG of the z = 1.63 cluster.

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