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Fig. 7


Measured size distribution of galaxies in the central projected R200 for the studied clusters, before (grey) and after (black) statistical field subtraction. Blue and red points: measured sizes for galaxies split over two bins of mean effective surface brightness, also after correction. In this size-range, the data are well described by a power-law index of –3.40 ± 0.19 (in bins of equal logarithmic size).

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