Fig. 9
Error contours at the 1 and 3σ c.l. for the best-fitting LF parameters considering the galaxy population within R < R200 (left panel) and R < 0.5R200 (right panel). Black, red and blue lines show the composite LF for the whole galaxy sample, red and blue galaxies, respectively. Solid lines indicate DARC clusters and dashed lines indicate relaxed clusters.
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