Fig. 9
Fraction of post-starburst galaxies as a function of the two cluster mass tracers, velocity dispersion (left) and LX (right). k+a and a+k are considered as one single class. As done for Fig. 7, only galaxies within R500 are taken into account. Points with different colours refer to different magnitude limits and are used later on for a comparison with high redshifts samples.
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