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Fig. 8.


Galaxy passive fraction as a function of the distance to the cluster in comoving Mpc. Red points are galaxies in filaments connected to the clusters, whose clustercentric distance is computed along the filaments. The results for galaxies in filaments connected to the clusters but with clustercentric Cartesian distance are plotted in yellow. In green we plot galaxies in annuli around the clusters, which are considered to fall on the cluster isotropically. The yellow and green distributions are built from absolute magnitude-matched samples.

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