Fig. 1.
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Filamentary network around cluster CE-29, as detected by DisPerSE applied to C-EAGLE galaxies. Filament spines (red lines) are shown together with the virial boundary of the cluster (white region) for approximately the full (40 Mpc)3 box (left) and zoomed to the central region (right). The locations where the filamentary network crosses the virial boundary are labelled with yellow symbols. The centres of the two merging subclusters (sc1 and sc2) are marked with black arrows.
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