Morphology-density relation, quenching, and mergers in CARLA clusters and protoclusters at 1.4 < z < 2.8

Open Access

Fig. 8.

ETG (left) and passive (right) galaxy fractions as a function of environment. Details are the same as in the right panels of Fig. 5 and Fig. 7, excluding the cluster CARLAJ0800+4029, and separating the z ∼ 2 clusters from the others at z < 1.9. This shows that the relations holds at z ∼ 2.

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