The signature of major mergers on the hydrostatic mass bias of galaxy clusters

Open Access

Fig. A.1.

Time evolution of the galaxy cluster CL4 with multiple overlapping non-isolated major mergers. Top panel: Evolution of the hydrostatic mass bias evaluated at R_vir. Bottom panel: Evolution Γ(a) over the virial volume. The time coordinate is the cosmic time of the simulation. The dashed vertical lines correspond to the major merger events.

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