The impact of baryons on the sparsity of simulated galaxy clusters from THE THREE HUNDRED Project - Astrophysical and cosmological implications

Open Access

Fig. A.1.

Average sparsity ⟨s_200, 500⟩ as function of M₂₀₀ for the clusters in the GADGET-X (top panel) and GIZMO-SIMBA (bottom panel) catalogues at z = 0 and 1, respectively. The blue solid line corresponds to the case of the full cluster sample, while the goldenrod solid line corresponds to the relaxed one. The shaded areas correspond to the standard deviation in each mass bin.

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