The impact of large-scale structure on the anisotropic quenching of satellites

Open Access

Fig. C.2.

Analogues of Figs. 3 (top panel) and 4 (bottom panel) considering only galaxies in systems having a halo mass in the range 12 < log₁₀[M_halo/M_⊙] < 13.5, typically corresponding to the group regime. The dependencies were calculated for 1360 groups with 5446 satellites in total.

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