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Table 1

Cluster sample.

Box Cutout center M vir,BCG R vir,BCG DM mass res r 200 M 200
Cluster IC gen [Mpc/h] Seed x-y-z [Mpc/h] [ M] [Mpc/h] [ M] [Mpc/h] [ M]

C01 MUSIC 80 13 671 38-47-66 5.44E14 2.39 2.82E8 1.24 4.37E14
C02 MUSIC 80 30 596 21-16-64 1.06E15 2.99 2.82E8 1.48 7.54E14
C03 MUSIC 80 30 596 22-16-62 2.09E14 1.53 2.82E8 0.99 2.24E14
C04 MUSIC 48 1502 35-33-20 2.99E14 1.90 6.1E7 0.92 1.81E14
C05 MUSIC 80 7964 62-62-39 1.17E14 1.44 2.82E8 0.73 8.7E13
C06 MUSIC 64 22 109 833 33-16-11 2.08E14 1.75 9.7E7 0.87 1.57E14
C07 NGenIC 100 27 036 89-49-70 1.45E14 1.71 5.52E8 0.79 1.13E14
C08 MUSIC 80 17 794 25-29-42 2.69E14 1.89 2.82E8 0.95 1.99E14
C09 MUSIC 80 25 922 25-48-52 5.29E14 2.37 2.82E8 1.24 4.36E14
C10 MUSIC 80 32 706 66-39-23 5.45E14 2.41 2.82E8 1.23 4.26E14
C11 MUSIC 48 8736 19-14-24 2.11E14 1.79 6.1E7 0.90 1.69E14
C12 NGenIC 100 20 905 34-76-35 2.49E14 1.86 5.52E8 0.98 2.15E14

Notes. For traceability we list the initial conditions generators (Col. 2), the box sizes (Col. 3), and the random seeds (Col. 4). With the cosmological parameters listed in Sect. 2.1 it is possible to reproduce the N-body simulations. We specify the (approximate) position of the clusters on which we centered the 20 Mpc/h cutout in Col. 5.

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