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Table 4
Excess of stellar mass in satellites in each of the subsamples, with respect to the overall best-fitting NFW profile.
| Stell mass density | |||
| Central excess | |||
| Cluster | c NFW | Relative | log(ΔM⋆/M⊙) |
|
|
|||
| All |
|
|
|
| z< 0.114 |
|
|
|
| z ≥ 0.114 |
|
|
|
| M200< 8.6 × 1014M⊙ |
|
|
|
| M200 ≥ 8.6 × 1014M⊙ |
|
|
|
| M⋆,BCG< 9.1 × 1011M⊙ |
|
|
|
| M⋆,BCG ≥ 9.1 × 1011M⊙ |
|
|
|
| n1Mpc,M⋆> 1010M⊙< 87 |
|
|
|
| n1Mpc,M⋆> 1010M⊙ ≥ 87 |
|
|
|
| K0< 70 keV cm2 |
|
|
|
| K0 ≥ 70 keV cm2 |
|
|
|
Notes. Both the relative contribution, and the absolute excess are given, both with respect to the stellar mass included in that NFW profile in the radial regime R< 0.10·R200.
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