Table 1
Results of the non-parametric halo occupation distribution analysis.
| ⟨T300kpc⟩ [keV] | Nobj | M∗ [ M⊙ ] | M500,MT [ M⊙ ] | Mgas,500 [ M⊙ ] | f ∗ |
|
|
|||||
| 2.35 ± 0.65 | 21 | (1.30 ± 0.82) × 1012 | 1.4 × 1014 | (9.77 ± 0.75) × 1012 | 0.0095 ± 0.0061 |
| 4.50 ± 0.35 | 7 | (3.86 ± 0.86) × 1012 | 3.9 × 1014 | (1.96 ± 0.16) × 1013 | 0.0099 ± 0.0022 |
| 5.13 ± 0.21 | 6 | (3.86 ± 0.79) × 1012 | 4.8 × 1014 | (2.90 ± 0.23) × 1013 | 0.0080 ± 0.0017 |
Notes. Column description: 1. Mean temperature and standard deviation in the considered temperature bin. 2. Number of clusters per bin. 3. Mean stellar mass per cluster. 4. Mean halo mass estimated using the MWL−T relation. 5. Mean gas mass per cluster (calculated for the same systems). 6. Mean stellar fraction.
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