Table 1.
Mass properties of the selected CAMIRA clusters for the redshift bin.
| Abundance matching | Weak lensing | Mass accretion history | |||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| MAM, 200c | S/NWL | zWL | MWL, 200c | MMAH, 200c | fMAH | zform | |||||||
| z range | min | max | mean | (z = zWL) | (z = 0) | (z = zWL) | |||||||
| [0.2, 0.4) | 1.5 | 0.3 | 8.0 | 3.4 | 2.9 | 0.7 | 13.6 | 0.28 | 2.4 | 0.2 | ∼3.2 | ∼0.76 | ∼0.69 |
| [0.4, 0.6) | 1.7 | 0.3 | 8.0 | 3.0 | 3.2 | 0.7 | 12.6 | 0.48 | 3.7 | 0.4 | ∼6.2 | ∼0.60 | ∼0.63 |
| [0.6, 0.8) | 1.6 | 0.3 | 6.8 | 2.4 | 2.9 | 0.6 | 8.6 | 0.68 | 2.8 | 0.4 | ∼6.0 | ∼0.47 | ∼0.64 |
| [0.8, 1.0) | 1.4 | 0.2 | 5.6 | 1.9 | 2.5 | 0.4 | 4.5 | 0.87 | 2.6 | 0.9 | ∼7.0 | ∼0.37 | ∼0.62 |
Notes. Mass properties for the redshift bin (Col. 1) as inferred from the abundance matching (Cols. 2–4), WL (Cols. 5–7), and mass accretion history (Cols. 8–10). The redshift bin is listed in Col. 1. The minimum, maximum, or mean mass as inferred from the abundance matching are listed in Cols. 2, 3, and 4, respectively. The WL-determined signal-to-noise ratio, mean redshift, and mean mass are listed in Cols. 5, 6, and 7, respectively. The extrapolated mass at z = 0, the fraction of accreted mass at the cluster redshift, and the formation redshift as inferred from a mass-accretion history model are reported in Cols. 8, 9, and 10, respectively. The masses are in units of 1014 M⊙.
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