Table 9.
Results of different mass estimates for all the observed galaxy clusters described in the main text.
| Mass | 1230C | 1230SW | 1230E | 1310C | 1310S | 1414S | 2116S |
|---|---|---|---|---|---|---|---|
| M500(β) | 1.9 ± 0.4 | 1.14 ± 0.2 | – | 2.0 ± 0.4 | 3.3±0.7 | 3.9 ± 1.0 | 1.02 ± 0.3 |
| M500(βfix) | 3.1±0.6 | 2.9 ± 0.5 | – | 3.1 ± 0.6 | 2.7±0.6 | 5.2 ± 1.5 | 1.5 ± 0.4 |
| M500(LX) | 4.7 ± 1.9 | 2.3 ± 0.9 | 1.5 ± 0.6 | 2.8 ± 1.1 | 3.6 ± 1.4 | 5.4 ± 2.1 | 3.2 ± 1.3 |
| M500(TX) | 3.1 ± 0.4 | 2.9 ± 0.16 | – | 3.3 ± 0.5 | 3.05 ± 0.5 | 5.2 ± 0.6 | 1.48 ± 0.3 |
| M500(Mgas) | 4.2 ± 0.6 | 2.3 ± 0.35 | 1.2 ± 0.2 | 3.05 ± 0.4 | 4.1 ± 0.6 | 6.0 ± 0.9 | 2.0 ± 0.3 |
| M500(YX) | 3.7 ± 0.4 | 2.3 ± 0.25 | – | 3.05 ± 0.3 | 3.6 ± 0.4 | 5.7 ± 0.6 | 1.7 ± 0.2 |
| Mdyn | 5.6 ± 1.0 | 2.7 ± 2.0 | ∼0.7 | ||||
| M500 | 3.7 ± 0.4 | 2.5 ± 0.25 | 1.35 ± 0.3 | 3.1 ± 0.3 | 3.4 ± 0.4 | 5.5 ± 0.6 | 1.9 ± 0.2 |
| r500 | 3.45 | 2.98 | 2.39 | 3.69 | 3.94 | 2.97 | 2.27 |
Notes. All masses are given in units of 1014 M⊙. M500(β) and M500(βfix) are hydrostatic mass estimates based on β models for the surface brightness distribution of the ICM, where the first value is based on the fitted value for β and the second value is for a model with β = 2/3. M500(LX) and M500(TX) are based on the X-ray luminosity–mass relation and temperature–mass relation, respectively. M500(Mgas) was determined from the total gas mass in the cluster and the relation of the baryon fraction with cluster mass, M500(YX) was derived from the scaling relation of the product of gas mass and temperature with cluster mass, and M500 was derived from the mean of the scaling relation results.
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