Table 3.
Estimated mass (first row) and concentration (second row) for the case of the galaxy clusters acting as lenses by means of the NFW+NFW profiles for small (≲100 kpc) and large (≳100 kpc) scales derived by Fernandez et al. (2022).
| Bin 1 | Bin 2 | Bin 3 | Total | |||||
|---|---|---|---|---|---|---|---|---|
| Richness [12–17] | Richness [18–25] | Richness [26–40] | Richness [12–220] | |||||
| NFWsmall | NFWlarge | NFWsmall | NFWlarge | NFWsmall | NFWlarge | NFWsmall | NFWlarge | |
| log10(M/M⊙) | 13.58 | 13.76 | 13.37 | 13.89 | 13.86 | 14.05 | 13.61 | 13.85 |
| C | 3.63 | 0.74 | 6.83 | 0.39 | 3.81 | 1.00 | 4.17 | 1.72 |
Notes. From left to right, the first three bins and the total case are summarised according to the best-fit mass density profile. For each of the four cases, the results for small and large angular scales are shown.
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