Table D.1.
KS statistic comparing 1D distributions of the LR+HALOSCOPE halo properties with respect to the HR ones in different mass bins, as indicated in the first two columns.
| M200b(M⊙h−1) | cvir | λ | c/a | b/a | |
| Min. | Max. | ||||
| 2 ×1011 | 4.5 ×1011 | 0.012 | 0.012 | 0.015 | 0.023 |
| 4.5 ×1011 | 1×1012 | 0.012 | 0.012 | 0.014 | 0.025 |
| 1 ×1012 | 2.3×1012 | 0.012 | 0.012 | 0.014 | 0.026 |
| 2.3×1012 | 5.3×1012 | 0.01 | 0.011 | 0.013 | 0.027 |
| 5.3×1012 | 1.2×1013 | 0.011 | 0.01 | 0.012 | 0.027 |
| 1.2×1013 | 2.7×1013 | 0.01 | 0.01 | 0.011 | 0.022 |
| 2.7 ×1013 | 6.15×1013 | 0.009 | 0.009 | 0.01 | 0.019 |
| 6.15×1013 | 1.4×1014 | 0.008 | 0.008 | 0.008 | 0.015 |
| 1.4×1014 | 3.2×1014 | 0.008 | 0.007 | 0.007 | 0.005 |
Notes. All the reported values are below the null hypothesis threshold. There is a good agreement between the distributions of LR+HALOSCOPE halo properties and those from the HR simulation
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