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Table 2.
Pairwise statistical tests of the enclosed dark matter masses within RHI across stellar mass bins.
| Comparison | Statistics | log(M*/M⊙) | ||||
|---|---|---|---|---|---|---|
| [8.7, 9.5) | [9.5, 10.0) | [10.0, 10.5) | [10.5, 11.0) | [11.0, 11.4) | ||
| N = 491 | N = 532 | N = 747 | N = 551 | N = 132 | ||
| TNG100-mock vs TNG100-true | MWU p-value | 9.2e–07 | 3.2e–06 | 2.1e–04 | 0.774 | 0.193 |
| Cliff’s δ | 0.181 | 0.165 | 0.111 | –0.010 | –0.093 | |
| KS p-value | 1.3e–07 | 2.6e–09 | 7.8e–05 | 0.060 | 0.036 | |
| ALFALFA vs TNG100-mock | MWU p-value | 2.3e–04 | 1.3e–05 | 1.0e–05 | 1.2e–06 | 8.8e–05 |
| Cliff’s δ | –0.136 | –0.155 | –0.132 | –0.169 | –0.279 | |
| KS p-value | 0.002 | 8.7e–05 | 1.2e–04 | 5.5e–05 | 0.002 | |
Notes. The samples compared are: TNG100-mock versus TNG100-true, and ALFALFA versus TNG100-mock. The number of galaxies in each bin is indicated in the third row of the table. Test statistics are the same as in Table 1.
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