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Table 2.
Summary of the HDBSCAN clustering at different inclinations using the line-of-sight velocity maps.
| Numbers | 90 degrees | 60 degrees | 45 degrees | 30 degrees | 20 degrees |
|---|---|---|---|---|---|
| Clusters | 3 | 3 | 3 | 3 | 2 |
| Clustered galaxies | 2001 | 2061 | 2061 | 1941 | 1929 |
| Outliers | 63 | 3 | 3 | 123 | 135 |
| Clustered galaxies with λR | 1955 | 2016 | 2018 | 1891 | 1891 |
| Clustered SRs with λR | 441 | 613 | 673 | 747 | 1013 |
Notes. SRs are defined by Eq. (1) among those for which λR can be calculated.
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