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Table 3.
Summary of the HDBSCAN clustering at different inclinations using the three types of kinematic maps.
| 90 degrees | 60 degrees | 45 degrees | 30 degrees | |
|---|---|---|---|---|
| Clusters | 5 | 3 | 3 | 3 |
| Clustered galaxies | 2039 | 2062 | 2053 | 2064 |
| Outliers | 25 | 2 | 11 | 0 |
| Clustered galaxies with λR | 1993 | 2017 | 2010 | 2014 |
| Clustered SRs with λR | 461 | 615 | 670 | 838 |
Notes. SRs are defined by Eq. (1) among those for which λR can be calculated.
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