Table 1
Summary of the compiled data used in this work.
| Substructure | Sample | # Objects | Source |
|---|---|---|---|
| Globular clusters | − | 147 | Vasiliev 2019 (Kinematics) |
| Harris 1996 ([Fe/H]) | |||
| Satellite galaxies | − | 30 | McConnachie & Venn 2020a,b |
| Halo structures | GSE | 557* | Kushniruk et al. 2024 |
| Splash | 2200* | Kushniruk et al. 2024 | |
| Thamnos | 111* | Kushniruk et al. 2024 | |
| Stellar streams | STREAMFINDER | 43 (1805*) | Ibata et al. 2024, 2021 |
| S5 survey DR1 | 12 (603*) | Li et al. 2019 | |
| Wukong | 13* | Limberg et al. 2024 | |
| LMS-1 | 48* | Malhan et al. 2021 | |
| C-19 | Yuan et al. 2022 | ||
| 10* | Martin et al. 2022 | ||
| Total | − | 238 (5347*) | − |
Notes. The first column shows the substructure group, the second column describes the sub sample of the group, the third column describes the number of objects in the group (GCs, galaxies or streams), with the * symbol indicating the number of individual stars. The final column shows the literature source from which the data was taken.
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