Table 3.
Total counts of cluster types.
| Type | Label | Criteria | Count | (high q.) (a) |
|---|---|---|---|---|
| OC | o | P(rJ)≥0.5 and | 5647 | 3530 |
| MJ ≥ 40 M⊙ | ||||
| MG | m | P(rJ) < 0.5 or | 1309 | 539 |
| MJ < 40 M⊙ | ||||
| – no rJ | P(rJ) < 0.5 | 992 | 301 | |
| – has rJ | P(rJ)≥0.5 | 317 | 238 | |
| GC | g | Crossmatching (b) | 132 | 25 |
| Too distant | d | d ≥ 15 kpc | 62 | 6 |
| Rejected | r | Manual (c) | 17 | – |
Notes.
Count of how many clusters of a given type are also in the high-quality sample of clusters from Paper II, which are those with a median CMD class greater than 0.5 and an astrometric S/N (CST) greater than 5σ.
Clusters defined as GCs in Vasiliev & Baumgardt (2021), Kharchenko et al. (2013), or Gran et al. (2022).
Clusters later matched to galaxies or dwarf galaxies, or removed due to being obvious clustering algorithm errors (see Sect. 4.1).
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