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Table 4.
Same as Table 3, but with no requirement of vlos, that is, requiring parallax errors δϖ/ϖ < 0.10 only.
| δϖ/ϖ < 0.10 | Accreted | in situ | Purity |
|---|---|---|---|
| Training set | 430 376 | 48 266 382 | 0.88% |
| Validation set | 8938 | 991 062 | 0.89% |
| Test set | 8828 | 991 172 | 0.88% |
Notes. Removing the requirement on vlos increases the sample size by a factor of ∼5 and the number of accreted stars by a factor of ∼9.
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