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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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