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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