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Fig. A.1.


Stars within Gaia DR2 with δϖ/ϖ < 0.10. These stars have been identified as in situ by our neural network. The b distribution is strongly peaked at 0 and the l distribution is relatively flat, consistent with stars that make up the disk. See Fig. 13 in the main text for the analogous distributions of the stars classified as accreted.

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