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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.