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Fig. 12.


Distributions of the stars in the RAVE DR5–Gaia DR2 catalog. The blue and orange lines denote stars labeled as in situ or accreted by the network using only 5D kinematics. The black-dashed lines show the distributions of the stars selected with the ZM selection method. The stars selected by the network have similar kinematic profiles, but extend to larger metallicities. The fact that these distributions agree with the expected halo distributions gives us confidence in our ability to derive a catalog of accreted stars for which we do not have access to a metallicity measurement.

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