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Fig. C.2.


Galactocentric velocity distributions of the two sets of stars in the Gaia DR2 dataset with small parallax errors and a measurement of the radial velocity as classified by the kinematic + photometric network. The 2nd and 3rd rows provide correlation plots for the stars labeled as accreted and in situ by the kinematic + photometric network, respectively. Many of the selected stars have kinematics similar to the disk.

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