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Fig. 1.

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Local sample of Gaia DR3 stars in different dynamical spaces (panels), classified into different groups (indicated by colour) by Dodd23. The panels show the spaces of energy and the vertical and perpendicular components of angular momentum used in Dodd23 to identify the Halo groups. The Disc group (purple) is kinematically selected with a Toomre velocity cut; the rest of the structures are found in the complementary kinematically selected Halo. In the plot, scatter points representing the Disc group have been down-sampled by a factor of 500, whilst the population in the legend is the total population of Disc stars.

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