Fig. 16.
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Distribution of the independent substructures detected in this work in the E − Lz (top) and the L⊥ − Lz (bottom) planes, colour-coded according to their isochrone fitting age (left) and [Fe/H] (right). This information is displayed in Table 12. In all panels, the grey background represents the original sample of halo stars analysed in this work.
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