Fig. 12.
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Metallicity distribution functions of the 12 extended substructures identified in this work. These MDFs are compared to that of the whole halo population under analysis (blue shaded area) and to that of Gaia-Enceladus (grey dashed histogram). Substructure ID and number of associated stars with a [Fe/H] determination from LAMOST LRS are listed. Error bars were computed assuming Poisson statistics.
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