Fig. 7.
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Characterisation of the substructures identified within the tentative structure B. Left: distribution in the E − Lz plane. The original sample of halo stars is shown as a grey background. Right: normalised MDFs. We use blue for B1 (Thamnos 1) and cyan for B2 (Thamnos 2; see text for details). Error bars are computed assuming Poisson statistics.
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