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Fig. 14.

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Metallicity distribution function of ellipsoidal candidates having vbroadM < 2, vradM < 2, and Δ[M/H] ≤ 0.1 dex from Gaia RVS spectra (aquamarine filled histogram), SB1 stars from the GALAH survey (dashed orange line), and APOGEE close giant binaries (purple dotted line).

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