Fig. 1.
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Phase-folded RV curves and orbital solutions constrained by Banyard et al. (2022) for the SB1s. The five marked with (*) do not pass the Lucy-Sweeney test (e/σe ≤ 2.49) and so are consistent with being circular (we show the eccentric solution). The ephemerises used to phase the RV curves are calculated with the orbital solutions in Table 2, with phase 0 corresponding to the periastron passage.
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