Fig. 7
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Comparison of the primary mass, MAa, derived in this work (vertical grey band, showing the 1σ credibility interval) against literature values. The markers represent estimates from non-seismic spectroscopy (Fuhrmann 1998), stellar modelling (Yang & Meng 2010; Li et al. 2019), and asteroseismic analyses (Grundahl et al. 2017; Gupta et al. 2025).
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