Fig. 3.
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Upper panel: ⟨V⟩ magnitudes of Monson et al. (2017) minus those calculated from the Gaia average BP magnitude (see Eq. (2)). Lower panel: as above, but for the ASAS ⟨V⟩ magnitudes of the RRd stars. Squares show the three outliers whose ⟨V⟩ magnitudes are seriously flawed (most likely by blending) in the ASAS setting. See text for further details.
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