Six red-giant asteroseismic binary candidates show blended oscillations that bias mass and radius estimates by factors of up to three.
KEP-A/B" columns present the results from the PDSs of KEPSEISMIC light curves for ABi-A/B (i=1-6), respectively. The
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Hidden oscillations in plain sight: identification of seismically unresolved red-giant asteroseismic binary candidates
Six red-giant asteroseismic binary candidates show blended oscillations that bias mass and radius estimates by factors of up to three.