Fig. 1
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Observed vs. synthetic fluxes (8800–8835 Å) for stars with interferometric Teff. Solid rainbow: CARMENES normalized template spectra. Dashed green: PHOENIX normalized synthetic spectra. Stars are sorted by decreasing Teff from Schweitzer et al. (2019), with interfer-ometrically derived Teff indicated above them. Bottom panel: zoom-in detail of one representative spectrum.
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