Fig. C.3

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Distributions of log R′HK,PHOENIX values in (a) Teff versus log g, (b) Teff versus [Fe/H], and (c) [Fe/H] versus log g parameter spaces for solar-like stars with more than one observation and σ log R′HK,PHOENIX / log R′HK,PHOENIX < 0.2. The form of this image is similar to that in Figure 13, where the error bars belong to the bottom end of the data point.
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