Variability in stellar granulation and convective blueshift with spectral type and magnetic activity - II. From young to old main-sequence K-G-F stars

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Fig. 3

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First panel: B−V versus T_eff for the 360 stars in our sample. Second panel: same for the TSS versus B−V. Third panel: same for the TSS versus T_eff. Fourth panel: same for the convective blueshift versus T_eff. Fifth panel: same for the convective blueshift versus B−V.

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