Fig. 5.

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⟨Sph⟩ distribution in logarithmic scale for the GKM dwarfs, split into Teff intervals of 300 K. The gray shaded histogram shows the distribution for the full subsamples, while the solid black and red lines show the histograms for the slow- and fast-rotating populations, respectively. For clarity, the distributions here are shown by the actual histograms, while we opt for the KDE for the remainder.
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