Table 2.
SCC between the log ⟨Sph⟩ and log σ(Sph) residuals and the different stellar properties of stars with similar Teff and L to those of the Sun (gray dots in Fig. 8).
| Teff⊙ ± 100 K; L⊙ ± 0.3 | |||||
|---|---|---|---|---|---|
| All | Spectroscopic | ||||
| N stars | 3470 | 1303 | |||
| ⟨Sph⟩5 th | 87.0 | 72.0 | |||
| ⟨Sph⟩95 th | 4454.6 | 4552.9 | |||
| ⟨Sph⟩ | σ(Sph) | ⟨Sph⟩ | σ(Sph) | ||
| SCC | Teff | 0.03 | −0.02 | −0.04 | −0.03 |
| L | −0.35 | −0.10 | −0.28 | −0.13 | |
| [Fe/H] | 0.20 | 0.02 | 0.34 | 0.11 | |
| Prot | −0.67 | −0.37 | −0.75 | −0.38 | |
| ⟨Sph⟩ | – | 0.92 | – | 0.94 | |
Notes. The first columns correspond to all stars within the parameter space, while the last ones correspond solely to the stars with spectroscopy. The top lines indicate the number of stars and 5th and 95th percentiles of the ⟨Sph⟩ distribution.
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