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Table 2.
Spearman correlation coefficients between the RVs and the BIS and FWHM activity indicators.
| Case | Indicator | rs | p-value |
|---|---|---|---|
| I | BIS | −0.13 | 0.44 |
| I | FWHM | −0.39 | 0.02 |
| II | BIS | −0.27 | 0.12 |
| II | FWHM | −0.42 | 0.11 |
Notes. The table presents both simulated cases: Case I–a periodically active star hosting a planet and Case II–a planet hosting star with random spectral variability (see text).
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