Table C.1
Stellar activity measurements from simulated PSLS light curves.
| σA | τA | σ1hr |
|---|---|---|
| 40 ppm | 0.8 d | 173 ppm |
| 166 ppm | 0.5 d | 178 ppm |
| 500 ppm | 0.3 d | 198 ppm |
Notes. The parameters σA and τA are used in PSLS to characterize the amplitude and timescale of stellar activity (Samadi et al. 2019). For comparison, σ1hr is the mean standard deviation that we extracted in a running 1 hr window from the light curves. For each combination of σA and τA we simulated 40 light curves.
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