Table 2
Detection limit ratios and power criteria.
| Star | R L corr | R L peak | R L LPA | R L corrLPA | Domain | R P 1 | R P 2 |
| (days) | |||||||
|
|
|||||||
| HD 10180 | 2.79 | 0.88 | 2.32 | 0.43 | 4–60 | 0.64 | 1.93 |
| HD 60532 | 2.14 | 1.30 | 2.14 | 1.00 | 150–650 | – | 2.61 |
| HD 105690 | 2.48 | 1.42 | 3.48 | 1.40 | 2–5 | 2.53 | 3.29 |
| HD 115892 | 3.23 | 0.76 | 3.28 | 1.06 | 2–5 | 1.56 | 2.10 |
| HD 124850 | 1.07 | – | 2.21 | 2.07 | – | – | – |
| HD 172555 | 1.64 | 0.91 | 2.37 | 1.49 | 0.01–0.05 | 1.08 | – |
| HD 199260 | 2.07 | 0.84 | 1.87 | 1.00 | 1–4 | 0.62 | 1.48 |
| HD 210302 | 1.03 | 1.06 | 1.49 | 1.50 | 1–3 | 0.93 | 1.14 |
| HD 219482 | 1.87 | 0.88 | 2.07 | 1.25 | 1–3 | 1.39 | 2.02 |
| β Pic | 4.00 | 3.14 | 4.53 | 1.15 | 0.01–0.05 | 2.28 | – |
Notes. RLcorr is the median of the ratio of the rms-based detection limits to the correlation-based detection limits. RLpeak is the median of the ratio of the rms-based detection limits to the peak detection limits. RLLPA is the median of the ratio of the rms-based detection limits to the LPA detection limits. RLcorrLPA is the median of the ratio of the correlation-based detection limits to the LPA detection limits. The domain indicates the period range used in Sect. 6 to estimate the power corresponding to the rms RV. RP1 and RP2 are the ratio of the power at the origin of the RV variations (computed, respectively, across the 0.01–1000 and 2–1000 day domains) to the average power threshold used in the LPA method.
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