Table 5
Detection efficiencies for different planet populations.
| M dwarf | Simulated | Recovered | Efficiency |
|
|
|||
| VHJ | 772 870 | 45.6% | 40.6% |
| HJ | 471 484 | 17.5% | 14.5% |
| WJ | 198 983 | 7.3% | 5.45% |
| VHS | 772 044 | 19.8% | 18.5% |
| VHN | 767 916 | 10.3% | 9.68% |
|
|
|||
| K, G, F dwarf | |||
|
|
|||
| VHJ | 2 476 929 | 9.32% | 8.72% |
Notes. For M dwarfs, we use all 65 258 targets minus the 8 planet candidates, for KGF dwarfs we use 460 910 targets, excluding the planet candidates. The percentage of recovered planets is calculated by normalizing the number of correct detections by the number of possible detections (see Eq. (4)). The efficiency is determined after selection criteria, alias clipping and visual bias filter have been applied to the results from the BLS analysis. For smaller stellar radii, larger planetary radii and shorter periods, the efficiency is higher.
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