Table 2
Some known USP planets given in the exoplanetarchive.ipac.caltech.edu catalog.
| Planet name | Period [hr] | Mass [M⊕] | Time [days] |
|---|---|---|---|
| CoRoT-7 b | 20.49 | 3.18 | 20.49 |
| Kepler-407 b | 16.06 | 3.20 | 11.38 |
| Kepler-10 b | 20.10 | 4.61 | 4.91 |
| WASP-47 e | 18.95 | 6.83 | (⋆) |
| 55 Cnc e | 17.68 | 8.08 | (⋆) |
Notes. For all targets, the stellar mass is assumed to be 1 M⊙ and the eccentricity 0. Columns indicate the planet’s name, orbital period, mass and the observational time we need with the proposed technique to achieve PDET = 80% and PFA =1% with test 
computed for L = 2 and d t = 12 hr. Symbols (⋆) indicate that the target is detectable with probability higher than 80% for the considered parameters (mass and period) and sampling rate. For instance, WASP-47 e would be detectable with probability > 97% as soon as the observation time is superior to 6 days and 55 Cnc e with aprobability >99%.
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