Table 2
Estimates for orders of magnitude of Fourier-peak strengths.
Notes. Red and blue numbers indicate swamping by stellar noise at a level of 10−3, with and without occultor, respectively. We assumed an observation duration T of one orbital period; longer observation increases the values of 
. Bottom three rows estimate strengths from the gravitational tide of a nearby moon on the planet, of the planet on the star, and of the star on the planet, respectively.
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