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Table 2

Adopted priors for the five parameters of the MCMC.

Parameter Prior Interval
Ag Uniform [0;1]
P* Gaussian N(P0,*, 3)
p1 Log-uniform [10−4;600]
p2 Log-uniform [5 × 10−5;2 × 104]
Offset Uniform [Fmean − 2 ptp;Fmean + 2 ptp]

Notes. P0,* represents the original value of the stellar rotation used to build the simulation, Fmean is the flux average, and ptp is the peak-to-peak variation of the light curve.

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