Distinguishing the albedo of exoplanets from stellar activity

Free Access

Table 2

Adopted priors for the five parameters of the MCMC.

Parameter	Prior	Interval
A_g	Uniform	[0;1]
P_*	Gaussian	N(P_0,*, 3)
p₁	Log-uniform	[10⁻⁴;600]
p₂	Log-uniform	[5 × 10⁻⁵;2 × 10⁴]
Offset	Uniform	[F_mean − 2 ptp;F_mean + 2 ptp]

Notes. P_0,* represents the original value of the stellar rotation used to build the simulation, F_mean is the flux average, and ptp is the peak-to-peak variation of the light curve.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.