Search for light curve modulations among Kepler candidates - Three very low-mass transiting companions

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Table 4

Priors used in the model fit of the REB modulations and transit, together with the results of the fit for each of the three characterized companions.

Par.	Prior	Units	KOI-554	KOI-1074	KOI-3728

M₂		M_Jup
R₂		R_Jup
M_⋆^a		M_⊙
R_⋆^a		R_⊙
a		au
e		–
ω		deg.
i		deg.
A _B ^c		–
B ^b		–
Sc		ppm

Notes. Parameters with Gaussian priors use as mean value and standard deviation those from CFOP (in the case of M_⋆ and R_⋆) or our calculated values and their uncertainties (B). These values can be found in Table 3.

^(a)

We truncate the Gaussians at 0 to avoid physically meaningless solutions.

^(b)

Assuming a 5% uncertainty.

^(c)

Values above 1 account for the possibility of these targets having some intrinsic luminosity.

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