Kepler-447b: a hot-Jupiter with an extremely grazing transit

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Table 4

Derived physical and orbital parameters from the fitted solution of the joint analysis.

Parameter	Derived parameters		Units	Assumptions^c
	Sol. A^a	Sol. B^b

R _⋆			R _⊙	M_⋆, log g
a			AU	P_orb, M_⋆
b				a/R_⋆, i, e, ω
T _dur			h	TR model
M _p			M _Jup	K, M_⋆, P_orb
R _p			R _Jup	R_p/R_⋆, R_⋆
⟨ ρ_p ⟩			ρ _Jup	M_p, R_p
A _ecl / A _pl ^†			%	b, R_p/R_⋆

Notes. All uncertainties cover the 99.7% of the probability distribution (i.e., 3σ).

^(a)

Stellar radius and mass obtained from our spectroscopic analysis (see Sect. 3.1).

^(b)

Stellar radius and mass obtained from Huber et al. (2014).

^(c)

Assumed parameters in the estimation of the derived properties.

^(†)

Fraction of the planet’s projected area eclipsing the stellar disk at mid-transit (in %).

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