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Table 2

Fitted and derived properties of Kepler-1705b and Kepler-1705c.

Parameter Prior Kepler-1705b Kepler-1705c
λ [deg] U[0,360] Fitted
P [day] U[8,12] Fitted
ecosϖ U(*) Fitted
esinϖ U(*) Fitted
Mpl[M] U[0,1e-2] Fitted
Rpl[R] U[0,1e-1] Fitted
b U[0,1] Fitted
t0 [BJD-2 454 833.0] Derived
aR Derived
e Derived
ϖ [deg] Derived
I [deg] Derived
Mpl [MEarth] Derived
Rpl [REarth] Derived
ρ [ρEarth] Derived
SN 9.55 8.84 Derived

Kepler-1705

ρ [ρ] G(0.573,0.077) Fitted
Limbdark u1 G(0.344,0.035) Fitted
Limbdark u2 G(0.297,0.043) Fitted
log10(jitter) U[-9,0] Fitted
log10(σGP) U[-9,0] Fitted
log10(τGP) [day] U[0,100] Fitted

Notes. λ (mean longitude), P (period), e (eccentricity), and ϖ (longitude of the periastron) are given at the date 2 455 196.2294 [BJD]. We computed the detection S/N as the median depth of transit over its standard deviation. U(x, y) priors are flat between x and y, G(x, y) priors are Gaussian of expected value x and standard deviation y. (*)For the k = ecosϖ and h = esinϖ variables, an additional prior was added to enforce a uniform distribution for their module e.

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