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Table 1

Median and 1σ limits of the posterior marginalised PDFs obtained for the WASP-47 system derived from our global MCMC analysis.

MCMC Jump parameters

Star
Teff [K] 5576 ± 68
[Fe/H] 0.36 ± 0.05
c 1 1.17 ± 0.03
c 2 −0.02 ± 0.02
Planet b
Pb [d] 4.1591409 ± 0.0000072
T0,b – 2 450 000 [BJDTDB] 5764.3463 ± 0.0002
0.04 ± 0.06
0.01 ± 0.09
[m s-1 d1/3] 225.7 ± 3.6
Planet c
Pc [d] 572 ± 7
T0,c – 2 450 000 [BJDTDB] 5981 ± 16
−0.21± 0.24
0.16 ± 0.20
[m s-1 d1/3] 248 ± 43

Derived parameters

Star
u 1 0.462 ± 0.014
u 2 0.242 ± 0.010
Density ρ [ρ] 0.68 ± 0.06
Surface gravity log g [cgs] 4.32 ± 0.05
Mass M [M] 1.026 ± 0.076
Radius R [R] 1.15 ± 0.04
Luminosity L [L] 1.14 ± 0.11
Planet b
Mass Mp,b [MJup] 1.13 ± 0.06
RV amplitude Kb [m s-1] 140 ± 2
Orbital eccentricity eb <0.026 (at 2σ)
Orbital semi-major axis ab [au] 0.051 ± 0.001
Density ρp,b [ρJ] 0.71 ± 0.08
Surface gravity log gp,b [cgs] 3.33 ± 0.03
Equilibrium temperature Teq,b* [K] 1275 ± 23
Planet c
Minimum mass Mp,csinip,c [MJup] 1.24 ± 0.22
RV amplitude Kc [m s-1] 30 ± 6
Orbital eccentricity ec 0.13 ± 0.10
Argument of periastron ωc [°] 144 ± 53
Orbital semi-major axis ac [au] 1.36 ± 0.04
Equilibrium temperature [K] 247 ± 5
a c / R 255 ± 7

Notes.

(*)

Assuming zero albedo and efficient redistribution of energy.

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