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Table C.11

Properties of the WASP-47 system

Parameter Symbol Value Unit Origin
Stellar parameters

Spectral type G9 Hellier et al. (2012)
Stellar temperature Teff 5552 ± 75 K Vanderburg et al. (2017)
Stellar mass M* 1 .040 ± 0.031 M Vanderburg et al. (2017)
Stellar radius R* 1.137 ± 0.013 R Vanderburg et al. (2017)
Stellar spin inclination i* 69.89.2+11.0$69.8_{ - 9.2}^{ + 11.0}$ deg This work
Stellar equatorial period Peq 39.44.5+2.2$39.4_{ - 4.5}^{ + 2.2}$ d Bryant & Bayliss (2022)
Stellar projected velocity veq sin i* 1.800.16+0.24$1.80_{ - 0.16}^{ + 0.24}$ km s−1 Sanchis-Ojeda et al. (2015)
Age τ 6.51.2+2.6$6.5_{ - 1.2}^{ + 2.6}$ Gyr Almenara et al. (2016)
Limb-darkening coefficients u1 0.540 Exofast
u2 0.209

Planet b parameters

Orbital period P 4.1591492 ± 0.0000006 d Bryant & Bayliss (2022)
Transit epoch T0 2457007.932103 ± 0.000019 BJDtdb Bryant & Bayliss (2022)
Eccentricity e 0 (fixed) Bryant & Bayliss (2022)
Argument of periastron ω 90 (fixed) deg Bryant & Bayliss (2022)
Stellar reflex velocity K 140.84 ± 0.40 m s−1 Bryant & Bayliss (2022)
Orbital inclination i 88.980.17+0.20$88.98_{ - 0.17}^{ + 0.20}$ deg Bryant & Bayliss (2022)
Projected spin-orbit angle λ 0 ± 24 deg Sanchis-Ojeda et al. (2015)
3D spin-orbit angle ψN 28.813.3+11.1$28.8_{ - 13.3}^{ + 11.1}$ deg This work
ψS 29.513.3+11.0$29.5_{ - 13.3}^{ + 11.0}$ deg
ψ 29.213.3+11.1$29.2_{ - 13.3}^{ + 11.1}$ deg

Planet c parameters

Orbital period P 588.8 ± 2.0 d Bryant & Bayliss (2022)
Inferior conjunction epoch T0 2457763.1 ± 4.3 BJDtdb Bryant & Bayliss (2022)
Eccentricity e 0.295 ± 0.016 Bryant & Bayliss (2022)
Argument of periastron ω 112.0 ± 4.3 deg Bryant & Bayliss (2022)
Stellar reflex velocity K 31.04 ± 0.40 m s−1 Bryant & Bayliss (2022)

Planet d parameters

Orbital period P 9.03052118 ± 0.00000753 d This work
Transit epoch T0 2459426.5437 ± 0.0028 t BJDTDB This work
Eccentricity e 0.010.007+0.011$0.01_{ - 0.007}^{ + 0.011}$ Bryant & Bayliss (2022)
Argument of periastron ω 16.598.6+84.2$16.5_{ - 98.6}^{ + 84.2}$ deg Bryant & Bayliss (2022)
Stellar reflex velocity K 4.26 ± 0.37 m s−1 Bryant & Bayliss (2022)
Scaled separation a/R* 16.340.11+0.08$16.34_{ - 0.11}^{ + 0.08}$ Bryant & Bayliss (2022)
Orbital inclination i 89.550.27+0.30$89.55_{ - 0.27}^{ + 0.30}$ deg Bryant & Bayliss (2022)
Impact parameter b 0.1280.085+0.076$0.128_{ - 0.085}^{ + 0.076}$ Bryant & Bayliss (2022)
Transit duration T14 4.288 ± 0.039 h Vanderburg et al. (2017)
Planet-to-star radius ratio Rp/R* 0.02876 ± 0.00017 Bryant & Bayliss (2022)
Projected spin-orbit angle Nondetection deg This work

Planet e parameters

Orbital period P 0.7895933 ± 0.0000044 d Bryant & Bayliss (2022)
Transit epoch T0 2457011.34862 ± 0.00030 BJDtdb Bryant & Bayliss (2022)
Eccentricity e 0 (fixed) Bryant & Bayliss (2022)
Argument of periastron ω 90 (fixed) deg Bryant & Bayliss (2022)
Stellar reflex velocity K 4.55 ± 0.37 m s−1 Bryant & Bayliss (2022)
Transit duration T14 1.899 ± 0.013 h Vanderburg et al. (2017)

We caution that WASP-47 d displays strong TTV with an amplitude of ~6 min. We report here the mid-transit time calculated with a TTV model at the specific epoch of our RM observations (see Sect. 5.11).

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