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Table C.5

Properties of the HD 89345 system

Parameter Symbol Value Unit Origin
Stellar parameters

Spectral type G5 Cannon & Pickering (1993)
Stellar temperature Teff 5499 ± 73 K Van Eylen et al. (2018)
Stellar radius R* 1.6570.004+0.020$1.657_{ - 0.004}^{ + 0.020}$ R Van Eylen et al. (2018)
Stellar spin inclination i* > 44 deg Van Eylen et al. (2018)
Stellar equatorial period Peq d
Stellar projected velocity veq sin i* 0.58 ± 0.28 km s−1 This work
Age τ 9.41.3+0.4$9.4_{ - 1.3}^{ + 0.4}$ Gyr Van Eylen et al. (2018)
Limb-darkening coefficients u1 0.535 Exofast
u2 0.215

Planet b parameters

Orbital period P 11.8144024 ± 0.0000066 d This work (TESS + K2)
Transit epoch T0 2458740.81147 ± 0.00044 BJDtdb This work (TESS + K2)
Eccentricity e 0.208 ± 0.039 This work
Argument of periastron ω 21.7 ± 19.1 This work
Stellar reflex velocity K 9.1 ± 0.5 This work
Scaled separation a/R* 13.625 ± 0.027 Van Eylen et al. (2018)
Orbital inclination i 87.68 ± 0.10 deg This work (TESS + K2)
Impact parameter b 0.564 ± 0.017 This work (TESS + K2)
Transit duration T14 5.65 ± 0.02 h This work (TESS + K2)
Planet-to-star radius ratio Rp/R* 0.03696 ± 0.00041 This work (TESS + K2)
Projected spin-orbit angle λ 74.232.5+33.6$74.2_{ - 32.5}^{ + 33.6}$ deg This work
3D spin-orbit angle ψN 78.723.0+22.5$78.7_{ - 23.0}^{ + 22.5}$ deg This work
ψS 81.623.2+22.2$81.6_{ - 23.2}^{ + 22.2}$ deg
ψ 80.123.1+22.3$80.1_{ - 23.1}^{ + 22.3}$ deg

Notes: Instead of using this lower limit we reproduced the PDF on i* from Van Eylen et al. (2018) to calculate the PDF on ψ from our results.

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