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Table 9

Physical parameters of the planetary system WASP-11/HAT-P-10 derived in this work.

Parameter Nomen./Unit This work West et al. (2009) Bakos et al. (2009) Wang et al. (2014)

Stellar parameters
Spectral class...... K3 V K K ...
Effective temperature...... Teff (K) 4900 ± 65 4800 ± 100 4980 ± 60 ...
Metal abundance...... [ Fe / H ] + 0.12 ± 0.09 + 0.0 ± 0.2 + 0.13 ± 0.08 ...
Proj. rotational velocity...... vsini (km s-1) 1.04 ± 0.15 < 6.0 0.5 ± 0.2 ...
Linear LD coefficient...... u 0.78 ± 0.16 ... ... ...
Mass...... M ( M) 0.806 ± 0.038 ± 0.013 0.83 ± 0.03 0.862 ± 0.014
Radius...... R (R) 0.772 ± 0.014 ± 0.004 0.79 ± 0.02
Mean density...... ρ (ρ) 1.748 ± 0.074 ... ...
Logarithmic surface gravity......... log g (cgs) 4.569 ± 0.018 ± 0.002 4.45 ± 0.20 4.56 ± 0.02 ...
Age...... (Gyr) ... 7.9 ± 3.8 ...

Planetary parameters
Mass...... Mp (MJup) 0.492 ± 0.023 ± 0.005 0.53 ± 0.07 0.487 ± 0.018 0.526 ± 0.019
Radius...... Rp (RJup) 0.990 ± 0.022 ± 0.005
Mean density...... ρp (ρJup) 0.475 ± 0.026 ± 0.002 0.594 ± 0.052
Surface gravity...... gp (m s-2) 12.45 ± 0.50 12.02 ± 0.83 ...
Equilibrium temperature...... Teq (K) 992 ± 14 960 ± 70 1020 ± 17
Safronov number...... Θ 0.0539 ± 0.0019 ± 0.0003 ... 0.053 ± 0.002 ...

Orbital parameters
Time of mid-transit...... T0 (BJDTDB) 2 454 729.90716
± 0.00020
2 454 473.05588
± 0.00020
2 454 759.68683
± 0.00016
2 454 808.07904
± 0.00012
Period...... Porb (days) 3.72247967
± 0.00000045
3.722465
± 0.000007
3.7224747
± 0.0000065
3.72247669
± 0.00000181
Semi-major axis...... a (au) 0.04375
± 0.00070 ± 0.00023
0.043 ± 0.002 0.0435 ± 0.0006 0.04473 ± 0.00024
Inclination...... i (degree) 89.03 ± 0.34
RV curve semi-amplitude...... KA (m s-1) 82.7 ± 4.2a 82.1 ± 7.4 74.5 ± 1.8
Barycentric RV...... γ (km s-1) 4.8951 ± 0.0021 4.9077 ± 0.0015 3.95 ± 0.43 ...
Proj. spin-orbit angle...... λ (degree) 7 ± 5 ... ... ...

Notes. Where two errorbars are given, the first refers to the statistical uncertainties and the second to the systematic errors.

(a)

This value of KA was determined from our RV data, which were taken during transit time only. The value reported by Bakos et al. (2009), which is based on RV data with a much better coverage of the orbital phase, was therefore preferred for the determination of the other physical parameters of the system (see Sect. 5).

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