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Table B.1.

Star-planet systems with a quasi-circular and quasi-coplanar orbit, e <  0.1 and |λ| < 30° with e and λ the eccentricity and the sky-projected spin-orbit misalignment angle, respectively.

Systems M [M] age [Gyr] R [R] Po [d] P [d] References
CoRoT-11 (b) 1.27 ± 0.05 2.0 ± 1.0 1.43 ± 0.033 2.994325 ± 2.1 × 10−5 1.73 ± 0.22 1
HAT-P-3 (b) 0.917 ± 0.03 1.6 ± 1.3 0.827 ± 0.055 2.899703 ± 5.4 × 10−5 20.2 ± 2.0 2
HAT-P-4 (b) 1.26 ± 0.14 1.27 ± 0.05 3.0565114 ± 2.8 × 10−6 3
HAT-P-8 (b) 1.28 ± 0.04 3.4 ± 1.0 1.5 ± 0.06 3.0763402 ± 1.5 × 10−6 3
HAT-P-9 (b) 1.28 ± 0.13 1.6 ± 1.4 1.4 ± 0.06 3.922814 ± 2 × 10−6 5.61 ± 0.78 4
HAT-P-13 (b) 1.22 ± 0.1 5.0 ± 0.8 1.28 ± 0.079 2.916243 ± 3 × 10−6 3
HAT-P-16 (b) 1.218 ± 0.039 2.0 ± 0.8 1.289 ± 0.066 2.77596 ± 3 × 10−6 3
HAT-P-20 (b) 0.756 ± 0.028 6.7 ± 3.8 0.867 ± 0.033 2.875317 ± 4 × 10−6 14.48 ± 0.02 5, 6
HAT-P-22 (b) 0.916 ± 0.035 12.4 ± 2.6 1.08 ± 0.058 3.21222 ± 9 × 10−6 28.7 ± 0.4 2
HAT-P-24 (b) 1.191 ± 0.042 2.8 ± 0.6 1.242 ± 0.067 3.35524 ± 7 × 10−6 6.67 ± 0.68 4
HAT-P-27 (b) 0.945 ± 0.035 4.4 ± 2.6 1.055 ± 0.036 3.0395803 ± 1.5 × 10−6 17.8 ± 7.8 7
HAT-P-36 (b) 1.022 ± 0.049 6.6 ± 1.8 1.264 ± 0.071 1.327347 ± 3 × 10−6 15.3 ± 0.4 8
HATS-2 (b) 0.882 ± 0.037 9.7 ± 2.9 1.168 ± 0.03 1.354133 ± 1 × 10−6 24.98 ± 0.04 9, 10
HD 149026 (b) 1.3 ± 0.1 2.0 ± 0.8 0.718 ± 0.065 2.8758916 ± 1.4 × 10−6 3
HD 209458 (b) 1.148 ± 0.022 4.0 ± 2.0 1.38 ± 0.018 3.52472 ± 2.82 × 10−5 14.4 ± 2.1 20, 21
KELT-1 (b) 1.335 ± 0.063 1.75 ± 0.25 1.217514 ± 1.5 × 10−5 1.35 ± 0.04 11
Kepler-8 (b) 1.213 ± 0.063 3.84 ± 1.5 1.419 ± 0.058 3.52254 ± 5 × 10−5 7.5 ± 0.3 12
TrES-2 (b) 0.98 ± 0.062 5.1 ± 2.7 1.189 ± 0.025 2.4706133738 ± 1.87 × 10−8 3
TrES-4 (b) 1.388 ± 0.042 2.9 ± 0.3 1.706 ± 0.056 3.5539268 ± 3.2 × 10−6 3
WASP-5 (b) 1.0 ± 0.06 3.0 ± 1.4 1.171 ± 0.057 1.6284246 ± 1.3 × 10−6 16.2 ± 0.4 9
WASP-6 (b) 0.888 ± 0.08 11.0 ± 7.0 3.361006 ± 3.5 × 10−6 23.8 ± 0.15 15
WASP-14 (b) 1.211 ± 0.122 0.75 ± 0.25 2.2437661 ± 1.1 × 10−6 23.68 ± 6.35 4
WASP-16 (b) 1.022 ± 0.101 2.3 ± 2.2 1.008 ± 0.071 3.1186009 ± 1.31 × 10−5 3
WASP-18 (b) 1.24 ± 0.04 0.63 ± 0.53 1.165 ± 0.077 0.9414518 ± 4 × 10−7 5.6 ± 1.11 4
WASP-19 (b) 0.904 ± 0.045 11.5 ± 2.7 1.395 ± 0.025 0.78884 ± 3 × 10−7 11.76 ± 0.09 9, 16
WASP-20 (b) 1.202 ± 0.04 1.459 ± 0.057 4.8996285 ± 3.4 × 10−6 3
WASP-28 (b) 1.021 ± 0.05 1.213 ± 0.042 3.40883 ± 6 × 10−6 3
WASP-52 (b) 0.87 ± 0.03 0.4 ± 0.3 1.27 ± 0.03 1.7497798 ± 1.2 × 10−6 11.8 ± 3.3 18
WASP-111 (b) 1.5 ± 0.11 2.6 ± 0.6 1.442 ± 0.094 2.310965 ± 3.4 × 10−6 8.4 ± 0.7 19

Notes. All the planets are hot Jupiters, denoted (b), and characterised by an orbital period Po found in the http://exoplanet.eu/ catalogue, along with the age, the radius R, and the mass M of the host star. The errors of these parameters (coming from the catalogue) generally refer to 1σ errors (Schneider et al. 2011). The references are for the stellar rotation period P.

References. (1) Gandolfi et al. (2010); (2) Mancini et al. (2018); (3) Brown (2014); (4) Lanza et al. (2011); (5) Esposito et al. (2017); (6) Granata et al. (2014); (7) Anderson et al. (2011); (8) Mancini et al. (2015); (9) Maxted et al. (2015); (10) Mohler-Fischer et al. (2013); (11) Ferraz-Mello et al. (2015); (12) Hirano et al. (2012); (15) Tregloan-Reed et al. (2015); (16) Tregloan-Reed et al. (2013); (18) Hébrard et al. (2013); (19) Anderson et al. (2014); (20) Winn et al. (2005); (21) Czesla et al. (2017).

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