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Table 5

Comparative table of all Rossiter-McLaughlin effects published and parameters.

Planet Rp (RJ) Mp (MJ) e P (day) i (°) β (°) VsinI (km s-1) References

HD 17156b  − 9.4 ± 9.3 6.3 ± 1.1 Cochran et al. (2008); Gillon et al. (2008)
HD 80606b 0.9 ± 0.1 4.0 ± 0.3 0.934 ± 0.003 111.436 ± 0.003 89.6 ± 0.4 2.2 Moutou et al. (2009); Winn et al. (2009a)
HD 147506b 5.63341 ± 0.00013 Loeillet et al. (2008)
HD 149026b 0.718 ± 0.065 0.352 ± 0.025 0 86.1 ± 1.4 12 ± 15 Wolf et al. (2007)
HD 189733b Triaud et al. (2009)
HD 209458b 1.355 ± 0.002 0.657 ± 0.006 0.0147 ± 0.0053 3.52474859 ± 0.00000038 86.55 ± 0.03 4.4 ± 1.4 4.70 ± 0.16 Winn et al. (2005); Knutson et al. (2007)
XO-3b 1.5 ± 0.2 12.5 ± 1.9 0.2884 ± 0.0035 3.19161 ± 0.00014 82.5 ± 1.5  − 37.3 ± 3.7 18.31 ± 1.3 Hébrard et al. (2008); Winn et al. (2009c)
HAT-P-1b 1.225 ± 0.059 0.524 ± 0.031 0 4.4652934 ± 0.0000093 86.28 ± 0.20  − 3.7 ± 2.1 3.75 ± 0.58 Johnson et al. (2008)
HAT-P-7b 0 2.2047304 ± 0.0000024  − 182.5 ± 9.4 Pál et al. (2008); Winn et al. (2009b); Narita et al. (2009)
TrES-1b 1.081 ± 0.029 0.61 ± 0.06 0 3.0300722 ± 0.0000002 88.4 ± 0.3  − 30 ± 21 1.3 ± 0.3 Narita et al. (2007)
TrES-2b 1.198 ± 0.053 0 2.470621 ± 0.00017 83.62 ± 0.14 9 ± 12 1.0 ± 0.6 Winn et al. (2008); Daemgen et al. (2009)
TrES-4b 1.674 ± 0.094 0.84 ± 0.10 0 3.553945 ± 0.000075 82.81 ± 0.33  − 7.3 ± 4.6 8.3 ± 1.1 Mandushev et al. (2007); Narita et al. (2010)
CoRoT-1b* 1.49 ± 0.08 1.03 ± 0.12 0 1.5089557 ± 0.0000064 85.1 ± 0.5 77 ± 11 5.2 ± 1.0 Barge et al. (2008); Pont et al. (2010)
CoRoT-2b 1.465 ± 0.029 3.31 ± 0.16 0 1.7429964 ± 0.0000017 87.84 ± 0.10  − 7.1 ± 5.0 Alonso et al. (2008); Bouchy et al. (2008)
CoRoT-3b* Triaud et al. (2009)
Kepler-8b* 0 84.07 ± 0.33 26.9 ± 4.6 10.5 ± 0.7 Jenkins et al. (2010)
WASP-2b 0 This paper
WASP-3b 0 1.846834 ± 0.000002 Pollacco et al. (2008); Tripathi et al. (2010)
WASP-4b 0 This paper
WASP-5b 0 This paper
WASP-6b 0 Gillon et al. (2009a)
WASP-8b Queloz et al. (2010)
WASP-14b 0.0903 ± 0.0027 2.23752 ± 0.000010 33.1 ± 7.4 2.89 ± 0.57 Joshi et al. (2009); Johnson et al. (2009)
WASP-15b 0 This paper
WASP-17b 0 This paper
WASP-18b This paper

Notes. Asterisks show claims of misalignments which remain to be confirmed.

This values is not really a VsinI but more an amplitude parameter for fitting the Rossiter-McLaughlin effect. Please refer to Sect. 4.6 treating WASP-18b.

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