Rossiter-McLaughlin effect measurements for WASP-16, WASP-25 and WASP-31?

We present new measurements of the Rossiter-McLaughlin (RM) effect for three WASP planetary systems, WASP-16, WASP-25 and WASP-31, from a combined analysis of their complete sets of photometric and spectroscopic data. We find a low amplitude RM effect for WASP-16 (T eff = 5700 ± 150 K), suggesting that the star is a slow rotator and thus of an advanced age, and obtain a projected alignment angle of λ = −4.2◦+11.0−13.9. For WASP-25 (T eff = 5750±100 K) we detect a projected spin-orbit angle of λ = 14.6◦ ± 6.7. WASP-31 (T eff = 6300 ± 100 K) is found to be well-aligned, with a projected spin-orbit angle of λ = 2.8◦±3.1. A circular orbit is consistent with the data for all three systems, in agreement with their respective discovery papers. We consider the results for these systems in the context of the ensemble of RM measurements made to date. We find that whilst WASP-16 fits the hypothesis of Winn et al. (2010) that ‘cool ’ stars (T eff < 6250 K) are preferentially aligned, WASP-31 has little impact on the proposed trend. We bring the total distribution of the true spin-orbit alignment angle, ψ, up to date, noting that recent results have improved the agreement with th