The GAPS programme with HARPS-N at TNG - XVI. Measurement of the Rossiter–McLaughlin effect of transiting planetary systems HAT-P-3, HAT-P-12, HAT-P-22, WASP-39, and WASP-60

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Table 4

Parameters from the best-fitting models of the RM effect for the five planetary systems.

Object	λ	v sin i_⋆	γ	ΔBIC
	(°)	(km s⁻¹)	(km s⁻¹)
HAT-P-3	21.2 ± 8.7	1.20 ± 0.36	− 23.3849 ± 0.0007	33.5
HAT-P-12			− 40.4589 ± 0.0023	10.3
HAT-P-22	− 2.1 ± 3.0	1.65 ± 0.26	12.6370 ± 0.0004	71.4
WASP-39	0 ± 11	1.40 ± 0.25	− 58.4421 ± 0.0020	19.7
WASP-60	− 129 ± 17	2.97 ± 0.47	− 26.5323 ± 0.0021	19.3

Notes. The Δ BIC values, i.e. the difference between the BIC values calculated from the best-fitting models with and without the RM effect, are also shown.

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