Activity induced variation in spin-orbit angles as derived from Rossiter–McLaughlin measurements

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Table 3

Details of the priors that we apply during our MCMC analysis.

Parameter	WASP-6b	WASP-19b	WASP-41b	WASP-52b	CoRoT-2b	Qatar-2b

vsini (km s⁻¹)
T₀(JD)

Notes. is a uniform prior with lower and upper limits of a and b; is a normal distribution with mean μ and width σ. Reported T₀ mean is the first transit time for each planet.

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