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Fig. 4
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Probability density of the posterior samples for the estimated rotational period of the star (Prot) when using a dSHO-GP to fit the WASP (gray, 2008–2014) and ASAS-SN (blue, 2012–2019) data. The posterior distributions for the RVs (orange, 2019–2020) come from the dSHO-GP component in the final joint fit (Sect. 5.3).
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