Fig. A.8

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Posterior distribution of the investigated parameters in the DE-MCMC analysis of the He I triplet. The excess of absorption c [%], offset [%], peak position, and FWHM correspond to the parameters we used in the Gaussian fit, while the jitter term σj, the semi-amplitude of the correlated noise h, and the correlation length λ were used to parametrize the SE kernel within the GP.
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