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Fig. 16.

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Marginal distributions of the orbital parameters for the six exoplanets in the HD 10180 dataset obtained with an MCMC sampler. The different datasets analysed are encoded by different colours: the DRS (black dots), our reduction before flux correction (blue dots), after flux correction (orange dots), and after morphological correction (green dots). Each row represents one of the orbital parameters, and each column represents a planet.

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