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Fig. G.1.

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Likelihood, prior and posterior of our Bayesian model. In the absence of the prior (top panel), our model is intentionally designed to be independent of both radius and direct magnitudes. However, this changes when the prior (middle panel) is introduced (bottom panel). Then the radial trend becomes visible, and the RC stars are classified as late-type. All plots use the same colour scale for p_late.

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