Fig. B.1.

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Detection of Achernar B from the GRAVITY individual observations in the closure phase signal T3ϕ for each of the four telescope triplets, and amplitude of the fringe visibility |V| for the six baselines. The observations are shown as black curves, and the best-fit model as red curves. The observing dates are given above each panel (see also Fig. 4 and Sect. 2.6 for further details).
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