Fig. I.2
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Left: Kp−Δυsys maps for the iron signal using the phase-dependent retrieval setup. Right: The retrieved planetary orbital velocity (υp) of the detected species for the pre-eclipse data alone, computed from 10,000 random samples of the MCMC. The dashed lines show the median value, and the shaded regions show the 1σ and 2σ contours (see Sect. 5.3).
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