Fig. 5
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Observed TTVs and TTVFaster/Ultranest TTV models for each of the three planets. Coloured lines show the median best-fit TTV models, while coloured regions show 1 -σ range. The predicted transit time for the low S/N SAINT-EX observation of planet d is shown as a triangle with white edges, while the observed transit time is shown with dark-edged inverted triangles. Planned TESS observations of the two planets in 2022 are shown in light green.
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