Fig. 2
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HARPS detrended and phase-folded RV time series of TOI-396 b (top panel), TOI-396 c (middle panel), and TOI-396 d (bottom panel) with the Keplerian model superimposed in red. For each planet, the time series were obtained after subtracting the RV contribution of the other planets. The error bars also account for the jitter contribution (displayed in grey).
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