Fig. 7
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Top: phase-folded ESPRESSO RVs (blue dots), HARPS RVs (orange diamonds), and median Keplerian model (black line) from the pyaneti 2c fit for the inner candidate planet TOI-2322.02 (left) and outer candidate planet TOI-2322.01 (right). The shaded grey regions show the 1σ and 2σ confidence intervals. Bottom: residuals to the fit.
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