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Fig. 6
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Phase-folded radial velocity curves (top) from HARPS (grey dots) and PFS (blue dots) measurements. The best-fit model of the Keplerian signal is plotted in black for HD 15337 b (left) and HD 15337 c (right). The bottom panel shows the residuals of the best-fit model as in Fig. 4. We over-plot the binned data and residuals.
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