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Fig. C.1
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L1 periodogram of the full dataset of RVs for HD20794. We see the most significant peaks at 18.3 d, 89.6 d, and 646 d. These peaks correspond to the planets b, c, and d we are seeing in our analysis. We see other peaks at ~ 85 d and 1027 d. These peaks appear in our analysis but we cannot claim those as new detections.
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