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Fig. 3


Decomposition of our nominal orbital model for GJ3634. The top panel shows RVs with the contribution of the long-term drift subtracted and phased with the planet’s orbital period. The bottom panel shows RVs as a function of time, with the Keplerian contribution removed. Gray points duplicate some of the red points. The model is also decomposed and plotted with a solid curve in each panel.

This figure is made of several images, please see below:

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