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Fig. 1

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Radial velocity data (red circles). The solid black line shows the fit to the acquired radial velocity data by assuming the period obtained by the Kepler team (Batalha et al. 2013) and the small eccentricity derived in Lillo-Box et al. (2014b) using the light-curve modulations (REB). The dotted line represents the independent curve obtained by using the parameters extracted from Lillo-Box et al. (2014b), using the REB modulations.

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