Fig. 2.

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RV time series data for HD 114082. FEROS data from RVSPY are shown as black circles. The RVs computed from the publicly available HARPS spectra are shown as gray circles. Error bars account for the suspected activity jitter (see text for details). The solid gray line shows the best-fit model (see parameters in Table 2), and the vertical blue line indicates the time of the observed transit. The lower panel shows the residuals of the fit.
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