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Fig. 3


Maps of the time-series CCFs as a function of RV relative to the star (in abscissa) and orbital phase (in ordinate). The dashed vertical white lines are marked at ± v sin i, and first and fourth contact of transit is indicated by white diamonds. Upper panel: map of the transit residuals after the model stellar profile was subtracted. The signature of HD 3167 c is the moderately bright feature that is visible from ingress to egress. Middle panel: transiting signature of HD 3167 c using the best-fit model, obtained with λ = − 88°. Lower panel: overall residual map after the model planet signature was subtracted.

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