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Fig. 2

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Examples of data plots at three different points in the analysis. (a) Top panel: exposures are stacked along the vertical axis in time (where orbital phase ϕ = 1.0 is the middle of the primary eclipse). The dotted white lines indicate before and after the transit. (b) Middle panel: Kpυsys detection map, where all values have been shifted into the planetary rest frame. The white dotted lines indicate rest frame system velocity (υsys = 0 km s−1) and the semi-amplitude of the radial velocity of the planet (Kp = 126 km s−1). (c) Bottom panel: example of what the cross-correlation function looks like at Kp = 126 km s−1, i.e. at the horizontal white line from (b).

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