Fig. 3

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CC both in the S/N (top panel) and in the significance (middle panel) framework, and LH confidence intervals (bottom panel) maps for each investigated molecule as a function of the planet’s maximum RV (KP) and the planet’s rest-frame velocity (Vrest). The dotted lines denote the expected RV semi-amplitude of WASP-69b in the planet rest frame (Vrest = 0 km s−1). The detection significance increased when transits were co-added.
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