Retrieving wind properties from the ultra-hot dayside of WASP-189 b with CRIRES+

Open Access

Fig. 3

Model spectra (top), cross-correlation functions (CCFs, middle), and K_p-v_offset maps (bottom) of CO, Fe and H₂O. The dashed lines in the middle panels indicate the expected course of the planetary trail (which is located between the two lines). The signals of CO and Fe are visible in the CCFs and K_p-v_offset maps, while H₂O was not detectable.

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