Fig. 4

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Significance analysis of potential H2O signals, illustrated for the night of 31 March 2022. Top panel: S/N map as a function of radial velocity in the exoplanet’s rest frame (vrest, horizontal axis) and the projected orbital velocity semi-amplitude, Kp (vertical axis). Horizontal lines mark the expected Kp, and vertical lines show the zero rest-frame velocity. Bottom panel: 1D cross-correlation function at the expected Kp (97.1 kms−1)of GJ 1214b.
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