Extended Data Fig. 2: ESPRESSO radial velocities of WASP-76.
From: Nightside condensation of iron in an ultrahot giant exoplanet
a, Stellar radial velocities (RV; blue points) and the maximum-likelihood fit using values from Extended Data Table 3. The transit occurs at the inferior conjunction (0 h). In-transit data have been removed as they are affected by the Rossiter–McLaughlin effect and the atmospheric absorption from the planet. b, Residuals of the radial velocities after subtraction of the maximum-likelihood fit. The standard deviation of the residuals is about 2.8 m s−1. Error bars correspond to 1σ uncertainties and include both parameterized noise terms.
