Top panel: phase-folded radial velocity curve comprised of radial velocity measurements from this work (ESPRESSO eclipse), ESPRESSO transit observations, and HARPS. The vertical extent of each point represents the error. For the radial velocities to appear as a continuous curve, the systemic velocity and the fitted instrumental offset were subtracted. Bottom panel: phase-folded short-cadence TESS light curve (light points). The darker points show a binned version of the curve. In both panels, the best-fit curve for a circular orbit is shown (orange).