Figure 2.
(a) HARPS RV variations in the solar rest frame, corrected for relativistic Doppler effects (but not yet corrected for Vesta's axial rotation). (b) HARPS RV variations of the Sun as a star (after removing the RV contribution of Vesta's axial rotation). (c) Nightly binned HARPS RV variations of the Sun as a star – note the change in scale on the y-axis. The values for each time series are provided in the Supplementary Files that are available online.