All of the RVs used in our analysis. Each data set shown is mean-subtracted to highlight the relative changes in RV of the star. We have also subtracted the etalon drift slope and offsets (calibrated using those from HD 3651; see Section 4.1 for more details) from the MAROON-X data. Our MAROON-X data have a much smaller scatter than the data from other instruments, indicating that our MAROON-X data will provide much more constraining power than previous observations.