Corner plot displaying the results of MCMC analysis on the Wapiti corrected RV time series is presented. This analysis involves fitting a model that consists of an offset γ₀, an RV jitter s (in log), and a Keplerian with parameters including the time of periastron T_b, the orbital period P_b, the semi-amplitude K_b, and the eccentricity and argument of periastron represented by and , respectively.