Gaussian fits for M35 for stars within a 0.°5 radius from the cluster center. These fits for the RV (top), distance (middle), and PM (bottom) distributions are shown in pink, where vertical dotted lines represent the mean of the Gaussian fit. Dashed purple lines indicate the Gaussian fit to the field RV data (top) and a sixth-order polynomial fit to the field star distances (middle). Combined fits are represented by gray curves in the top and middle plots.