Cumulative distribution functions of the (left) binary and single star population, (middle) different mass ranges of the single star sample, and (right) different mass ranges of the binary star sample. (For binaries, we use the primary mass of the system.) We also show a p-value in the left panel resulting from a K-S test between the binary and single star samples. Resulting p-values from K-S tests between the highest and lowest mass ranges for the middle and right panel are 7.79 × 10⁻³ and 3.44 × 10⁻⁵, respectively.