Summary of the double compact object (DCO) rates in our synthetic population at Solar metallicity (Z = 0.0142). We quantify the rates of DCOs (from left to right): NS-NS binaries, BH-BH binaries, and NS-BH binaries. For each column, the upper portion (light pink) indicates non-merging DCOs, the lower column (dark pink) indicates DCOs that merge in a Hubble time, and the hatching indicates DCOs that had a rejuvenated companion before both SNe. The y-axis is scaled as in Fig. 2.