GWTC-3 yields BNS merger rates of 10-1700 Gpc^{-3} yr^{-1}, NS-BH rates of 7.8-140, BBH rates of 17.9-44 at z=0.2 with (1+z)^{2.9} evolution, plus mass distributions showing peaks at chirp masses 8.3 and 27.9 solar masses and a sharp drop after the neutron-star maximum mass.
Kalogera, Spin-Orbit Misalignment in Close Binaries with Two Compact Objects, Astrophys
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The population of merging compact binaries inferred using gravitational waves through GWTC-3
GWTC-3 yields BNS merger rates of 10-1700 Gpc^{-3} yr^{-1}, NS-BH rates of 7.8-140, BBH rates of 17.9-44 at z=0.2 with (1+z)^{2.9} evolution, plus mass distributions showing peaks at chirp masses 8.3 and 27.9 solar masses and a sharp drop after the neutron-star maximum mass.