Simulated joint aLIGO plus Fermi/GBM catalogs show that about 8 GW detections and 571 short GRBs measure the BNS merger rate density to roughly 50% out to z=1 and constrain the sGRB-to-merger ratio eta to 45%.
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A systematic study of binary neutron star merger rate density history using simulated gravitational wave and short gamma-ray burst observations
Simulated joint aLIGO plus Fermi/GBM catalogs show that about 8 GW detections and 571 short GRBs measure the BNS merger rate density to roughly 50% out to z=1 and constrain the sGRB-to-merger ratio eta to 45%.