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The masses of neutron stars in neutron star binaries are observed to fall ina narrow mass range around $\sim 1.33$ M$_{\odot}$. We explore the advantage offocusing on this region of the parameter space in gravitational wave searches.We find that an all-sky (externally triggered) search with optimally reducedtemplate bank is expected to detect $14\%$ ($61\%$) more binary mergers thanwithout the reduction. A reduced template bank can also represent significantimprovement in technical cost. We also develop a more detailed search methodusing binary mass distribution, and find similar sensitivity increase to thatdue to the reduced template bank.

Beyond the Horizon Distance: LIGO-Virgo can Boost Gravitational Wave Detection Rates by Exploiting the Mass Distribution of Neutron Stars