Low-latency template-bank estimates of binary neutron star chirp mass are biased by less than about 10^-3 solar masses even when the true signals contain spins, misalignment, and tides that the search templates ignore.
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The reliability of the low-latency estimation of binary neutron star chirp mass
Low-latency template-bank estimates of binary neutron star chirp mass are biased by less than about 10^-3 solar masses even when the true signals contain spins, misalignment, and tides that the search templates ignore.