Precomputed inner products make coherent Bayesian gravitational wave searches on astrometric data tractable, yielding Kepler and Roman strain sensitivities around 10^-12.4 and 10^-11.4 from 10 nHz to 1 microHz.
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A Fast Bayesian Method for Coherent Gravitational Wave Searches with Relative Astrometry
Precomputed inner products make coherent Bayesian gravitational wave searches on astrometric data tractable, yielding Kepler and Roman strain sensitivities around 10^-12.4 and 10^-11.4 from 10 nHz to 1 microHz.