A frequentist CGW search method with non-parametric red noise suppression and optimal pulsar selection achieves Bayesian-comparable accuracy on NANOGrav-based simulations at far lower computational cost.
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Scalable continuous gravitational wave detection in PTA data with non-parametric red noise suppression and optimal pulsar selection
A frequentist CGW search method with non-parametric red noise suppression and optimal pulsar selection achieves Bayesian-comparable accuracy on NANOGrav-based simulations at far lower computational cost.