Targeted PTA searches for CWs from 114 AGN in NANOGrav 15 yr data yield no detections, factor-of-two tighter limits than all-sky searches, and updated constraints ruling out part of the parameter space for a binary in 3C 66B.
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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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The NANOGrav 15 yr Data Set: Targeted Searches for Supermassive Black Hole Binaries
Targeted PTA searches for CWs from 114 AGN in NANOGrav 15 yr data yield no detections, factor-of-two tighter limits than all-sky searches, and updated constraints ruling out part of the parameter space for a binary in 3C 66B.
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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.