The NANOGrav 15 yr Dataset: Targeted Searches for Supermassive Black Hole Binaries
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Abstract
Abstract We present the first targeted searches for continuous gravitational waves (CWs) from 114 active galactic nuclei that may host supermassive black hole binaries, using the NANOGrav 15 yr dataset. By incorporating electromagnetic priors on sky location, distance, redshift, and CW frequency, our strain and chirp-mass upper limits are typically improved by a factor of ∼2 (median 2.2) relative to all-sky limits at the same frequency. Bayesian comparisons against a model including only a Hellings–Downs-correlated background disfavors a CW signal for all targets, with a mean Bayes factor of 0.73 ± 0.32. Two targets have Bayes factors slightly above unity, but coherence tests, random-targeting experiments, and…
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Keywords
- Pulsar
- Gravitational wave
- Supermassive black hole
- Binary black hole
- Bayes factor
- Prior probability
- Bayesian probability
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