A small set of anchor pulsars with sub-wavelength distance precision can reduce 90% credible sky localization areas to 0.1-9.2 square degrees at SNR 20, enabling host galaxy identification.
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No continuous GW signals detected from eccentric SMBBHs in OJ 287 or nearby clusters; total mass in OJ 287 limited to below 5.25e10 solar masses and high mass-ratio binaries excluded at 10 nHz.
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From Detection to Host Galaxy Identification: Precision Continuous Gravitational Wave Localization with a Few Anchor Pulsars
A small set of anchor pulsars with sub-wavelength distance precision can reduce 90% credible sky localization areas to 0.1-9.2 square degrees at SNR 20, enabling host galaxy identification.
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Targeted search for eccentric supermassive binary black holes in OJ 287 and nearby galaxy clusters with PPTA DR3
No continuous GW signals detected from eccentric SMBBHs in OJ 287 or nearby clusters; total mass in OJ 287 limited to below 5.25e10 solar masses and high mass-ratio binaries excluded at 10 nHz.