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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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.