Detection of the GW of the Crab Pulsar in the LIGO and Virgo O3b series
preprint
OA: closed
Abstract
After compensation for phase modulation and frequency drift, the pulsar's GW can be detected in the records of all three interferometers. The signatures agree with the known values measured with electromagnetic waves.
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- last seen: 2026-05-19T01:45:01.086888+00:00