Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO-Virgo data
We present a directed search for continuous gravitational wave (CW) signals emitted by spinning neutron stars located in the inner parsecs of the Galactic Center (GC). Compelling evidence for the presence of a numerous population of neutron stars has been reported in the literature, turning this reg...
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Format: | Article |
Language: | English |
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American Physical Society
2024
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Online Access: | https://hdl.handle.net/1721.1/154861 |