JournalPhysical Review D (2470-0010), 106, 042003 ~ -
Enrollment typeSCIE
publication date 20220809
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 region into a very interesting place to look for CWs.
