Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/120852
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Type: Journal article
Title: All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data
Author: Abbott, B.
Abbott, R.
Abbott, T.
Acernese, F.
Ackley, K.
Adams, C.
Adya, V.
Affeldt, C.
Agathos, M.
Agatsuma, K.
Aggarwal, N.
Aguiar, O.
Aiello, L.
Ain, A.
Ajith, P.
Allen, G.
Altin, P.
Amato, A.
Ananyeva, A.
Anderson, S.
et al.
Citation: Physical Review D, 2019; 100(2)
Publisher: American Physical Society
Issue Date: 2019
ISSN: 2470-0010
2470-0029
Statement of
Responsibility: 
B. P. Abbott, R. Abbott, T. D. Abbott, S. Abraham, F. Acernese ... P. J. Veitch ... et al. (LIGO Scientific Collaboration and Virgo Collaboration)
Abstract: We present results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast spinning neutron stars with an asymmetry around their rotation axis, using data from the second observing run of the Advanced LIGO detectors. Three different semicoherent methods are used to search in a gravitational-wave frequency band from 20 to 1922 Hz and a first frequency derivative from −1×10−8 to 2×10−9  Hz/s. None of these searches has found clear evidence for a CW signal, so upper limits on the gravitational-wave strain amplitude are calculated, which for this broad range in parameter space are the most sensitive ever achieved.
Rights: © 2019 American Physical Society.
RMID: 0030121070
DOI: 10.1103/PhysRevD.100.024004
Appears in Collections:Physics publications

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