Physical review. D/Physical review. D. · 2018 · 78 citations · 50 references
Natural SciencesAstronomyPhysicsAstrophysicsGravitationGravityGeneral RelativityGravitational WavesNeutron StarsGravitational Wave AstronomyGravitational Wave Data AnalysisGravitational Wave DetectionGravitational-wave EmissionIsolated Neutron StarsSignalsSpinningUpper Bounds
We report on a new all-sky search for periodic gravitational waves in the frequency band 475-2000 Hz and with a frequency time derivative in the range of -1.0; 0.1 10 -8 Hz=s. Potential signals could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. This search uses the data from Advanced LIGO's first observational run O1. No gravitational-wave signals were observed, and upper limits were placed on their strengths. For completeness, results from the separately published low-frequency search 20-475 Hz are included as well. Our lowest upper limit on worst-case (linearly polarized) strain amplitude h 0 is 4 10 -25 near 170 Hz, while at the high end of our frequency range, we achieve a worst-case upper limit of 1.3 10 -24 . For a circularly polarized source (most favorable orientation), the smallest upper limit obtained is 1.5 10 -25 .
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J. Aasi, B. P. Abbott, R. Abbott et al. · Classical and Quantum Gravity · 2015 · 3.4K citations · Full text
Natural Sciences, Astronomy, Physics +16
Characterization of the LIGO detectors during their sixth science run
J. Aasi, J. Abadie, B. P. Abbott et al. · Classical and Quantum Gravity · 2015 · 1.3K citations · Full text
Natural Sciences, Astronomy, Physics +13
GW150914: The Advanced LIGO Detectors in the Era of First Discoveries
B. P. Abbott, R. Abbott, T. D. Abbott et al. · Physical Review Letters · 2016 · 762 citations · Full text
Natural Sciences, Astronomy, Physics +15