期刊
CLASSICAL AND QUANTUM GRAVITY
卷 33, 期 13, 页码 -出版社
IOP Publishing Ltd
DOI: 10.1088/0264-9381/33/13/134001
关键词
gravitational waves; detector characterization; GW150914
类别
资金
- Australian Research Council
- Council of Scientific and Industrial Research of India
- Department of Science and Technology, India
- Science AMP
- Engineering Research Board (SERB), India
- Ministry of Human Resource Development, India
- Spanish Ministerio de Economia y Competitividad
- Conselleria d'Economia i Competitivitat of the Govern de les Illes Balears
- Conselleria d'Educacio Cultura i Universitats of the Govern de les Illes Balears
- National Science Centre of Poland
- European Commission
- Royal Society
- Scottish Funding Council
- Scottish Universities Physics Alliance
- Hungarian Scientific Research Fund (OTKA)
- Lyon Institute of Origins (LIO)
- National Research Foundation of Korea
- Industry Canada
- Province of Ontario through the Ministry of Economic Development and Innovation
- Natural Science and Engineering Research Council Canada
- Canadian Institute for Advanced Research
- Brazilian Ministry of Science, Technology, and Innovation
- Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP)
- Russian Foundation for Basic Research
- Leverhulme Trust
- Research Corporation
- Ministry of Science and Technology (MOST), Taiwan
- Kavli Foundation
- Science and Technology Facilities Council [PPA/G/S/2002/00652, ST/L000946/1, ST/K005014/1, ST/L003465/1, ST/N000633/1, ST/I006269/1 Gravitational Waves, ST/J000019/1, ST/N005716/1, ST/H002006/1, ST/J00166X/1, ST/N000080/1, ST/N005406/1, ST/M004090/1, ST/K000845/1, ST/I006242/1, ST/N000072/1, ST/I006285/1, ST/N005430/1, ST/L000954/1, Gravitational Waves, ST/N000064/1, ST/I006269/1, ST/N00003X/1] Funding Source: researchfish
- STFC [ST/L000946/1, ST/N000072/1, ST/N005716/1, ST/J00166X/1, ST/J000019/1, ST/L000954/1, ST/I006242/1, ST/M004090/1, ST/N00003X/1, PPA/G/S/2002/00652, Gravitational Waves, ST/I006285/1, ST/N000080/1, ST/H002006/1, ST/K000845/1, ST/N005430/1, ST/I006269/1, ST/N000633/1, ST/N005406/1, ST/N000064/1, ST/L003465/1, PP/C505791/1, ST/K005014/1] Funding Source: UKRI
- Direct For Computer & Info Scie & Enginr
- Office of Advanced Cyberinfrastructure (OAC) [1443047] Funding Source: National Science Foundation
- Direct For Education and Human Resources
- Division Of Human Resource Development [1242090] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Physics [1505524, 1404395, 1204371, 1506497, 1505629, 1125897, 1505373, 1307020, 1307401, 1307429, 1404139, 1205882, 1255650] Funding Source: National Science Foundation
- Division Of Physics
- Direct For Mathematical & Physical Scien [1305864, 1205512, 1505779, 1607585, 1505308, 1151836, 1104371, 1207010, 1506254, 1506360] Funding Source: National Science Foundation
On 14 September 2015, a gravitational wave signal from a coalescing black hole binary system was observed by the Advanced LIGO detectors. This paper describes the transient noise backgrounds used to determine the significance of the event (designated GW150914) and presents the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around the time of the event. The detectors were operating nominally at the time of GW150914. We have ruled out environmental influences and non-Gaussian instrument noise at either LIGO detector as the cause of the observed gravitational wave signal.
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