4.4 Article

All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run

期刊

CLASSICAL AND QUANTUM GRAVITY
卷 35, 期 6, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.1088/1361-6382/aaab76

关键词

LIGO-Virgo; gravitational waves; long duration transient

资金

  1. Australian Research Council
  2. Council of Scientific and Industrial Research of India
  3. Department of Science and Technology, India
  4. Science AMP
  5. Engineering Research Board (SERB), India
  6. Ministry of Human Resource Development, India
  7. Spanish Agencia Estatal de Investigacion
  8. Vicepresidencia i Conselleria d'Innovacio, Recerca i Turisme
  9. Conselleria d'Educacio i Universitat del Govern de les Illes Balears
  10. Conselleria d'Educacio, Investigacio, Cultura i Esport de la Generalitat Valenciana
  11. National Science Centre of Poland
  12. Swiss National Science Foundation (SNSF)
  13. Russian Foundation for Basic Research
  14. Russian Science Foundation
  15. European Commission
  16. European Regional Development Funds (ERDF)
  17. Royal Society
  18. Scottish Funding Council
  19. Scottish Universities Physics Alliance
  20. Hungarian Scientific Research Fund (OTKA)
  21. Lyon Institute of Origins (LIO)
  22. Paris Ile-de-France Region
  23. National Research, Development and Innovation Office Hungary (NKFI)
  24. National Research Foundation of Korea
  25. Industry Canada
  26. Province of Ontario through the Ministry of Economic Development and Innovation
  27. Natural Science and Engineering Research Council Canada
  28. Canadian Institute for Advanced Research
  29. Brazilian Ministry of Science, Technology, Innovations, and Communications
  30. International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR)
  31. Research Grants Council of Hong Kong
  32. National Natural Science Foundation of China (NSFC)
  33. Leverhulme Trust
  34. Ministry of Science and Technology (MOST), Taiwan
  35. Kavli Foundation
  36. EGO consortium
  37. Science and Technology Facilities Council [ST/P000258/1, ST/I000887/1, ST/N000080/1, 1096295, ST/N005406/1, ST/R000336/1, ST/L000954/1 Gravitational Waves, ST/M006735/1, 1366891, 1654298, ST/K000845/1, ST/I001085/1, ST/L003465/1, ST/N000064/1, Gravitational Waves, ST/N005430/1, ST/K000365/1, ST/I001085/1 Gravitational Waves, ST/I000887/1 Gravitational Waves, PP/F001118/1, ST/I006242/1, ST/N005422/1, ST/L000946/1, PPA/G/S/2002/00652, 1653071, ST/I006269/1, ST/N005406/2, ST/J000019/1 Gravitational Waves, ST/I006277/1, ST/N000633/1, ST/I006242/1 Gravitational Waves, ST/L000954/1, ST/J000019/1, ST/N000072/1, ST/I006285/1, ST/G504284/1, ST/J000345/1, ST/H002006/1, ST/J000361/1, PP/F001096/1, ST/N005481/1, ST/L000911/1, ST/J00166X/1, ST/N00003X/1, ST/I000291/1, 1573115, ST/N005716/1] Funding Source: researchfish
  38. Direct For Mathematical & Physical Scien [1455090] Funding Source: National Science Foundation
  39. Division Of Physics [1607709, 1606654, 1607585, 1404139] Funding Source: National Science Foundation
  40. STFC [Gravitational Waves, ST/J00166X/1, ST/K005014/2, ST/N005406/1, ST/K000365/1, ST/N005430/1, ST/N005422/1, ST/I006277/1, ST/J000361/1, 1653071, ST/N00003X/1, ST/I006242/1, 1653089, ST/L000946/1, ST/N005716/1, ST/K005014/1, ST/M000931/1, 1654298, ST/N000064/1, ST/L000911/1, PP/F001096/1, ST/J000345/1, ST/G504284/1, PPA/G/S/2002/00652, ST/L000954/1, ST/I006269/1, ST/J000019/1, ST/I001085/1, ST/I006285/1, ST/N000633/1, ST/N005406/2, ST/R000336/1, 2142081, ST/N000080/1, ST/N005481/1, ST/H002006/1, PP/F001118/1, ST/K000845/1, ST/M006735/1, ST/I000887/1, ST/L003465/1, ST/N000072/1, ST/P000258/1] Funding Source: UKRI

向作者/读者索取更多资源

We present the results of a search for long-duration gravitational wave transients in the data of the LIGO Hanford and LIGO Livingston second generation detectors between September 2015 and January 2016, with a total observational time of 49 d. The search targets gravitational wave transients of 10-500 s duration in a frequency band of 24-2048 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. No significant events were observed. As a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. We also show that the search is sensitive to sources in the Galaxy emitting at least similar to 10-8 M(circle dot)c(2) in gravitational waves.

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