4.4 Article

First joint search for gravitational-wave bursts in LIGO and GEO 600 data

期刊

CLASSICAL AND QUANTUM GRAVITY
卷 25, 期 24, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/25/24/245008

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资金

  1. United States National Science Foundation for the construction and operation of the LIGO Laboratory
  2. Science and Technology Facilities Council of the United Kingdom
  3. Max-Planck-Society
  4. State of Niedersachsen/Germany
  5. Australian Research Council
  6. Council of Scientific and Industrial Research of India
  7. Istituto Nazionale di Fisica Nucleare of Italy
  8. Spanish Ministerio de Educacion y Ciencia
  9. Conselleria d'Economia
  10. Hisenda i Innovacio of the Govern de les Illes Balears
  11. Royal Society
  12. Scottish Funding Council
  13. Scottish Universities Physics Alliance
  14. National Aeronautics and Space Administration
  15. Carnegie Trust
  16. Leverhulme Trust
  17. David and Lucile Packard Foundation
  18. Research Corporation
  19. Alfred P Sloan Foundation
  20. LIGO Laboratory [LIGO-P080008-B-Z]
  21. STFC [PP/F001096/1, PP/F001118/1, ST/G504284/1, PP/F00110X/1, PP/E001203/1] Funding Source: UKRI
  22. Science and Technology Facilities Council [PP/E001203/1, ST/G504284/1, PP/F001118/1, PP/F00110X/1, PP/F001096/1] Funding Source: researchfish
  23. Division Of Physics
  24. Direct For Mathematical & Physical Scien [0757058] Funding Source: National Science Foundation

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We present the results of the first joint search for gravitational-wave bursts by the LIGO and GEO 600 detectors. We search for bursts with characteristic central frequencies in the band 768-2048 Hz in the data acquired between 22 February and 23 March, 2005 (fourth LSC Science Run-S4). We discuss the inclusion of the GEO 600 data in the Waveburst-CorrPower pipeline that first searches for coincident excess power events without taking into account differences in the antenna responses or strain sensitivities of the various detectors. We compare the performance of this pipeline to that of the coherent Waveburst pipeline based on the maximum likelihood statistic. This likelihood statistic is derived from a coherent sum of the detector data streams that takes into account the antenna patterns and sensitivities of the different detectors in the network. We find that the coherent Waveburst pipeline is sensitive to signals of amplitude 30-50% smaller than the Waveburst-CorrPower pipeline. We perform a search for gravitational-wave bursts using both pipelines and find no detection candidates in the S4 data set when all four instruments were operating stably.

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