All-sky search for long-duration gravitational wave transients with initial LIGO

Research output: Contribution to journal › Article › Research › peer review

Authors

  • The LIGO Scientific Collaboration
  • The Virgo Collaboration
  • Karsten Danzmann
  • Michele Heurs
  • Fumiko Kawazoe
  • Harald Lück
  • Daniel Steinmeyer
  • Henning Fedor Cornelius Vahlbruch
  • Benno Willke
  • Holger Wittel
  • Bruce Allen
  • Peter Aufmuth
  • A. Bisht
  • Timo Denker
  • Stefan Kaufer
  • Christian Krüger
  • J. D. Lough
  • A. Sawadsky
  • Dirk Schütte

Research Organisations

External Research Organisations

  • California Institute of Caltech (Caltech)
  • Louisiana State University
  • Universita di Salerno
  • Monte S. Angelo University Federico II
  • University of Florida
  • Universite de Savoie
  • University of Sannio
  • Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • National Institute for Subatomic Physics (Nikhef)
  • LIGO Laboratory
  • Instituto Nacional de Pesquisas Espaciais
  • Inter-University Centre for Astronomy and Astrophysics India
  • Tata Institute of Fundamental Research (TIFR HYD)
  • Carson College of Business
  • University of Birmingham
  • University of Glasgow
  • Seoul National University
  • Carleton College
  • Australian National University
  • University of Melbourne
  • Tsinghua University
  • University of Western Australia
  • Observatoire de la Côte d’Azur (OCA)
  • Rochester Institute of Technology
  • Northwestern University
  • University of Wisconsin Milwaukee
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Details

Original languageEnglish
Article number042005
JournalPhysical Review D
Volume93
Issue number4
Publication statusPublished - 12 Feb 2016

Abstract

We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10-500 s in a frequency band of 40-1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; 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. For signals from black hole accretion disk instabilities, we set upper limits on the source rate density between 3.4×10-5 and 9.4×10-4 Mpc-3 yr-1 at 90% confidence. These are the first results from an all-sky search for unmodeled long-duration transient gravitational waves.

ASJC Scopus subject areas

Cite this

All-sky search for long-duration gravitational wave transients with initial LIGO. / The LIGO Scientific Collaboration; The Virgo Collaboration; Danzmann, Karsten et al.
In: Physical Review D, Vol. 93, No. 4, 042005, 12.02.2016.

Research output: Contribution to journal › Article › Research › peer review

The LIGO Scientific Collaboration, The Virgo Collaboration, Danzmann, K, Heurs, M, Kawazoe, F, Lück, H, Steinmeyer, D, Vahlbruch, HFC, Willke, B, Wittel, H, Allen, B, Aufmuth, P, Bisht, A, Denker, T, Kaufer, S, Krüger, C, Lough, JD, Sawadsky, A & Schütte, D 2016, 'All-sky search for long-duration gravitational wave transients with initial LIGO', Physical Review D, vol. 93, no. 4, 042005. https://doi.org/10.1103/PhysRevD.93.042005, https://doi.org/10.15488/12018
The LIGO Scientific Collaboration, The Virgo Collaboration, Danzmann, K., Heurs, M., Kawazoe, F., Lück, H., Steinmeyer, D., Vahlbruch, H. F. C., Willke, B., Wittel, H., Allen, B., Aufmuth, P., Bisht, A., Denker, T., Kaufer, S., Krüger, C., Lough, J. D., Sawadsky, A., & Schütte, D. (2016). All-sky search for long-duration gravitational wave transients with initial LIGO. Physical Review D, 93(4), Article 042005. https://doi.org/10.1103/PhysRevD.93.042005, https://doi.org/10.15488/12018
The LIGO Scientific Collaboration, The Virgo Collaboration, Danzmann K, Heurs M, Kawazoe F, Lück H et al. All-sky search for long-duration gravitational wave transients with initial LIGO. Physical Review D. 2016 Feb 12;93(4):042005. doi: 10.1103/PhysRevD.93.042005, 10.15488/12018
The LIGO Scientific Collaboration ; The Virgo Collaboration ; Danzmann, Karsten et al. / All-sky search for long-duration gravitational wave transients with initial LIGO. In: Physical Review D. 2016 ; Vol. 93, No. 4.
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abstract = "We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10-500 s in a frequency band of 40-1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; 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. For signals from black hole accretion disk instabilities, we set upper limits on the source rate density between 3.4×10-5 and 9.4×10-4 Mpc-3 yr-1 at 90% confidence. These are the first results from an all-sky search for unmodeled long-duration transient gravitational waves.",
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T1 - All-sky search for long-duration gravitational wave transients with initial LIGO

AU - The LIGO Scientific Collaboration

AU - The Virgo Collaboration

AU - Abbott, B. P.

AU - Abbott, R.

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AU - Abernathy, M. R.

AU - Acernese, F.

AU - Ackley, K.

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AU - Adams, T.

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AU - Agatsuma, K.

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AU - Ain, A.

AU - Ajith, P.

AU - Bose, S.

AU - Brown, D. D.

AU - Chen, Y.

AU - Danilishin, S. L.

AU - Danzmann, Karsten

AU - Fricke, T. T.

AU - Hanke, M. M.

AU - Hennig, J.

AU - Heurs, Michele

AU - Kawazoe, Fumiko

AU - Lee, H. K.

AU - Lück, Harald

AU - Luo, J.

AU - Nguyen, T. T.

AU - Schmidt, J.

AU - Schmidt, P.

AU - Shaltev, M.

AU - Steinmeyer, Daniel

AU - Sun, L.

AU - Vahlbruch, Henning Fedor Cornelius

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AU - Wang, X.

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AU - Willke, Benno

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AU - Zhang, L.

AU - Zhang, Y.

AU - Zhou, M.

AU - Allen, Bruce

AU - Aufmuth, Peter

AU - Bisht, A.

AU - Denker, Timo

AU - Kaufer, Stefan

AU - Krüger, Christian

AU - Lough, J. D.

AU - Sawadsky, A.

AU - Schütte, Dirk

PY - 2016/2/12

Y1 - 2016/2/12

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AB - We present the results of a search for long-duration gravitational wave transients in two sets of data collected by the LIGO Hanford and LIGO Livingston detectors between November 5, 2005 and September 30, 2007, and July 7, 2009 and October 20, 2010, with a total observational time of 283.0 days and 132.9 days, respectively. The search targets gravitational wave transients of duration 10-500 s in a frequency band of 40-1000 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. All candidate triggers were consistent with the expected background; 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. For signals from black hole accretion disk instabilities, we set upper limits on the source rate density between 3.4×10-5 and 9.4×10-4 Mpc-3 yr-1 at 90% confidence. These are the first results from an all-sky search for unmodeled long-duration transient gravitational waves.

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