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Abbott, B. [Author]; Abbott, R. [Author]; Adhikari, R. [Author]; Ageev, A. [Author]; Allen, B. [Author]; Amin, R. [Author]; Anderson, S.B. [Author]; Anderson, W.G. [Author]; Araya, M. [Author]; Armandula, H. [Author]; Asiri, F. [Author]; Aufmuth, P. [Author]; Aulbert, C. [Author]; Babak, S. [Author]; Balasubramanian, R. [Author]; Ballmer, S. [Author]; Barish, B.C. [Author]; Barker, D. [Author]; Barker-Patton, C. [Author]; Barnes, M. [Author]; Barr, B. [Author]; Barton, M.A. [Author]; Bayer, K. [Author]; Beausoleil, R. [Author]; [...]

First upper limits from LIGO on gravitational wave bursts - [published Version]

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  • Media type: E-Article; Text
  • Title: First upper limits from LIGO on gravitational wave bursts
  • Contributor: Abbott, B. [Author]; Abbott, R. [Author]; Adhikari, R. [Author]; Ageev, A. [Author]; Allen, B. [Author]; Amin, R. [Author]; Anderson, S.B. [Author]; Anderson, W.G. [Author]; Araya, M. [Author]; Armandula, H. [Author]; Asiri, F. [Author]; Aufmuth, P. [Author]; Aulbert, C. [Author]; Babak, S. [Author]; Balasubramanian, R. [Author]; Ballmer, S. [Author]; Barish, B.C. [Author]; Barker, D. [Author]; Barker-Patton, C. [Author]; Barnes, M. [Author]; Barr, B. [Author]; Barton, M.A. [Author]; Bayer, K. [Author]; Beausoleil, R. [Author]; [...]
  • imprint: College Park, MD : American Physical Society, 2004
  • Published in: Physical Review D - Particles, Fields, Gravitation and Cosmology 69 (2004), Nr. 10 ; Physical Review D - Particles, Fields, Gravitation and Cosmology
  • Issue: published Version
  • Language: English
  • DOI: https://doi.org/10.15488/12090; https://doi.org/10.1103/PhysRevD.69.102001
  • ISSN: 1550-7998
  • Keywords: search ; network ; laser
  • Origination:
  • Footnote: Diese Datenquelle enthält auch Bestandsnachweise, die nicht zu einem Volltext führen.
  • Description: We report on a search for gravitational wave bursts using data from the first science run of the Laser Interferometer Gravitational Wave Observatory (LIGO) detectors. Our search focuses on bursts with durations ranging from 4 to 100 ms, and with significant power in the LIGO sensitivity band of 150 to 3000 Hz. We bound the rate for such detected bursts at less than 1.6 events per day at a 90% confidence level. This result is interpreted in terms of the detection efficiency for ad hoc waveforms (Gaussians and sine Gaussians) as a function of their root-sum-square strain hrss; typical sensitivities lie in the range hrss∼10−19–10−17strain/√Hz, depending on the waveform. We discuss improvements in the search method that will be applied to future science data from LIGO and other gravitational wave detectors. © 2004 The American Physical Society.
  • Access State: Open Access