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All-Sky Search for Long-Duration Gravitational Wave Transients in the First Advanced LIGO Observing Run

  • B. P. Abbott
  • , K. Gill
  • , B. Hughey
  • , J. W. W. Pratt
  • , E. Rhoades
  • , E. Schmidt
  • , S. G. Schwalbe
  • , M. J. Szczepańczyk
  • , M. Zanolin
  • , et al.
  • California Institute of Technology
  • Embry-Riddle Aeronautical University

Research output: Contribution to journalArticlepeer-review

Abstract

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 and , with a total observational time of . 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  ~10−8 in gravitational waves.

Original languageAmerican English
JournalClassical and Quantum Gravity
Volume35
DOIs
StatePublished - Feb 14 2018

Keywords

  • gravitational waves
  • LIGO-Virgo
  • long duration transient

Disciplines

  • Astrophysics and Astronomy
  • Cosmology, Relativity, and Gravity

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