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.

doi:10.1088/1361-6382/aaab76

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.

Physics & Astronomy

Research output: Contribution to journal › Article › peer-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 language	American English
Journal	Classical and Quantum Gravity
Volume	35
DOIs	https://doi.org/10.1088/1361-6382/aaab76
State	Published - Feb 14 2018

Keywords

gravitational waves
LIGO-Virgo
long duration transient

Disciplines

Astrophysics and Astronomy
Cosmology, Relativity, and Gravity

Access to Document

10.1088/1361-6382/aaab76License: CC BY

All-Sky Search for Long-Duration Gravitational Wave Transients inFinal published version, 1.41 MBLicense: CC BY

Cite this

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

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 \textasciitilde{}10−8 in gravitational waves.",

keywords = "gravitational waves, LIGO-Virgo, long duration transient",

author = "Abbott, \{B. P.\} and K. Gill and B. Hughey and Pratt, \{J. W. W.\} and E. Rhoades and E. Schmidt and Schwalbe, \{S. G.\} and Szczepa{\'n}czyk, \{M. J.\} and M. Zanolin and et al.",

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doi = "10.1088/1361-6382/aaab76",

language = "American English",

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journal = "Classical and Quantum Gravity",

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AU - Abbott, B. P.

AU - Gill, K.

AU - Hughey, B.

AU - Pratt, J. W. W.

AU - Rhoades, E.

AU - Schmidt, E.

AU - Schwalbe, S. G.

AU - Szczepańczyk, M. J.

AU - Zanolin, M.

AU - al., et

PY - 2018/2/14

Y1 - 2018/2/14

N2 - 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.

AB - 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.

KW - gravitational waves

KW - LIGO-Virgo

KW - long duration transient

UR - https://commons.erau.edu/publication/784

U2 - 10.1088/1361-6382/aaab76

DO - 10.1088/1361-6382/aaab76

M3 - Article

SN - 1361-6382

VL - 35

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

ER -

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

Abstract

Keywords

Disciplines

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