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Characterising transient noise in the LIGO detectors

Research output: Contribution to journalArticle

Data from the LIGO detectors typically contain many non-Gaussian noise transients which arise due to instrumental and environmental conditions. These non-Gaussian transients can be an issue for the modelled and unmodelled transient gravitational-wave searches, as they can mask or mimic a true signal. Data quality can change quite rapidly, making it imperative to track and find new sources of transient noise so that data are minimally contaminated. Several examples of transient noise and the tools used to track them are presented. These instances serve to highlight the diverse range of noise sources present at the LIGO detectors during their second observing run.
Original languageEnglish
Article number20170286
JournalPhilosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
Volume376
Issue number2120
Early online date16 Apr 2018
DOIs
Publication statusPublished - May 2018

Documents

  • 1804.07592v1

    Accepted author manuscript (Post-print), 846 KB, PDF-document

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