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Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817

Pankow, Chris and Chatziioannou, Katerina and Chase, Eve A. and Littenberg, Tyson B. and Evans, Matthew and McIver, Jessica and Cornish, Neil J. and Haster, Carl-Johan and Kanner, Jonah and Raymond, Vivien and Vitale, Salvatore and Zimmerman, Aaron (2018) Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817. Physical Review D, 98 (8). Art. No. 084016. ISSN 2470-0010. http://resolver.caltech.edu/CaltechAUTHORS:20181010-094039772

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Abstract

In the coming years gravitational-wave detectors will undergo a series of improvements, with an increase in their detection rate by about an order of magnitude. Routine detections of gravitational-wave signals promote novel astrophysical and fundamental theory studies, while simultaneously leading to an increase in the number of detections temporally overlapping with instrumentally- or environmentally-induced transients in the detectors (glitches), often of unknown origin. Indeed, this was the case for the very first detection by the LIGO and Virgo detectors of a gravitational-wave signal consistent with a binary neutron star coalescence, GW170817. A loud glitch in the LIGO-Livingston detector, about one second before the merger, hampered coincident detection (which was initially achieved solely with LIGO-Hanford data). Moreover, accurate source characterization depends on specific assumptions about the behavior of the detector noise that are rendered invalid by the presence of glitches. In this paper, we present the various techniques employed for the initial mitigation of the glitch to perform source characterization of GW170817 and study advantages and disadvantages of each mitigation method. We show that, despite the presence of instrumental noise transients louder than the one affecting GW170817, we are still able to produce unbiased measurements of the intrinsic parameters from simulated injections with properties similar to GW170817.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/PhysRevD.98.084016DOIArticle
https://journals.aps.org/prd/abstract/10.1103/PhysRevD.98.084016PublisherArticle
https://arxiv.org/abs/1808.03619arXivDiscussion Paper
ORCID:
AuthorORCID
Kanner, Jonah0000-0001-8115-0577
Additional Information:© 2018 American Physical Society. Received 10 August 2018; published 10 October 2018. The authors are grateful for useful conversations with Duncan Brown and Stanislav Babak in the construction of the manuscript. C. P. is supported by the NSF Grant No. PHY-1607709, and also acknowledges support by the Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA). E. A. C. thanks the LSSTC Data Science Fellowship Program; her time as a fellow has benefited this work. E. A. C. also acknowledges support from the Illinois Space Grant Consortium Graduate Fellowship Program. N. C. acknowledges support from the NSF Award No. PHY-1306702. M. E and S. V. acknowledge the support of the National Science Foundation and the Laser Interferometer Gravitational-Wave Observatory (LIGO) Laboratory. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation and operates under cooperative agreement PHY-0757058. The authors thank the LIGO Scientific Collaboration for access to the data and gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, and the Max-Planck-Society (MPS) for support of the construction of Advanced LIGO. Additional support for Advanced LIGO was provided by the Australian Research Council.
Group:LIGO
Funders:
Funding AgencyGrant Number
NSFPHY-1607709
Northwestern UniversityUNSPECIFIED
Illinois Space Grant ConsortiumUNSPECIFIED
NSFPHY-1306702
NSFPHY-0757058
Science and Technology Facilities Council (STFC)UNSPECIFIED
Max-Planck-Society (MPS)UNSPECIFIED
Australian Research CouncilUNSPECIFIED
Record Number:CaltechAUTHORS:20181010-094039772
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20181010-094039772
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:90225
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:10 Oct 2018 17:07
Last Modified:10 Oct 2018 17:07

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