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  Fast detection and automatic parameter estimation of a gravitational wave signal with a novel method

Wang, Y. (2015). Fast detection and automatic parameter estimation of a gravitational wave signal with a novel method. General Relativity and Gravitation, 47(12): 142. doi:10.1007/s10714-015-1987-0.

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1402.6217.pdf (Preprint), 491KB
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 Creators:
Wang, Yan1, Author
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24010              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc, Astrophysics, Instrumentation and Methods for Astrophysics, astro-ph.IM
 Abstract: The detection of gravitational wave usually requires to match the measurement
data with a large number of templates, which is computationally very expensive.
Compressed sensing methods allow one to match the data with a small number of
templates and interpolate the rest. However, the interpolation process is still
computationally expensive. In this article, we designed a novel method that
only requires to match the data with a few templates, yet without needing any
interpolation process. The algorithm worked well for signals with relatively
high SNRs. It also showed promise for low SNRs signals.

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 Dates: 2014-02-252015
 Publication Status: Issued
 Pages: 5 pages
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 Table of Contents: -
 Rev. Type: -
 Identifiers: arXiv: 1402.6217
DOI: 10.1007/s10714-015-1987-0
 Degree: -

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Title: General Relativity and Gravitation
Source Genre: Journal
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Pages: - Volume / Issue: 47 (12) Sequence Number: 142 Start / End Page: - Identifier: -