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  Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors

Klimenko, S., Vedovato, G., Drago, M., Salemi, F., Tiwari, V., Prodi, G. A., et al. (2016). Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors. Physical Review D, 93: 042004. doi:10.1103/PhysRevD.93.042004.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0029-7793-5 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-002A-70ED-2
Genre: Journal Article

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1511.05999.pdf (Preprint), 725KB
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 Creators:
Klimenko, S., Author
Vedovato, G., Author
Drago, M.1, Author              
Salemi, F., Author
Tiwari, V., Author
Prodi, G. A., Author
Lazzaro, C., Author
Ackley, K., Author
Tiwari, S., Author
Cost-, C. F. Da Silva, Author
Mitselmakher, G., Author
Affiliations:
1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24011              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc, Astrophysics, Instrumentation and Methods for Astrophysics, astro-ph.IM
 Abstract: We present a method for detection and reconstruction of the gravitational-wave (GW) transients with the networks of advanced detectors. Originally designed to search for transients with the initial GW detectors, it uses significantly improved algorithms, which enhances both the low-latency searches with rapid localization of GW events for the electro-magnetic followup and high confidence detection of a broad range of the transient GW sources. In the paper we present the analytic framework of the method. Following a short description of the core analysis algorithms, we introduce a novel approach to the reconstruction of the GW polarization from a pattern of detector responses to a GW signal. This polarization pattern is a unique signature of an arbitrary GW signal that can be measured independent from the other source parameters. The polarization measurements enable rapid reconstruction of the GW waveforms, sky localization and helps identification of the source origin.

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 Dates: 2015-11-182016-01-222016
 Publication Status: Published in print
 Pages: 9 pages, 4 figures, 1 table
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1511.05999
DOI: 10.1103/PhysRevD.93.042004
 Degree: -

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Title: Physical Review D
  Other : Phys. Rev. D.
Source Genre: Journal
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Publ. Info: Lancaster, Pa. : American Physical Society
Pages: - Volume / Issue: 93 Sequence Number: 042004 Start / End Page: - Identifier: ISSN: 0556-2821
CoNE: http://pubman.mpdl.mpg.de/cone/journals/resource/111088197762258