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  Analysis Framework for the Prompt Discovery of Compact Binary Mergers in Gravitational-wave Data

Messick, C., Blackburn, K., Brady, P., Brockill, P., Cannon, K., Caudill, S., et al. (2017). Analysis Framework for the Prompt Discovery of Compact Binary Mergers in Gravitational-wave Data. Physical Review D, 95(4): 042001. doi:10.1103/PhysRevD.95.042001.

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 Creators:
Messick, Cody, Author
Blackburn, Kent, Author
Brady, Patrick, Author
Brockill, Patrick, Author
Cannon, Kipp, Author
Caudill, Sarah, Author
Chamberlin, Sydney J., Author
Creighton, Jolien D. E., Author
Everett, Ryan, Author
Hanna, Chad, Author
Lang, Ryan N., Author
Li, Tjonnie G. F., Author
Meacher, Duncan, Author
Pankow, Chris, Author
Privitera, Stephen1, Author           
Qi, Hong, Author
Sachdev, Surabhi, Author
Sadeghian, Laleh, Author
Sathyaprakash, B., Author
Singer, Leo, Author
Thomas, E. Gareth, AuthorWade, Leslie, AuthorWade, Madeline, AuthorWeinstein, Alan, Author more..
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

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Free keywords: Astrophysics, Instrumentation and Methods for Astrophysics, astro-ph.IM
 Abstract: We describe a stream-based analysis pipeline to detect gravitational waves from the merger of binary neutron stars, binary black holes, and neutron-star-black-hole binaries within ~ 1 minute of the arrival of the merger signal at Earth. Such low-latency detection is crucial for the prompt response by electromagnetic facilities in order to observe any fading electromagnetic counterparts that might be produced by mergers involving at least one neutron star. Even for systems expected not to produce counterparts, analysis of the data in low-latency for their GW signals is useful for deciding when not to point telescopes, and as feedback to observatory operations. The pipeline also operates in an offline mode, in which it incorporates more refined information about data quality and employs acausal methods that are inapplicable to the online mode.

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 Dates: 2016-04-1420162017
 Publication Status: Issued
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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: 95 (4) Sequence Number: 042001 Start / End Page: - Identifier: ISSN: 0556-2821
CoNE: https://pure.mpg.de/cone/journals/resource/111088197762258