Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo
- Creators
- Abbott, B. P.
- Abbott, R.
- Abernathy, M. R.
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Adhikari, R. X.
- Anderson, S. B.
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Arai, K.
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Araya, M. C.
- Barayoga, J. C.
- Barish, B. C.
- Berger, B. K.
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Billingsley, G.
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Blackburn, J. K.
- Bork, R.
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Brooks, A. F.
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Cahillane, C.
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Callister, T.
- Cepeda, C.
- Chakraborty, R.
- Chalermsongsak, T.
- Couvares, P.
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Coyne, D. C.
- Dergachev, V.
- Drever, R. W. P.
- Ehrens, P.
- Etzel, T.
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Gossan, S. E.
- Gushwa, K. E.
- Gustafson, E. K.
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Hall, E. D.
- Heptonstall, A. W.
- Hodge, K. A.
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Isi, M.
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Kanner, J. B.
- Kells, W.
- Kondrashov, V.
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Korth, W. Z.
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Kozak, D. B.
- Lazzarini, A.
- Li, T. G. F.
- Mageswaran, M.
- Maros, E.
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Martynov, D.
- Marx, J. N.
- McIntyre, G.
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Meshkov, S.
- Pedraza, M.
- Perreca, A.
- Price, L. R.
- Quintero, E. A.
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Reitze, D. H.
- Robertson, N. A.
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Rollins, J. G.
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Sachdev, S.
- Sanchez, E. J.
- Schmidt, P.
- Shao, Z.
- Singer, A.
- Smith, N. D.
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Smith, R. J. E.
- Taylor, R.
- Thirugnanasambandam, M. P.
- Torrie, C. I.
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Vajente, G.
- Vass, S.
- Wallace, L.
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Weinstein, A. J.
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Williams, R. D.
- Wipf, C. C.
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Yamamoto, H.
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Zhang, L.
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Chen, Y.
- Engels, W.
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Ott, C. D.
- Thorne, K. S.
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Chatziioannou, K.
- LIGO Scientific Collaboration
- Virgo Collaboration
Abstract
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We determine the expected sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron-star systems, which are considered the most promising for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90% credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5 deg^2 to 20 deg^2 will require at least three detectors of sensitivity within a factor of ∼ 2 of each other and with a broad frequency bandwidth. Should the third LIGO detector be relocated to India as expected, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.
Additional Information
© 2016 The Author(s). Springer International. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. Figures that have been previously published elsewhere may not be reproduced without consent of the original copyright holders. Accepted: 22 January 2016. Published: 8 February 2016. The authors 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, the Max Planck Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO 600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de EconomÃa y Competitividad, the Conselleria d'Economia i Competitivitat and Conselleria d'Educació, Cultura i Universitats of the Govern de les Illes Balears, the National Science Centre of Poland, the FOCUS Programme of Foundation for Polish Science, the European Union, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Brazilian Ministry of Science, Technology, and Innovation, the Research Corporation, Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS and the State of Niedersachsen/Germany for provision of computational resources. This article has been assigned LIGO Document number External LinkP1200087, Virgo Document number External LinkVIR-0288A-12.Attached Files
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Submitted - 1304.0670v3.pdf
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Additional details
- PMCID
- PMC5256041
- Eprint ID
- 65325
- Resolver ID
- CaltechAUTHORS:20160314-070823106
- NSF
- Science and Technology Facilities Council (STFC)
- Max-Planck-Society
- State of Niedersachsen/Germany
- Australian Research Council
- Istituto Nazionale di Fisica Nucleare (INFN)
- Centre National de la Recherche Scientifique (CNRS)
- Stichting voor Fundamenteel Onderzoek der Materie (FOM)
- Council of Scientific and Industrial Research of India
- Department of Science and Technology, India
- Science and Engineering Research Board (SERB)
- Ministry of Human Resource Development, India
- Ministerio de EconomÃa y Competitividad (MINECO)
- Conselleria d'Economia i Competitivitat
- Conselleria d'Educaciό Cultura i Universitats of the Govern de les Illes Balears
- National Science Centre of Poland
- FOCUS Programme of Foundation for Polish Science
- European Union
- Royal Society
- Scottish Funding Council
- Scottish Universities Physics Alliance
- Lyon Institute of Origins (LIO)
- National Research Foundation of Korea
- Industry Canada
- Natural Sciences and Engineering Research Council of Canada (NSERC)
- Ministério da Ciência, Tecnologia e Inovação
- Research Corporation
- Ministry of Science and Technology (Taipei)
- Kavli Foundation
- Ontario Ministry of Economic Development and Innovation
- Created
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2016-03-14Created from EPrint's datestamp field
- Updated
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2022-05-10Created from EPrint's last_modified field
- Caltech groups
- LIGO, TAPIR
- Other Numbering System Name
- VIRGO Document
- Other Numbering System Identifier
- VIR-0288A-12