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Strong-lensing of Gravitational Waves by Galaxy Clusters

Published online by Cambridge University Press:  29 January 2019

Graham P. Smith ,
Christopher Berry ,
Matteo Bianconi ,
Will M. Farr ,
Mathilde Jauzac ,
Richard Massey ,
Johan Richard ,
Andrew Robertson ,
Keren Sharon  and
Alberto Vecchio
...Show all authors
Graham P. Smith
Affiliation:
School of Physics and Astronomy, University of Birmingham, Birmingham, B15 2TT, England Email: [email protected]
Christopher Berry
Affiliation:
School of Physics and Astronomy, University of Birmingham, Birmingham, B15 2TT, England Birmingham Institute of Gravitational Wave Astronomy, University of Birmingham, Birmingham, B15 2TT, England
Matteo Bianconi
Affiliation:
School of Physics and Astronomy, University of Birmingham, Birmingham, B15 2TT, England
Will M. Farr
Affiliation:
School of Physics and Astronomy, University of Birmingham, Birmingham, B15 2TT, England Birmingham Institute of Gravitational Wave Astronomy, University of Birmingham, Birmingham, B15 2TT, England
Mathilde Jauzac
Affiliation:
Centre for Extragalactic Astronomy, Department of Physics, Durham University, Durham DH1 3LE, England Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE, England Astrophysics and Cosmology Research Unit, School of Mathematical Sciences, University of KwaZulu-Natal, Durban 4041, South Africa Laboratoire d’Astrophysique École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny CH-1290 Versoix, Switzerland
Richard Massey
Affiliation:
Centre for Extragalactic Astronomy, Department of Physics, Durham University, Durham DH1 3LE, England
Johan Richard
Affiliation:
CRAL, Observatoire de Lyon, Université Lyon 1, 9 Avenue Ch. André, 69561 Saint Genis Laval Cedex, France
Andrew Robertson
Affiliation:
Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE, England
Keren Sharon
Affiliation:
Department of Astronomy, University of Michigan, 500 Church St., Ann Arbor, MI 48109USA
Alberto Vecchio
Affiliation:
School of Physics and Astronomy, University of Birmingham, Birmingham, B15 2TT, England Birmingham Institute of Gravitational Wave Astronomy, University of Birmingham, Birmingham, B15 2TT, England
John Veitch
Affiliation:
School of Physics and Astronomy, University of Glasgow, G12 8QQ, Scotland
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Abstract

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Discovery of strongly-lensed gravitational wave (GW) sources will unveil binary compact objects at higher redshifts and lower intrinsic luminosities than is possible without lensing. Such systems will yield unprecedented constraints on the mass distribution in galaxy clusters, measurements of the polarization of GWs, tests of General Relativity, and constraints on the Hubble parameter. Excited by these prospects, and intrigued by the presence of so-called “heavy black holes” in the early detections by LIGO-Virgo, we commenced a search for strongly-lensed GWs and possible electromagnetic counterparts in the latter stages of the second LIGO observing run (O2). Here, we summarise our calculation of the detection rate of strongly-lensed GWs, describe our review of BBH detections from O1, outline our observing strategy in O2, summarize our follow-up observations of GW170814, and discuss the future prospects of detection.

Keywords

gravitational lensinggravitational wavesgalaxies: clusters: individual (MACS J0140.0−0555, MACS J1311.0−0310, RCS 0224−0002, Abell 3084, SMACS J0304.3− 4401)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S338: Gravitational Wave Astrophysics: Early Results from Gravitational Wave Searches and Electromagnetic Counterparts , October 2017 , pp. 98 - 102
Copyright
Copyright © International Astronomical Union 2019 

References

Abbott, B. P., et al., 2016a, Astrophys. J. Lett., 818, 22Google Scholar
Abbott, B. P., et al., 2016b, Phys. Rev. X, 6, 041015Google Scholar
Abbott, B. P., et al., 2017a, Phys. Rev. Lett., 118, 221101Google Scholar
Abbott, B. P., et al., 2017b, Phys. Rev. Lett., 119, 141101Google Scholar
Abbott, B. P., et al., 2017c, arXiv:1304.0670v4Google Scholar
Boldrin, M., et al., 2016, Mon. Not. R. Astron. Soc., 457, 2738Google Scholar
Broadhurst, T., et al., 2018, arXiv:1802.05273Google Scholar
Chatziioannou, K., Yunes, N., & Cornish, N., 2012, Phys. Rev. D, 86, 022004Google Scholar
Farr, W. M., et al., 2011, Astrophys. J., 741, 103Google Scholar
Fohlmeister, J., et al., 2007, Astrophys. J., 662, 62Google Scholar
Hilbert, S., et al., 2008, Mon. Not. R. Astron. Soc., 386, 1845Google Scholar
Inada, N., et al., 2014, Astron. J., 147, 153Google Scholar
Jauzac, M., et al., 2016, Mon. Not. R. Astron. Soc., 457, 2029Google Scholar
Li, S.-S., et al., 2018, arXiv:1802.05089Google Scholar
Liao, K., et al., 2017, Nature Communications, 8, 1148Google Scholar
LIGO Scientific Collaboration and Virgo Collaboration, 2017, GCN Circ. 21474, https://gcn.gsfc.nasa.gov/gcn3/21474.gcn3Google Scholar
LIGO Scientific Collaboration and Virgo Collaboration, 2017, GCN Circ. 21493, https://gcn.gsfc.nasa.gov/gcn3/21493.gcn3Google Scholar
Ng, K. K. J., et al., 2018, Phys. Rev. D, 97, 023012Google Scholar
Oguri, M., et al., 2010, Pub. Astron. Soc. Japan, 62, 1017Google Scholar
Oguri, M., et al., 2013, Mon. Not. R. Astron. Soc., 429, 482Google Scholar
Rodney, S. A., et al., 2016, Astrophys. J., 820, 50Google Scholar
Sharon, K., et al., 2017, Astrophys. J., 835, 5Google Scholar
Smith, G. P., et al., 2009, Astrophys. J. Lett., 707, 163Google Scholar
Smith, G. P., et al., 2017, GCN Circ. 21692, https://gcn.gsfc.nasa.gov/gcn3/21692.gcn3Google Scholar
Smith, G. P., et al., 2018, Mon. Not. R. Astron. Soc., 475, 3823Google Scholar
Wang, Y., Stebbins, A., & Turner, E. L., 1996, Phys. Rev. Lett., 77, 2875Google Scholar