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author Wipf, Christopher C.
Weiss, Rainer
Waldman, Samuel J.
Stein, Leo Chaim
Stein, Andrew J.
Smith, Nicolas de Mateo
Shapiro, B.
Sarin, P.
Markowitz, Jared John
Katsavounidis, Erotokritos
Hughey, Brennan J.
Harry, Gregory
Grimaldi, F.
Goda, K.
Foley, Stephany
Duke, I.
Cao, Junwei
Brunet, G.
Blackburn, Lindy L.
Barsotti, Lisa
Mavalvala, Nergis
Zucker, Michael E
Mittleman, Richard K
Corbitt, Thomas R
Shoemaker, David H
Mason, Kenneth R
MacInnis, Myron E
Fritschel, Peter K
Evans, Matthew J
Donovan, Frederick J
Bodiya, Timothy P.
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Wipf, Christopher C.
Weiss, Rainer
Waldman, Samuel J.
Stein, Leo Chaim
Stein, Andrew J.
Smith, Nicolas de Mateo
Shapiro, B.
Sarin, P.
Markowitz, Jared John
Katsavounidis, Erotokritos
Hughey, Brennan J.
Harry, Gregory
Grimaldi, F.
Goda, K.
Foley, Stephany
Duke, I.
Cao, Junwei
Brunet, G.
Blackburn, Lindy L.
Barsotti, Lisa
Mavalvala, Nergis
Zucker, Michael E
Mittleman, Richard K
Corbitt, Thomas R
Shoemaker, David H
Mason, Kenneth R
MacInnis, Myron E
Fritschel, Peter K
Evans, Matthew J
Donovan, Frederick J
Bodiya, Timothy P.
author_sort Wipf, Christopher C.
collection MIT
description We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35M[subscript ⊙], using LIGO observations between November 14, 2006 and May 18, 2007. No gravitational-wave signals were detected. We report upper limits on the rate of compact binary coalescence as a function of total mass. The LIGO cumulative 90%-confidence rate upper limits of the binary coalescence of neutron stars, black holes and black hole-neutron star systems are 1.4×10[superscript -2], 7.3×10[superscript -4] and 3.6×10[superscript -3]  yr[superscript -1] L[subscript 10][superscript -1], respectively, where L[subscript 10] is 10[superscript 10] times the blue solar luminosity.
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spelling mit-1721.1/518422022-09-30T17:31:54Z Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO’s fifth science run Wipf, Christopher C. Weiss, Rainer Waldman, Samuel J. Stein, Leo Chaim Stein, Andrew J. Smith, Nicolas de Mateo Shapiro, B. Sarin, P. Markowitz, Jared John Katsavounidis, Erotokritos Hughey, Brennan J. Harry, Gregory Grimaldi, F. Goda, K. Foley, Stephany Duke, I. Cao, Junwei Brunet, G. Blackburn, Lindy L. Barsotti, Lisa Mavalvala, Nergis Zucker, Michael E Mittleman, Richard K Corbitt, Thomas R Shoemaker, David H Mason, Kenneth R MacInnis, Myron E Fritschel, Peter K Evans, Matthew J Donovan, Frederick J Bodiya, Timothy P. Massachusetts Institute of Technology. Department of Physics MIT Kavli Institute for Astrophysics and Space Research Mavalvala, Nergis Zucker, Michael E. Wipf, Christopher C. Weiss, Rainer Waldman, Samuel J. Stein, Leo Chaim Stein, Andrew J. Smith, Nicolas de Mateo Shoemaker, David H. Shapiro, B. Sarin, P. Mittleman, Richard K. Mason, Kenneth R. Markowitz, Jared John MacInnis, Myron E. Katsavounidis, Erotokritos Hughey, Brennan J. Harry, Gregory Grimaldi, F. Goda, K. Fritschel, Peter K. Foley, Stephany Evans, Matthew J. Duke, I. Donovan, Frederick J. Corbitt, Thomas R. Cao, Junwei Brunet, G. Bodiya, Timothy Paul Blackburn, Lindy L. Barsotti, Lisa Mavalvala, Nergis We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35M[subscript ⊙], using LIGO observations between November 14, 2006 and May 18, 2007. No gravitational-wave signals were detected. We report upper limits on the rate of compact binary coalescence as a function of total mass. The LIGO cumulative 90%-confidence rate upper limits of the binary coalescence of neutron stars, black holes and black hole-neutron star systems are 1.4×10[superscript -2], 7.3×10[superscript -4] and 3.6×10[superscript -3]  yr[superscript -1] L[subscript 10][superscript -1], respectively, where L[subscript 10] is 10[superscript 10] times the blue solar luminosity. Alfred P. Sloan Foundation Research Corporation David and Lucile Packard Foundation Leverhulme Trust Carnegie Trust National Aeronautics and Space Administration Scottish Universities Physics Alliance Scottish Funding Council Royal Society, United Kingdom Conselleria d’Economia, Hisenda i Innovació of the Govern de les Illes Balears Ministerio de Ciencia e Innovación, Spain Istituto Nazionale di Fisica Nucleare of Italy Council of Scientific and Industrial Research of India Australian Research Council State of Niedersachsen/Germany Max Planck Society for the Advancement of Science Science and Technology Facilities Council, United Kingdom National Science Foundation 2010-03-01T15:30:30Z 2010-03-01T15:30:30Z 2009-08 2009-06 Article http://purl.org/eprint/type/JournalArticle 1550-2368 1550-7998 http://hdl.handle.net/1721.1/51842 LIGO Scientific Collaboration et al. “Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO's fifth science run.” Physical Review D 80.4 (2009): 047101. © 2009 The American Physical Society https://orcid.org/0000-0003-0219-9706 https://orcid.org/0000-0001-6550-3045 https://orcid.org/0000-0002-4147-2560 https://orcid.org/0000-0001-8459-4499 https://orcid.org/0000-0002-2544-1596 https://orcid.org/0000-0003-1983-3187 en_US http://dx.doi.org/10.1103/PhysRevD.80.047101 Physical Review D Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf American Physical Society APS
spellingShingle Wipf, Christopher C.
Weiss, Rainer
Waldman, Samuel J.
Stein, Leo Chaim
Stein, Andrew J.
Smith, Nicolas de Mateo
Shapiro, B.
Sarin, P.
Markowitz, Jared John
Katsavounidis, Erotokritos
Hughey, Brennan J.
Harry, Gregory
Grimaldi, F.
Goda, K.
Foley, Stephany
Duke, I.
Cao, Junwei
Brunet, G.
Blackburn, Lindy L.
Barsotti, Lisa
Mavalvala, Nergis
Zucker, Michael E
Mittleman, Richard K
Corbitt, Thomas R
Shoemaker, David H
Mason, Kenneth R
MacInnis, Myron E
Fritschel, Peter K
Evans, Matthew J
Donovan, Frederick J
Bodiya, Timothy P.
Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO’s fifth science run
title Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO’s fifth science run
title_full Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO’s fifth science run
title_fullStr Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO’s fifth science run
title_full_unstemmed Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO’s fifth science run
title_short Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO’s fifth science run
title_sort search for gravitational waves from low mass compact binary coalescence in 186 days of ligo s fifth science run
url http://hdl.handle.net/1721.1/51842
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0001-6550-3045
https://orcid.org/0000-0002-4147-2560
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0002-2544-1596
https://orcid.org/0000-0003-1983-3187
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