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author Bodiya, Timothy Paul
Corbitt, Thomas R.
Donovan, Frederick J.
Dwyer, S.
Evans, Matthew J.
Foley, S.
Fritschel, Peter K.
Harry, Gregory
Katsavounidis, Erotokritos
Kissel, Jeffrey S.
MacInnis, Myron E.
Mandel, I.
Mason, Kenneth R.
Matichard, Fabrice
Mavalvala, Nergis
Mittleman, Richard K.
Oelker, Eric Glenn
Shapiro, B.
Shoemaker, David H.
Smith-Lefebvre, Nicolas D.
Soto, J.
Stein, A. J.
Stein, L. C.
Vaulin, Ruslan
Waldman, S. J.
Weiss, Rainer
Wipf, C. C.
Zucker, Michael E.
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Bodiya, Timothy Paul
Corbitt, Thomas R.
Donovan, Frederick J.
Dwyer, S.
Evans, Matthew J.
Foley, S.
Fritschel, Peter K.
Harry, Gregory
Katsavounidis, Erotokritos
Kissel, Jeffrey S.
MacInnis, Myron E.
Mandel, I.
Mason, Kenneth R.
Matichard, Fabrice
Mavalvala, Nergis
Mittleman, Richard K.
Oelker, Eric Glenn
Shapiro, B.
Shoemaker, David H.
Smith-Lefebvre, Nicolas D.
Soto, J.
Stein, A. J.
Stein, L. C.
Vaulin, Ruslan
Waldman, S. J.
Weiss, Rainer
Wipf, C. C.
Zucker, Michael E.
author_sort Bodiya, Timothy Paul
collection MIT
description We present the results of a search for gravitational waves associated with 154 gamma-ray bursts (GRBs) that were detected by satellite-based gamma-ray experiments in 2009-2010, during the sixth LIGO science run and the second and third Virgo science runs. We perform two distinct searches: a modeled search for coalescences of either two neutron stars or a neutron star and black hole, and a search for generic, unmodeled gravitational-wave bursts. We find no evidence for gravitational-wave counterparts, either with any individual GRB in this sample or with the population as a whole. For all GRBs we place lower bounds on the distance to the progenitor, under the optimistic assumption of a gravitational-wave emission energy of 10[superscript –2] M ☉ c [superscript 2] at 150 Hz, with a median limit of 17 Mpc. For short-hard GRBs we place exclusion distances on binary neutron star and neutron-star-black-hole progenitors, using astrophysically motivated priors on the source parameters, with median values of 16 Mpc and 28 Mpc, respectively. These distance limits, while significantly larger than for a search that is not aided by GRB satellite observations, are not large enough to expect a coincidence with a GRB. However, projecting these exclusions to the sensitivities of Advanced LIGO and Virgo, which should begin operation in 2015, we find that the detection of gravitational waves associated with GRBs will become quite possible.
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spelling mit-1721.1/929282022-09-27T18:05:16Z SEARCH FOR GRAVITATIONAL WAVES ASSOCIATED WITH GAMMA-RAY BURSTS DURING LIGO SCIENCE RUN 6 AND VIRGO SCIENCE RUNS 2 AND 3 Bodiya, Timothy Paul Corbitt, Thomas R. Donovan, Frederick J. Dwyer, S. Evans, Matthew J. Foley, S. Fritschel, Peter K. Harry, Gregory Katsavounidis, Erotokritos Kissel, Jeffrey S. MacInnis, Myron E. Mandel, I. Mason, Kenneth R. Matichard, Fabrice Mavalvala, Nergis Mittleman, Richard K. Oelker, Eric Glenn Shapiro, B. Shoemaker, David H. Smith-Lefebvre, Nicolas D. Soto, J. Stein, A. J. Stein, L. C. Vaulin, Ruslan Waldman, S. J. Weiss, Rainer Wipf, C. C. Zucker, Michael E. Massachusetts Institute of Technology. Department of Physics MIT Kavli Institute for Astrophysics and Space Research Bodiya, Timothy Paul Corbitt, Thomas R. Donovan, Frederick J. Dwyer, S. Evans, Matthew J. Foley, S. Fritschel, Peter K. Harry, Gregory Katsavounidis, Erotokritos Kissel, Jeffrey S. MacInnis, Myron E. Mandel, I. Mason, Kenneth R. Matichard, Fabrice Mavalvala, Nergis Mittleman, Richard K. Oelker, Eric Glenn Shapiro, B. Shoemaker, David H. Smith-Lefebvre, Nicolas D. Soto, J. Stein, A. J. Stein, L. C. Vaulin, Ruslan Waldman, S. J. Weiss, Rainer Wipf, C. C. Zucker, Michael E. We present the results of a search for gravitational waves associated with 154 gamma-ray bursts (GRBs) that were detected by satellite-based gamma-ray experiments in 2009-2010, during the sixth LIGO science run and the second and third Virgo science runs. We perform two distinct searches: a modeled search for coalescences of either two neutron stars or a neutron star and black hole, and a search for generic, unmodeled gravitational-wave bursts. We find no evidence for gravitational-wave counterparts, either with any individual GRB in this sample or with the population as a whole. For all GRBs we place lower bounds on the distance to the progenitor, under the optimistic assumption of a gravitational-wave emission energy of 10[superscript –2] M ☉ c [superscript 2] at 150 Hz, with a median limit of 17 Mpc. For short-hard GRBs we place exclusion distances on binary neutron star and neutron-star-black-hole progenitors, using astrophysically motivated priors on the source parameters, with median values of 16 Mpc and 28 Mpc, respectively. These distance limits, while significantly larger than for a search that is not aided by GRB satellite observations, are not large enough to expect a coincidence with a GRB. However, projecting these exclusions to the sensitivities of Advanced LIGO and Virgo, which should begin operation in 2015, we find that the detection of gravitational waves associated with GRBs will become quite possible. United States. National Aeronautics and Space Administration Carnegie Trust David & Lucile Packard Foundation Alfred P. Sloan Foundation 2015-01-16T14:57:49Z 2015-01-16T14:57:49Z 2012-10 2012-05 Article http://purl.org/eprint/type/JournalArticle 0004-637X 1538-4357 http://hdl.handle.net/1721.1/92928 Abadie, J., B. P. Abbott, R. Abbott, T. D. Abbott, M. Abernathy, T. Accadia, F. Acernese, et al. “SEARCH FOR GRAVITATIONAL WAVES ASSOCIATED WITH GAMMA-RAY BURSTS DURING LIGO SCIENCE RUN 6 AND VIRGO SCIENCE RUNS 2 AND 3.” The Astrophysical Journal 760, no. 1 (October 30, 2012): 12. © 2012 The American Astronomical Society https://orcid.org/0000-0003-2815-7387 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/10.1088/0004-637x/760/1/12 The Astrophysical Journal 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 IOP Publishing American Astronomical Society
spellingShingle Bodiya, Timothy Paul
Corbitt, Thomas R.
Donovan, Frederick J.
Dwyer, S.
Evans, Matthew J.
Foley, S.
Fritschel, Peter K.
Harry, Gregory
Katsavounidis, Erotokritos
Kissel, Jeffrey S.
MacInnis, Myron E.
Mandel, I.
Mason, Kenneth R.
Matichard, Fabrice
Mavalvala, Nergis
Mittleman, Richard K.
Oelker, Eric Glenn
Shapiro, B.
Shoemaker, David H.
Smith-Lefebvre, Nicolas D.
Soto, J.
Stein, A. J.
Stein, L. C.
Vaulin, Ruslan
Waldman, S. J.
Weiss, Rainer
Wipf, C. C.
Zucker, Michael E.
SEARCH FOR GRAVITATIONAL WAVES ASSOCIATED WITH GAMMA-RAY BURSTS DURING LIGO SCIENCE RUN 6 AND VIRGO SCIENCE RUNS 2 AND 3
title SEARCH FOR GRAVITATIONAL WAVES ASSOCIATED WITH GAMMA-RAY BURSTS DURING LIGO SCIENCE RUN 6 AND VIRGO SCIENCE RUNS 2 AND 3
title_full SEARCH FOR GRAVITATIONAL WAVES ASSOCIATED WITH GAMMA-RAY BURSTS DURING LIGO SCIENCE RUN 6 AND VIRGO SCIENCE RUNS 2 AND 3
title_fullStr SEARCH FOR GRAVITATIONAL WAVES ASSOCIATED WITH GAMMA-RAY BURSTS DURING LIGO SCIENCE RUN 6 AND VIRGO SCIENCE RUNS 2 AND 3
title_full_unstemmed SEARCH FOR GRAVITATIONAL WAVES ASSOCIATED WITH GAMMA-RAY BURSTS DURING LIGO SCIENCE RUN 6 AND VIRGO SCIENCE RUNS 2 AND 3
title_short SEARCH FOR GRAVITATIONAL WAVES ASSOCIATED WITH GAMMA-RAY BURSTS DURING LIGO SCIENCE RUN 6 AND VIRGO SCIENCE RUNS 2 AND 3
title_sort search for gravitational waves associated with gamma ray bursts during ligo science run 6 and virgo science runs 2 and 3
url http://hdl.handle.net/1721.1/92928
https://orcid.org/0000-0003-2815-7387
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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