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author Barsotti, Lisa
Foley, Stephany
Harry, Gregory
Kissel, Jeffrey S.
Mandel, Ilya
Matichard, Fabrice
Oelker, Eric Glenn
Soto, Jose M.
Stein, Andrew J.
Stein, Leo Chaim
Vaulin, Ruslan
Waldman, Samuel J.
Weiss, Rainer
Wipf, Christopher C.
Mavalvala, Nergis
Katsavounidis, Erotokritos
Bodiya, Timothy P.
Donovan, Frederick J
Shoemaker, David H
Zucker, Michael E
Corbitt, Thomas R
Dwyer, Sheila Elizabeth
Fritschel, Peter K
Evans, Matthew J
MacInnis, Myron E
Mason, Kenneth R
Mittleman, Richard K
Shapiro, B.
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Barsotti, Lisa
Foley, Stephany
Harry, Gregory
Kissel, Jeffrey S.
Mandel, Ilya
Matichard, Fabrice
Oelker, Eric Glenn
Soto, Jose M.
Stein, Andrew J.
Stein, Leo Chaim
Vaulin, Ruslan
Waldman, Samuel J.
Weiss, Rainer
Wipf, Christopher C.
Mavalvala, Nergis
Katsavounidis, Erotokritos
Bodiya, Timothy P.
Donovan, Frederick J
Shoemaker, David H
Zucker, Michael E
Corbitt, Thomas R
Dwyer, Sheila Elizabeth
Fritschel, Peter K
Evans, Matthew J
MacInnis, Myron E
Mason, Kenneth R
Mittleman, Richard K
Shapiro, B.
author_sort Barsotti, Lisa
collection MIT
description We present results from a search for gravitational-wave bursts in the data collected by the LIGO and Virgo detectors between July 7, 2009 and October 20, 2010: data are analyzed when at least two of the three LIGO-Virgo detectors are in coincident operation, with a total observation time of 207 days. The analysis searches for transients of duration ≲1  s over the frequency band 64–5000 Hz, without other assumptions on the signal waveform, polarization, direction or occurrence time. All identified events are consistent with the expected accidental background. We set frequentist upper limits on the rate of gravitational-wave bursts by combining this search with the previous LIGO-Virgo search on the data collected between November 2005 and October 2007. The upper limit on the rate of strong gravitational-wave bursts at the Earth is 1.3 events per year at 90% confidence. We also present upper limits on source rate density per year and Mpc3 for sample populations of standard-candle sources. As in the previous joint run, typical sensitivities of the search in terms of the root-sum-squared strain amplitude for these waveforms lie in the range ∼5×10-22  Hz-1/2 to ∼1×10-20  Hz-1/2. The combination of the two joint runs entails the most sensitive all-sky search for generic gravitational-wave bursts and synthesizes the results achieved by the initial generation of interferometric detectors
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spelling mit-1721.1/721472022-09-30T21:22:30Z All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run Barsotti, Lisa Foley, Stephany Harry, Gregory Kissel, Jeffrey S. Mandel, Ilya Matichard, Fabrice Oelker, Eric Glenn Soto, Jose M. Stein, Andrew J. Stein, Leo Chaim Vaulin, Ruslan Waldman, Samuel J. Weiss, Rainer Wipf, Christopher C. Mavalvala, Nergis Katsavounidis, Erotokritos Bodiya, Timothy P. Donovan, Frederick J Shoemaker, David H Zucker, Michael E Corbitt, Thomas R Dwyer, Sheila Elizabeth Fritschel, Peter K Evans, Matthew J MacInnis, Myron E Mason, Kenneth R Mittleman, Richard K Shapiro, B. Massachusetts Institute of Technology. Department of Physics Massachusetts Institute of Technology. School of Science MIT Kavli Institute for Astrophysics and Space Research Weiss, Rainer Barsotti, Lisa Bodiya, Timothy Paul Corbitt, Thomas R. Donovan, Frederick J. Dwyer, Sheila J. Foley, Stephany Fritschel, Peter K. Harry, Gregory Evans, Matthew J. Kissel, Jeffrey S. MacInnis, Myron E. Mandel, Ilya Mason, Kenneth R. Matichard, Fabrice Mittleman, Richard K. Oelker, Eric Glenn Shapiro, Brett Noah Shoemaker, David H. Soto, Jose M. Stein, Andrew J. Stein, Leo Chaim Vaulin, Ruslan Waldman, Samuel J. Weiss, Rainer Wipf, Christopher C. Zucker, Michael E. Mavalvala, Nergis Katsavounidis, Erotokritos We present results from a search for gravitational-wave bursts in the data collected by the LIGO and Virgo detectors between July 7, 2009 and October 20, 2010: data are analyzed when at least two of the three LIGO-Virgo detectors are in coincident operation, with a total observation time of 207 days. The analysis searches for transients of duration ≲1  s over the frequency band 64–5000 Hz, without other assumptions on the signal waveform, polarization, direction or occurrence time. All identified events are consistent with the expected accidental background. We set frequentist upper limits on the rate of gravitational-wave bursts by combining this search with the previous LIGO-Virgo search on the data collected between November 2005 and October 2007. The upper limit on the rate of strong gravitational-wave bursts at the Earth is 1.3 events per year at 90% confidence. We also present upper limits on source rate density per year and Mpc3 for sample populations of standard-candle sources. As in the previous joint run, typical sensitivities of the search in terms of the root-sum-squared strain amplitude for these waveforms lie in the range ∼5×10-22  Hz-1/2 to ∼1×10-20  Hz-1/2. The combination of the two joint runs entails the most sensitive all-sky search for generic gravitational-wave bursts and synthesizes the results achieved by the initial generation of interferometric detectors 2012-08-15T16:04:59Z 2012-08-15T16:04:59Z 2012-06 2012-03 Article http://purl.org/eprint/type/JournalArticle 1550-7998 1089-4918 http://hdl.handle.net/1721.1/72147 Abadie, J. et al. “All-sky Search for Gravitational-wave Bursts in the Second Joint LIGO-Virgo Run.” Physical Review D 85.12 (2012): 122007. © 2012 American Physical Society. https://orcid.org/0000-0003-0219-9706 https://orcid.org/0000-0003-2815-7387 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.85.122007 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 Barsotti, Lisa
Foley, Stephany
Harry, Gregory
Kissel, Jeffrey S.
Mandel, Ilya
Matichard, Fabrice
Oelker, Eric Glenn
Soto, Jose M.
Stein, Andrew J.
Stein, Leo Chaim
Vaulin, Ruslan
Waldman, Samuel J.
Weiss, Rainer
Wipf, Christopher C.
Mavalvala, Nergis
Katsavounidis, Erotokritos
Bodiya, Timothy P.
Donovan, Frederick J
Shoemaker, David H
Zucker, Michael E
Corbitt, Thomas R
Dwyer, Sheila Elizabeth
Fritschel, Peter K
Evans, Matthew J
MacInnis, Myron E
Mason, Kenneth R
Mittleman, Richard K
Shapiro, B.
All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run
title All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run
title_full All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run
title_fullStr All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run
title_full_unstemmed All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run
title_short All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run
title_sort all sky search for gravitational wave bursts in the second joint ligo virgo run
url http://hdl.handle.net/1721.1/72147
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0003-2815-7387
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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