@article{caltechauthors43573,
          volume = {88},
          number = {12},
           month = {December},
          author = {J. Aasi and J. Abadie and B. P. Abbott and R. Abbott and M. R. Abernathy and R. X. Adhikari and P. Ajith and R. A. Anderson and K. Arai and M. C. Araya and L. Austin and J. C.  Barayoga and G. Billingsley and E. Black and J. K. Blackburn and R. Bork and A. F. Brooks and C. Cepeda and R. Chakraborty and T. Chalermsongsak and Y. Chen and D. C. Coyne and B. Daudert and V. Dergachev and R. W. P. Drever and J. C. Driggers and P. Ehrens and T. Etzel and N. Fotopoulos and S. Gossan and K. E. Gushwa and E. K. Gustafson and E. Hall and J. Harms and J. Heefner and A. W. Heptonstall and K. A. Hodge and T. Hong and A. Ivanov and M. Jacobson and E. James and P. Kalmus and K. Kaufman and W. Kells and P. J. King and V. Kondrashov and W. Z. Korth and D. Kozak and A. Lazzarini and J. B. Lewis and D. Lloyd and J. Luan and M. Mageswaran and K. Mailand and E. Maros and D. Martynov and J. N. Marx and G. McIntyre and S. Meshkov and H. Miao and T. Nash and G. H. Ogin and C. Osthelder and C. D. Ott and M. Pedraza and M. Phelps and C. Poux and L. R. Price and S. Privitera and E. Quintero and V. Raymond and J. G. Rollins and V. Sannibale and F. Seifert and A. Singer and L. Singer and M. R. Smith and N. D. Smith-Lefebvre and R. Taylor and M. P. Thirugnanasambandam and E. Thrane and K. S. Thorne and S. Vass and M. Vallisneri and L. Wallace and A. J. Weinstein and R. Williams and H. Yamamoto and H. Yang and D. Yeaton-Massey and L. Zhang and J. Zweizig and S. B. Anderson and N. A. Robertson and C. I. Torrie},
            note = {{\copyright} 2013 American Physical Society.

Received 9 October 2013; published 13 December 2013.

The authors gratefully acknowledge the support of the
United States National Science Foundation for the construction
and operation of the LIGO Laboratory, the
Science and Technology Facilities Council of the United
Kingdom, the Max-Planck-Society, and the State of
Niedersachsen/Germany for support of the construction
and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre
National de la Recherche Scientifique for the construction
and operation of the Virgo detector. The authors also
gratefully acknowledge the support of the research by
these agencies and by the Australian Research Council,
the International Science Linkages program of the
Commonwealth of Australia, the Council of Scientific
and Industrial Research of India, the Istituto Nazionale di
Fisica Nucleare of Italy, the Spanish Ministerio de
Econom??a y Competitividad, the Conselleria d?Economia
Hisenda i Innovacio? of the Govern de les Illes Balears, the
Foundation for Fundamental Research on Matter supported
by the Netherlands Organisation for Scientific Research,
the Polish Ministry of Science and Higher Education, the
FOCUS Programme of Foundation for Polish Science, the
Royal Society, the Scottish Funding Council, the Scottish
Universities Physics Alliance, The National Aeronautics
and Space Administration, OTKA of Hungary, 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 Carnegie Trust, the
Leverhulme Trust, the David and Lucile Packard
Foundation, the Research Corporation, and the Alfred P.
Sloan Foundation.},
           title = {Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts},
       publisher = {American Physical Society},
            year = {2013},
         journal = {Physical Review D},
           pages = {Article No. 122004},
             url = {http://resolver.caltech.edu/CaltechAUTHORS:20140130-095945569},
        abstract = {Long gamma-ray bursts (GRBs) have been linked to extreme core-collapse supernovae from massivestars. Gravitational waves (GW) offer a probe of the physics behind long GRBs. We investigate models of long-lived ({\texttt{\char126}}10?1000 s) GW emission associated with the accretion disk of a collapsed star or with its
protoneutron star remnant. Using data from LIGO?s fifth science run, and GRB triggers from the Swift experiment, we perform a search for unmodeled long-lived GW transients. Finding no evidence of GW emission, we place 90\% confidence-level upper limits on the GW fluence at Earth from long GRBs for
three waveforms inspired by a model of GWs from accretion disk instabilities. These limits range from F {\ensuremath{<}} 3:5 ergs cm{\^{ }}(-2) to F {\ensuremath{<}} 1200 ergs cm{\^{ }}(-2), depending on the GRB and on the model, allowing us to probe
optimistic scenarios of GW production out to distances as far as {$\approx$} 33 Mpc. Advanced detectors are expected to achieve strain sensitivities 10x better than initial LIGO, potentially allowing us to probe the engines of the nearest long GRBs.}
}

{"_id":"ZoR4jQtDpYjPEHphw","bibbaseid":"aasi-abadie-abbott-abbott-abernathy-adhikari-ajith-anderson-etal-searchforlonglivedgravitationalwavetransientscoincidentwithlonggammaraybursts-2013","downloads":0,"creationDate":"2017-11-11T20:48:21.457Z","title":"Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts","author_short":["Aasi, J.","Abadie, J.","Abbott, B. P.","Abbott, R.","Abernathy, M. R.","Adhikari, R. X.","Ajith, P.","Anderson, R. A.","Arai, K.","Araya, M. C.","Austin, L.","Barayoga, J. C.","Billingsley, G.","Black, E.","Blackburn, J. K.","Bork, R.","Brooks, A. F.","Cepeda, C.","Chakraborty, R.","Chalermsongsak, T.","Chen, Y.","Coyne, D. C.","Daudert, B.","Dergachev, V.","Drever, R. W. P.","Driggers, J. C.","Ehrens, P.","Etzel, T.","Fotopoulos, N.","Gossan, S.","Gushwa, K. E.","Gustafson, E. K.","Hall, E.","Harms, J.","Heefner, J.","Heptonstall, A. W.","Hodge, K. A.","Hong, T.","Ivanov, A.","Jacobson, M.","James, E.","Kalmus, P.","Kaufman, K.","Kells, W.","King, P. J.","Kondrashov, V.","Korth, W. Z.","Kozak, D.","Lazzarini, A.","Lewis, J. B.","Lloyd, D.","Luan, J.","Mageswaran, M.","Mailand, K.","Maros, E.","Martynov, D.","Marx, J. N.","McIntyre, G.","Meshkov, S.","Miao, H.","Nash, T.","Ogin, G. H.","Osthelder, C.","Ott, C. D.","Pedraza, M.","Phelps, M.","Poux, C.","Price, L. R.","Privitera, S.","Quintero, E.","Raymond, V.","Rollins, J. G.","Sannibale, V.","Seifert, F.","Singer, A.","Singer, L.","Smith, M. R.","Smith-Lefebvre, N. D.","Taylor, R.","Thirugnanasambandam, M. P.","Thrane, E.","Thorne, K. S.","Vass, S.","Vallisneri, M.","Wallace, L.","Weinstein, A. J.","Williams, R.","Yamamoto, H.","Yang, H.","Yeaton-Massey, D.","Zhang, L.","Zweizig, J.","Anderson, S. B.","Robertson, N. A.","Torrie, C. I."],"year":2013,"bibtype":"article","biburl":"https://authors.library.caltech.edu/cgi/exportview/person-az/Adhikari-R-X/LocalBibTeX/Adhikari-R-X.bib","bibdata":{"bibtype":"article","type":"article","volume":"88","number":"12","month":"December","author":[{"firstnames":["J."],"propositions":[],"lastnames":["Aasi"],"suffixes":[]},{"firstnames":["J."],"propositions":[],"lastnames":["Abadie"],"suffixes":[]},{"firstnames":["B.","P."],"propositions":[],"lastnames":["Abbott"],"suffixes":[]},{"firstnames":["R."],"propositions":[],"lastnames":["Abbott"],"suffixes":[]},{"firstnames":["M.","R."],"propositions":[],"lastnames":["Abernathy"],"suffixes":[]},{"firstnames":["R.","X."],"propositions":[],"lastnames":["Adhikari"],"suffixes":[]},{"firstnames":["P."],"propositions":[],"lastnames":["Ajith"],"suffixes":[]},{"firstnames":["R.","A."],"propositions":[],"lastnames":["Anderson"],"suffixes":[]},{"firstnames":["K."],"propositions":[],"lastnames":["Arai"],"suffixes":[]},{"firstnames":["M.","C."],"propositions":[],"lastnames":["Araya"],"suffixes":[]},{"firstnames":["L."],"propositions":[],"lastnames":["Austin"],"suffixes":[]},{"firstnames":["J.","C."],"propositions":[],"lastnames":["Barayoga"],"suffixes":[]},{"firstnames":["G."],"propositions":[],"lastnames":["Billingsley"],"suffixes":[]},{"firstnames":["E."],"propositions":[],"lastnames":["Black"],"suffixes":[]},{"firstnames":["J.","K."],"propositions":[],"lastnames":["Blackburn"],"suffixes":[]},{"firstnames":["R."],"propositions":[],"lastnames":["Bork"],"suffixes":[]},{"firstnames":["A.","F."],"propositions":[],"lastnames":["Brooks"],"suffixes":[]},{"firstnames":["C."],"propositions":[],"lastnames":["Cepeda"],"suffixes":[]},{"firstnames":["R."],"propositions":[],"lastnames":["Chakraborty"],"suffixes":[]},{"firstnames":["T."],"propositions":[],"lastnames":["Chalermsongsak"],"suffixes":[]},{"firstnames":["Y."],"propositions":[],"lastnames":["Chen"],"suffixes":[]},{"firstnames":["D.","C."],"propositions":[],"lastnames":["Coyne"],"suffixes":[]},{"firstnames":["B."],"propositions":[],"lastnames":["Daudert"],"suffixes":[]},{"firstnames":["V."],"propositions":[],"lastnames":["Dergachev"],"suffixes":[]},{"firstnames":["R.","W.","P."],"propositions":[],"lastnames":["Drever"],"suffixes":[]},{"firstnames":["J.","C."],"propositions":[],"lastnames":["Driggers"],"suffixes":[]},{"firstnames":["P."],"propositions":[],"lastnames":["Ehrens"],"suffixes":[]},{"firstnames":["T."],"propositions":[],"lastnames":["Etzel"],"suffixes":[]},{"firstnames":["N."],"propositions":[],"lastnames":["Fotopoulos"],"suffixes":[]},{"firstnames":["S."],"propositions":[],"lastnames":["Gossan"],"suffixes":[]},{"firstnames":["K.","E."],"propositions":[],"lastnames":["Gushwa"],"suffixes":[]},{"firstnames":["E.","K."],"propositions":[],"lastnames":["Gustafson"],"suffixes":[]},{"firstnames":["E."],"propositions":[],"lastnames":["Hall"],"suffixes":[]},{"firstnames":["J."],"propositions":[],"lastnames":["Harms"],"suffixes":[]},{"firstnames":["J."],"propositions":[],"lastnames":["Heefner"],"suffixes":[]},{"firstnames":["A.","W."],"propositions":[],"lastnames":["Heptonstall"],"suffixes":[]},{"firstnames":["K.","A."],"propositions":[],"lastnames":["Hodge"],"suffixes":[]},{"firstnames":["T."],"propositions":[],"lastnames":["Hong"],"suffixes":[]},{"firstnames":["A."],"propositions":[],"lastnames":["Ivanov"],"suffixes":[]},{"firstnames":["M."],"propositions":[],"lastnames":["Jacobson"],"suffixes":[]},{"firstnames":["E."],"propositions":[],"lastnames":["James"],"suffixes":[]},{"firstnames":["P."],"propositions":[],"lastnames":["Kalmus"],"suffixes":[]},{"firstnames":["K."],"propositions":[],"lastnames":["Kaufman"],"suffixes":[]},{"firstnames":["W."],"propositions":[],"lastnames":["Kells"],"suffixes":[]},{"firstnames":["P.","J."],"propositions":[],"lastnames":["King"],"suffixes":[]},{"firstnames":["V."],"propositions":[],"lastnames":["Kondrashov"],"suffixes":[]},{"firstnames":["W.","Z."],"propositions":[],"lastnames":["Korth"],"suffixes":[]},{"firstnames":["D."],"propositions":[],"lastnames":["Kozak"],"suffixes":[]},{"firstnames":["A."],"propositions":[],"lastnames":["Lazzarini"],"suffixes":[]},{"firstnames":["J.","B."],"propositions":[],"lastnames":["Lewis"],"suffixes":[]},{"firstnames":["D."],"propositions":[],"lastnames":["Lloyd"],"suffixes":[]},{"firstnames":["J."],"propositions":[],"lastnames":["Luan"],"suffixes":[]},{"firstnames":["M."],"propositions":[],"lastnames":["Mageswaran"],"suffixes":[]},{"firstnames":["K."],"propositions":[],"lastnames":["Mailand"],"suffixes":[]},{"firstnames":["E."],"propositions":[],"lastnames":["Maros"],"suffixes":[]},{"firstnames":["D."],"propositions":[],"lastnames":["Martynov"],"suffixes":[]},{"firstnames":["J.","N."],"propositions":[],"lastnames":["Marx"],"suffixes":[]},{"firstnames":["G."],"propositions":[],"lastnames":["McIntyre"],"suffixes":[]},{"firstnames":["S."],"propositions":[],"lastnames":["Meshkov"],"suffixes":[]},{"firstnames":["H."],"propositions":[],"lastnames":["Miao"],"suffixes":[]},{"firstnames":["T."],"propositions":[],"lastnames":["Nash"],"suffixes":[]},{"firstnames":["G.","H."],"propositions":[],"lastnames":["Ogin"],"suffixes":[]},{"firstnames":["C."],"propositions":[],"lastnames":["Osthelder"],"suffixes":[]},{"firstnames":["C.","D."],"propositions":[],"lastnames":["Ott"],"suffixes":[]},{"firstnames":["M."],"propositions":[],"lastnames":["Pedraza"],"suffixes":[]},{"firstnames":["M."],"propositions":[],"lastnames":["Phelps"],"suffixes":[]},{"firstnames":["C."],"propositions":[],"lastnames":["Poux"],"suffixes":[]},{"firstnames":["L.","R."],"propositions":[],"lastnames":["Price"],"suffixes":[]},{"firstnames":["S."],"propositions":[],"lastnames":["Privitera"],"suffixes":[]},{"firstnames":["E."],"propositions":[],"lastnames":["Quintero"],"suffixes":[]},{"firstnames":["V."],"propositions":[],"lastnames":["Raymond"],"suffixes":[]},{"firstnames":["J.","G."],"propositions":[],"lastnames":["Rollins"],"suffixes":[]},{"firstnames":["V."],"propositions":[],"lastnames":["Sannibale"],"suffixes":[]},{"firstnames":["F."],"propositions":[],"lastnames":["Seifert"],"suffixes":[]},{"firstnames":["A."],"propositions":[],"lastnames":["Singer"],"suffixes":[]},{"firstnames":["L."],"propositions":[],"lastnames":["Singer"],"suffixes":[]},{"firstnames":["M.","R."],"propositions":[],"lastnames":["Smith"],"suffixes":[]},{"firstnames":["N.","D."],"propositions":[],"lastnames":["Smith-Lefebvre"],"suffixes":[]},{"firstnames":["R."],"propositions":[],"lastnames":["Taylor"],"suffixes":[]},{"firstnames":["M.","P."],"propositions":[],"lastnames":["Thirugnanasambandam"],"suffixes":[]},{"firstnames":["E."],"propositions":[],"lastnames":["Thrane"],"suffixes":[]},{"firstnames":["K.","S."],"propositions":[],"lastnames":["Thorne"],"suffixes":[]},{"firstnames":["S."],"propositions":[],"lastnames":["Vass"],"suffixes":[]},{"firstnames":["M."],"propositions":[],"lastnames":["Vallisneri"],"suffixes":[]},{"firstnames":["L."],"propositions":[],"lastnames":["Wallace"],"suffixes":[]},{"firstnames":["A.","J."],"propositions":[],"lastnames":["Weinstein"],"suffixes":[]},{"firstnames":["R."],"propositions":[],"lastnames":["Williams"],"suffixes":[]},{"firstnames":["H."],"propositions":[],"lastnames":["Yamamoto"],"suffixes":[]},{"firstnames":["H."],"propositions":[],"lastnames":["Yang"],"suffixes":[]},{"firstnames":["D."],"propositions":[],"lastnames":["Yeaton-Massey"],"suffixes":[]},{"firstnames":["L."],"propositions":[],"lastnames":["Zhang"],"suffixes":[]},{"firstnames":["J."],"propositions":[],"lastnames":["Zweizig"],"suffixes":[]},{"firstnames":["S.","B."],"propositions":[],"lastnames":["Anderson"],"suffixes":[]},{"firstnames":["N.","A."],"propositions":[],"lastnames":["Robertson"],"suffixes":[]},{"firstnames":["C.","I."],"propositions":[],"lastnames":["Torrie"],"suffixes":[]}],"note":"o̧pyright 2013 American Physical Society. Received 9 October 2013; published 13 December 2013. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom??a y Competitividad, the Conselleria d?Economia Hisenda i Innovacio? of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, OTKA of Hungary, 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 Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.","title":"Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts","publisher":"American Physical Society","year":"2013","journal":"Physical Review D","pages":"Article No. 122004","url":"http://resolver.caltech.edu/CaltechAUTHORS:20140130-095945569","abstract":"Long gamma-ray bursts (GRBs) have been linked to extreme core-collapse supernovae from massivestars. Gravitational waves (GW) offer a probe of the physics behind long GRBs. We investigate models of long-lived (\\textttḩar12610?1000 s) GW emission associated with the accretion disk of a collapsed star or with its protoneutron star remnant. Using data from LIGO?s fifth science run, and GRB triggers from the Swift experiment, we perform a search for unmodeled long-lived GW transients. Finding no evidence of GW emission, we place 90% confidence-level upper limits on the GW fluence at Earth from long GRBs for three waveforms inspired by a model of GWs from accretion disk instabilities. These limits range from F \\ensuremath< 3:5 ergs cm\\^ (-2) to F \\ensuremath< 1200 ergs cm\\^ (-2), depending on the GRB and on the model, allowing us to probe optimistic scenarios of GW production out to distances as far as $\\approx$ 33 Mpc. Advanced detectors are expected to achieve strain sensitivities 10x better than initial LIGO, potentially allowing us to probe the engines of the nearest long GRBs.","bibtex":"@article{caltechauthors43573,\n volume = {88},\n number = {12},\n month = {December},\n author = {J. Aasi and J. Abadie and B. P. Abbott and R. Abbott and M. R. Abernathy and R. X. Adhikari and P. Ajith and R. A. Anderson and K. Arai and M. C. Araya and L. Austin and J. C. Barayoga and G. Billingsley and E. Black and J. K. Blackburn and R. Bork and A. F. Brooks and C. Cepeda and R. Chakraborty and T. Chalermsongsak and Y. Chen and D. C. Coyne and B. Daudert and V. Dergachev and R. W. P. Drever and J. C. Driggers and P. Ehrens and T. Etzel and N. Fotopoulos and S. Gossan and K. E. Gushwa and E. K. Gustafson and E. Hall and J. Harms and J. Heefner and A. W. Heptonstall and K. A. Hodge and T. Hong and A. Ivanov and M. Jacobson and E. James and P. Kalmus and K. Kaufman and W. Kells and P. J. King and V. Kondrashov and W. Z. Korth and D. Kozak and A. Lazzarini and J. B. Lewis and D. Lloyd and J. Luan and M. Mageswaran and K. Mailand and E. Maros and D. Martynov and J. N. Marx and G. McIntyre and S. Meshkov and H. Miao and T. Nash and G. H. Ogin and C. Osthelder and C. D. Ott and M. Pedraza and M. Phelps and C. Poux and L. R. Price and S. Privitera and E. Quintero and V. Raymond and J. G. Rollins and V. Sannibale and F. Seifert and A. Singer and L. Singer and M. R. Smith and N. D. Smith-Lefebvre and R. Taylor and M. P. Thirugnanasambandam and E. Thrane and K. S. Thorne and S. Vass and M. Vallisneri and L. Wallace and A. J. Weinstein and R. Williams and H. Yamamoto and H. Yang and D. Yeaton-Massey and L. Zhang and J. Zweizig and S. B. Anderson and N. A. Robertson and C. I. Torrie},\n note = {{\\copyright} 2013 American Physical Society.\r\n\r\nReceived 9 October 2013; published 13 December 2013.\r\n\r\nThe authors gratefully acknowledge the support of the\r\nUnited States National Science Foundation for the construction\r\nand operation of the LIGO Laboratory, the\r\nScience and Technology Facilities Council of the United\r\nKingdom, the Max-Planck-Society, and the State of\r\nNiedersachsen/Germany for support of the construction\r\nand operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre\r\nNational de la Recherche Scientifique for the construction\r\nand operation of the Virgo detector. The authors also\r\ngratefully acknowledge the support of the research by\r\nthese agencies and by the Australian Research Council,\r\nthe International Science Linkages program of the\r\nCommonwealth of Australia, the Council of Scientific\r\nand Industrial Research of India, the Istituto Nazionale di\r\nFisica Nucleare of Italy, the Spanish Ministerio de\r\nEconom??a y Competitividad, the Conselleria d?Economia\r\nHisenda i Innovacio? of the Govern de les Illes Balears, the\r\nFoundation for Fundamental Research on Matter supported\r\nby the Netherlands Organisation for Scientific Research,\r\nthe Polish Ministry of Science and Higher Education, the\r\nFOCUS Programme of Foundation for Polish Science, the\r\nRoyal Society, the Scottish Funding Council, the Scottish\r\nUniversities Physics Alliance, The National Aeronautics\r\nand Space Administration, OTKA of Hungary, the Lyon\r\nInstitute of Origins (LIO), the National Research\r\nFoundation of Korea, Industry Canada and the Province\r\nof Ontario through the Ministry of Economic Development\r\nand Innovation, the National Science and Engineering\r\nResearch Council Canada, the Carnegie Trust, the\r\nLeverhulme Trust, the David and Lucile Packard\r\nFoundation, the Research Corporation, and the Alfred P.\r\nSloan Foundation.},\n title = {Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts},\n publisher = {American Physical Society},\n year = {2013},\n journal = {Physical Review D},\n pages = {Article No. 122004},\n url = {http://resolver.caltech.edu/CaltechAUTHORS:20140130-095945569},\n abstract = {Long gamma-ray bursts (GRBs) have been linked to extreme core-collapse supernovae from massivestars. Gravitational waves (GW) offer a probe of the physics behind long GRBs. We investigate models of long-lived ({\\texttt{\\char126}}10?1000 s) GW emission associated with the accretion disk of a collapsed star or with its\r\nprotoneutron star remnant. Using data from LIGO?s fifth science run, and GRB triggers from the Swift experiment, we perform a search for unmodeled long-lived GW transients. Finding no evidence of GW emission, we place 90\\% confidence-level upper limits on the GW fluence at Earth from long GRBs for\r\nthree waveforms inspired by a model of GWs from accretion disk instabilities. These limits range from F {\\ensuremath{<}} 3:5 ergs cm{\\^{ }}(-2) to F {\\ensuremath{<}} 1200 ergs cm{\\^{ }}(-2), depending on the GRB and on the model, allowing us to probe\r\noptimistic scenarios of GW production out to distances as far as {$\\approx$} 33 Mpc. Advanced detectors are expected to achieve strain sensitivities 10x better than initial LIGO, potentially allowing us to probe the engines of the nearest long GRBs.}\n}\n\n","author_short":["Aasi, J.","Abadie, J.","Abbott, B. P.","Abbott, R.","Abernathy, M. R.","Adhikari, R. X.","Ajith, P.","Anderson, R. A.","Arai, K.","Araya, M. C.","Austin, L.","Barayoga, J. C.","Billingsley, G.","Black, E.","Blackburn, J. K.","Bork, R.","Brooks, A. F.","Cepeda, C.","Chakraborty, R.","Chalermsongsak, T.","Chen, Y.","Coyne, D. C.","Daudert, B.","Dergachev, V.","Drever, R. W. P.","Driggers, J. C.","Ehrens, P.","Etzel, T.","Fotopoulos, N.","Gossan, S.","Gushwa, K. E.","Gustafson, E. K.","Hall, E.","Harms, J.","Heefner, J.","Heptonstall, A. W.","Hodge, K. A.","Hong, T.","Ivanov, A.","Jacobson, M.","James, E.","Kalmus, P.","Kaufman, K.","Kells, W.","King, P. J.","Kondrashov, V.","Korth, W. Z.","Kozak, D.","Lazzarini, A.","Lewis, J. B.","Lloyd, D.","Luan, J.","Mageswaran, M.","Mailand, K.","Maros, E.","Martynov, D.","Marx, J. N.","McIntyre, G.","Meshkov, S.","Miao, H.","Nash, T.","Ogin, G. H.","Osthelder, C.","Ott, C. D.","Pedraza, M.","Phelps, M.","Poux, C.","Price, L. R.","Privitera, S.","Quintero, E.","Raymond, V.","Rollins, J. G.","Sannibale, V.","Seifert, F.","Singer, A.","Singer, L.","Smith, M. R.","Smith-Lefebvre, N. D.","Taylor, R.","Thirugnanasambandam, M. P.","Thrane, E.","Thorne, K. S.","Vass, S.","Vallisneri, M.","Wallace, L.","Weinstein, A. J.","Williams, R.","Yamamoto, H.","Yang, H.","Yeaton-Massey, D.","Zhang, L.","Zweizig, J.","Anderson, S. B.","Robertson, N. A.","Torrie, C. I."],"key":"caltechauthors43573","id":"caltechauthors43573","bibbaseid":"aasi-abadie-abbott-abbott-abernathy-adhikari-ajith-anderson-etal-searchforlonglivedgravitationalwavetransientscoincidentwithlonggammaraybursts-2013","role":"author","urls":{"Paper":"http://resolver.caltech.edu/CaltechAUTHORS:20140130-095945569"},"downloads":0,"html":""},"search_terms":["search","long","lived","gravitational","wave","transients","coincident","long","gamma","ray","bursts","aasi","abadie","abbott","abbott","abernathy","adhikari","ajith","anderson","arai","araya","austin","barayoga","billingsley","black","blackburn","bork","brooks","cepeda","chakraborty","chalermsongsak","chen","coyne","daudert","dergachev","drever","driggers","ehrens","etzel","fotopoulos","gossan","gushwa","gustafson","hall","harms","heefner","heptonstall","hodge","hong","ivanov","jacobson","james","kalmus","kaufman","kells","king","kondrashov","korth","kozak","lazzarini","lewis","lloyd","luan","mageswaran","mailand","maros","martynov","marx","mcintyre","meshkov","miao","nash","ogin","osthelder","ott","pedraza","phelps","poux","price","privitera","quintero","raymond","rollins","sannibale","seifert","singer","singer","smith","smith-lefebvre","taylor","thirugnanasambandam","thrane","thorne","vass","vallisneri","wallace","weinstein","williams","yamamoto","yang","yeaton-massey","zhang","zweizig","anderson","robertson","torrie"],"keywords":[],"authorIDs":["5a0762140a821ce24800003b"],"dataSources":["87H4BDEWXjGHR2RTf"]}