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Search for Gravitational Waves Associated with<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>γ</mml:mi></mml:math>-ray Bursts Detected by the Interplanetary Network
J. Aasi, B. P. Abbott, R. Abbott, T. D. Abbott, M. R. Abernathy, F. Acernese, K. Ackley, C. Adams, T. Adams, P. Addesso, R. X. Adhikari, C. Affeldt, M. Agathos, N. Aggarwal, O. D. Aguiar, P. Ajith, A. Alemic, B. Allen, A. Allocca, D. Amariutei, M. Andersen, R. A. Anderson, S. B. Anderson, W. G. Anderson, K. Arai, M. C. Araya, C. C. Arceneaux, J. S. Areeda, S. Ast, S. M. Aston, P. Astone, P. Aufmuth, H. Augustus, C. Aulbert, B. E. Aylott, S. Babak, P. T. Baker, G. Ballardin, S. W. Ballmer, J. C. Barayoga, M. Barbet, B. C. Barish, D. Barker, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, M. A. Barton, I. Bartos, R. Bassiri, A. Basti, J. C. Batch, J. Bauchrowitz, Th. S. Bauer, C. Baune, V. Bavigadda, B. Behnke, M. Bejger, M. G. Beker, Krzysztof Belczyński, A. S. Bell, C. Bell, G. Bergmann, D. Bersanetti, A. Bertolini, J. Betzwieser, I. A. Bilenko, G. Billingsley, J. Birch, S. Biscans, M. Bitossi, C. Biwer, M. A. Bizouard, E. Black, J. K. Blackburn, Lindy Blackburn, D. G. Blair, S. Bloemen, O. Bock, T. P. Bodiya, M. Boër, G. Bogaert, C. Bogan, C. Bond, F. Bondu, L. Bonelli, R. Bonnand, R. Bork, M. Born, V. Boschi, S. Bose, L. Bosi, C. Bradaschia, P. R. Brady, V. B. Braginsky, M. Branchesi, J. E. Brau, T. Briant, D. O. Bridges, A. Brillet, M. Brinkmann, V. Brisson, A. F. Brooks, D. Brown, D. D. Brown, Frank Brückner, Saps Buchman, A. Buikema, T. Bulik, H. J. Bulten, A. Buonanno, R. Burman, D. Buskulic, C. Buy, L. Cadonati, G. Cagnoli, J. Calderón Bustillo, E. Calloni, J. B. Camp, P. Campsie, K. C. Cannon, B. Canuel, J. Cao, C. D. Capano, F. Carbognani, L. Carbone, S. Caride, Giuseppe Castaldi, S. Caudill, M. Cavaglià, F. Cavalier, R. Cavalieri, C. Celerier, G. Cella, C. Cepeda, E. Cesarini, R. Chakraborty, T. Chalermsongsak, S. J. Chamberlin, S. Chao, P. Charlton, E. Chassande‐Mottin, X. Chen, Yu‐Hung Chen, A. Chincarini, A. Chiummo, H. S. Cho, M. Cho, J. H. Chow, N. Christensen, Q. Chu, M. Cieślar, S. Chung, G. Ciani, F. Clara, Daniel E. Clark, J. A. Clark, J. H. Clayton, F. Cleva, E. Coccia, P.‐F. Cohadon, A. Colla, Christophe Collette, M. Colombini, L. Cominsky, M. Constancio, A. Conte, D. Cook, T. R. Corbitt, Neil J. Cornish, A. Corsi, C. A. Costa, M. W. Coughlin, J.‐P. Coulon, S. T. Countryman, P. Couvares, D. M. Coward, M. J. Cowart, D. C. Coyne, R. Coyne, K. Craig, J. D. E. Creighton, R. P. Croce, S. G. Crowder, A. Cumming, L. Cunningham, E. Cuoco, Curt Cutler, K. Dahl, T. Dal Canton, M. Damjanic, S. L. Danilishin, Salvatore D’Antonio, K. Danzmann, V. Dattilo, H. Daveloza, M. Davier, G. S. Davies, E. J. Daw, R. Day, T. Dayanga, D. DeBra, G. Debreczeni, J. Degallaix, S. Deléglise, W. Del Pozzo, T. Denker, T. Dent, H. Dereli, V. Dergachev, R. De Rosa, R. T. DeRosa, R. DeSalvo, S. Dhurandhar, M. C. Díaz, J. Dickson, L. Di Fiore, A. Di Lieto, I. Di Palma, A. Di Virgilio, V. Dolique, E. Dominguez, F. Donovan, K. L. Dooley, S. Doravari, R. Douglas, T. P. Downes, M. Drago, R. W. P. Drever, J. C. Driggers, Zhihui Du, S. E. Dwyer, T. Eberle, T. Edo, M. C. Edwards, A. Effler, H.‐B. Eggenstein, P. Ehrens, J. Eichholz, S. S. Eikenberry, G. Endrőczi, R C Essick, T. Etzel, M. Evans, T. M. Evans, M. Factourovich, V. Fafone, S. Fairhurst, X. Fan, Q. Fang, S. Farinon, B. Farr, Will M. Farr, M. Favata, D. Fazi, H. Fehrmann, M. M. Fejer, D. Feldbaum, F. Feroz, I. Ferrante, E. C. Ferreira, F. Ferrini, F. Fidecaro, L. S. Finn, I. Fiori, R. P. Fisher, R. Flaminio, J.-D. Fournier, Sebastián Franco, S. Frasca, F. Frasconi, M. Frede, Z. Frei, A. Freise, R. Frey, T. T. Fricke, P. Fritschel, V. V. Frolov, P. Fulda, M. Fyffe, J. R. Gair, L. Gammaitoni, S. G. Gaonkar, F. Garufi, N. Gehrels, G. Gemme, B. Gendre, E. Genin, A. Gennai, S. Ghosh, J. A. Giaime, K. D. Giardina, A. Giazotto, J. Gleason, E. Goetz, L. Gondán, G. González, Neil Gordon, M. L. Gorodetsky, S. E. Gossan, S. Goßler, R. Gouaty, Christian Gräf, P. B. Graff, M. Granata, A. Grant, S. Gras, C. Gray, R. J. S. Greenhalgh, A. M. Gretarsson, P. Groot, H. Grote, K. Grover, S. Grünewald, G. M. Guidi, C. Guido, K. Gushwa, E. K. Gustafson, R. Gustafson, J. Ha, E. D. Hall, W. O. Hamilton, D. Hammer, G. Hammond, M. M. Hanke, J. Hanks, C. Hanna, M. D. Hannam, J. Hanson, J. Harms, I. W. Harry, E. D. Harstad, M. J. Hart, M. T. Hartman, C.‐J. Haster, K. Haughian, A. Heidmann, M. C. Heintze, H. Heitmann, P. Hello, M. Hendry, I. S. Heng, A. W. Heptonstall, M. Heurs, M. Hewitson, S. Hild, D. Hoak, K. A. Hodge, D. Hofman, K. Holt, P. Hopkins, Travis Horrom, D. Hoske, D. J. Hosken, J. Hough, E. J. Howell, Yi-Ming Hu, E. A. Huerta, B. Hughey, S. Husa, S. H. Huttner, M. Huynh, T. Huynh–Dinh, A. Idrisy, D. R. Ingram, R. Inta, G. Islas, T. Isogai, A. Ivanov, B. R. Iyer, K. Izumi, M. Jacobson, H. Jang, P. Jaranowski, Y. Ji, F. Jiménez-Forteza, W. W. Johnson, D. I. Jones, R. Jones, R. J. G. Jonker, L. Ju, K. Haris, P. Kalmus, V. Kalogera, S. Kandhasamy, G. Kang, J. B. Kanner, J. Karlen, M. Kasprzack, E. Katsavounidis, W. Katzman, H. Kaufer, S. Kaufer, T. Kaur, K. Kawabe, F. Kawazoe, F. Kéfélian, G. M. Keiser, D. Keitel, Darcy B. Kelley, W. Kells, D. G. Keppel, A. Khalaidovski, F. Y. Khalili, Е. А. Хазанов, C. Kim, K. Kim, N. G. Kim, Nakwoo Kim, S. Kim, Y.-M. Kim, E. J. King, P. J. King, D. L. Kinzel, J. S. Kissel, S. Klimenko, J. Kline, S. M. Koehlenbeck, K. Kokeyama, V. Kondrashov, S. Koranda, W. Z. Korth, I. Kowalska, D. B. Kozak, V. Kringel, B. Krishnan, A. Królak, A. Kumar, D. Nanda Kumar, P. Kumar, S. Kumar, L. Kuo, A. Kutynia, Ping Koy Lam, M. Landry, B. Lantz, Shane L. Larson, P. D. Lasky, A. Lazzarini, C. Lazzaro, P. Leaci, S. Leavey, E. O. Lebigot, Chang‐Hwan Lee, H. K. Lee, Hyung Mok Lee, J. Lee, P. J. Lee, M. Leonardi, J. R. Leong, I. Leonor, A. Le Roux, N. Leroy, N. Letendre, Y. Levin, B. M. Levine, J. B. Lewis, T. G. F. Li, Kenneth G. Libbrecht, A. Libson, A. C. Lin, T. B. Littenberg, N. A. Lockerbie, Veronica Lockett-Ruiz, D. Lodhia, K. M. Loew, J. Logue, A. L. Lombardi, Ericson López, M. Lorenzini, V. Loriette, M. Lormand, G. Losurdo, J. D. Lough, M. J. Lubinski, H. Lück, A. P. Lundgren, Y. Ma, E. Macdonald, T. MacDonald, B. Machenschalk, M. MacInnis, D. M. Macleod, F. Magaña‐Sandoval, R. M. Magee, M. Mageswaran, C. Maglione, K. Mailand, E. Majorana, I. Maksimovic, V. Malvezzi, N. Man, G. M. Manca, Ilya Mandel, V. Mandic, V. Mangano, N. M. Mangini, G. L. Mansell, M. Mantovani, F. Marchesoni, F. Marion, Szabolcs Márka, Z. Márka, A. S. Markosyan, E. Maros, J. Marque, F. Martelli, I. W. Martin, R. M. Martin, L. Martinelli, Д. В. Мартынов, J. N. Marx, K. Mason, A. Masserot, T. J. Massinger, F. Matichard, L. Matone, N. Mavalvala, G. May, N. Mazumder, G. Mazzolo, R. McCarthy, D. E. McClelland, S. C. McGuire, G. McIntyre, J. McIver, K. McLin, D. Meacher, G. D. Meadors, M. Mehmet, J. Meidam, M. Meinders, A. Melatos, G. Mendell, R. A. Mercer, S. Meshkov, C. Messenger, M. S. Meyer, P. M. Meyers, F. Mezzani, H. Miao, C. Michel, Е. Е. Михайлов, L. Milano, J. Miller, Y. Minenkov, Chiara M. F. Mingarelli, C. Mishra, S. Mitra, V. P. Mitrofanov, G. Mitselmakher, R. Mittleman, B. Moe, A. Moggi, M. Mohan, S. R. P. Mohapatra, D. Moraru, G. Moreno, N. Morgado, S. R. Morriss, K. Mossavi, B. Mours, C. M. Mow–Lowry, C. Mueller, G. Mueller, Suvodip Mukherjee, A. Mullavey, J. Münch, D. Murphy, P. G. Murray, A. Mytidis, M. F. Nagy, I. Nardecchia, L. Naticchioni, R. K. Nayak, V. Necula, G. Nelemans, I. Neri, M. Néri, G. Newton, T. Nguyen, Alex B. Nielsen, S. Nissanke, A. Nitz, F. Nocera, D. Nolting, M. E. N. Normandin, L. K. Nuttall, E. Ochsner, J. O’Dell, E. Oelker, J. J. Oh, S. H. Oh, F. Ohme, S. Omar, P. Oppermann, Richard J. Oram, B. O’Reilly, W. Ortega, R. O’Shaughnessy, C. Osthelder, D. J. Ottaway, R. S. Ottens, H. Overmier, B. J. Owen, A. Pai, O. Palashov, C. Palomba, H. Pan, Y. Pan, C. Pankow, F. Paoletti, M. A. Papa, H. Paris, A. Pasqualetti, R. Passaquieti, D. Passuello, M. Pedraza, A. Pele, A. Perreca, M. Phelps, M. Pichot, M. Pickenpack, F. Piergiovanni, V. Pierro, L. Pinard, I. M. Pinto, M. Pitkin, J. Poeld, R. Poggiani, A. K. Poteomkin, J. Powell, J. Prasad, V. Predoi, S. Premachandra, T. Prestegard, Larry R. Price, M. Prijatelj, S. Privitera, G. A. Prodi, L. Prokhorov, O. Puncken, M. Punturo, P. Puppo, M. Pürrer, J. Qin, V. Quetschke, E. A. Quintero, R. Quitzow-James, F. J. Raab, D. S. Rabeling, István Rácz, H. Radkins, P. Raffai, S. Raja, G Rajalakshmi, M. Rakhmanov, C. Ramet, K. E. Ramirez, P. Rapagnani, V. Raymond, M. Razzano, V. Re, Sarah Recchia, C. M. Reed, T. Regimbau, S. Reid, D. H. Reitze, Oscar Reula, E. Rhoades, R. Riesen, K. Riles, N. A. Robertson, F. Robinet, A. Rocchi, S. B. Roddy, L. Rolland, J. G. Rollins, R. Romano, G. Romanov, J. H. Romie, D. Rosińska, S. Rowan, A. Rüdiger, P. Ruggi, K. Ryan, F. Salemi, L. Sammut, V. Sandberg, J. R. Sanders, S. Sankar, V. Sannibale, I. Santiago-Prieto, E. Saracco, B. Sassolas, B. S. Sathyaprakash, P. R. Saulson, R. L. Savage, Jacob Scheuer, R. Schilling, M. Schilman, P. Schmidt, R. Schnabel, R. M. S. Schofield, E. Schreiber, D. Schuette, B. F. Schutz, J. Scott, S. M. Scott, D. Sellers, A. S. Sengupta, D. Sentenac, V. Sequino, A. Sergeev, D. A. Shaddock, S. Shah, M. S. Shahriar, M. Shaltev, Z. Shao, B. Shapiro, P. Shawhan, D. H. Shoemaker, T. L. Sidery, K. Siellez, X. Siemens, D. Sigg, D. Simakov, A. Singer, L. Singer, R. Singh, A. M. Sintes, B. J. J. Slagmolen, J. Slutsky, J. R. Smith, M. R. Smith, R. J. E. Smith, N. D. Smith-Lefebvre, E. J. Son, B. Sorazu, T. Souradeep, A. Staley, J. Stebbins, M. Steinke, J. Steinlechner, S. Steinlechner, B. C. Stephens, S. Steplewski, S. P. Stevenson, R. Stone, D. J. Stops, K. A. Strain, N. Straniero, S. Strigin, R. Sturani, A. L. Stuver, T. Z. Summerscales, S. Susmithan, P. J. Sutton, B. L. Swinkels, M. Tacca, D. Talukder, D. B. Tanner, Jian Tao, S. P. Tarabrin, R. Taylor, G. Tellez, M. P. Thirugnanasambandam, M. Thomas, P. Thomas, K. A. Thorne, K. S. Thorne, E. Thrane, V. Tiwari, K. V. Tokmakov, C. Tomlinson, M. Tonelli, C. Torres, F. Travasso, G. Traylor, M. Tse, D. Tshilumba, H. Tuennermann, D. Ugolini, C. S. Unnikrishnan, A. L. Urban, S. A. Usman, H. Vahlbruch, G. Vajente, G. Valdes, M. Vallisneri, J. F. J. van den Brand, Marc van der Sluys, J. V. van Heijningen, A. A. van Veggel, S. Vass, M. Vasúth, R. Vaulin, A. Vecchio, G. Vedovato, J. Veitch, P. J. Veitch, K. Venkateswara, D. Verkindt, F. Vetrano, A. Viceré, R. Vincent-Finley, J.-Y. Vinet, S. Vitale, T. Vo, H. Vocca, C. Vorvick, W. D. Vousden, S. P. Vyachanin, A. R. Wade, L. E. Wade, M. Wade, M. Walker, L. Wallace, S. Walsh, M. Wang, X. Wang, R. L. Ward, M. Wąs, B. Weaver, L.‐W. Wei, M. Weinert, A. J. Weinstein, R. Weiss, T. Welborn, L. Wen, P. Weßels, M. West, T. Westphal, K. Wette, J. T. Whelan, David White, B. F. Whiting, K. Wiesner, C. Wilkinson, Kurtis A. Williams, L. Williams, R. Williams, T. D. Williams, A. R. Williamson, J. L. Willis, B. Willke, M. H. Wimmer, W. Winkler, C. C. Wipf, A. G. Wiseman, H. Wittel, G. Woan, N. Wolovick, J. Worden, Yuxuan Wu, J. Yablon, I. Yakushin, W. Yam, H. Yamamoto, C. C. Yancey, Huan Yang, S. Yoshida, M. Yvert, A. Zadrożny, M. Zanolin, J.-P. Zendri, Fan Zhang, L. Zhang, C. Zhao, H. Zhu, X. J. Zhu, M. E. Zucker, S. E. Zuraw, J. Zweizig, R. L. Aptekar, J. L. Atteia, T. Cline, V. Connaughton, D. Frederiks, S. Golenetskii, K. Hurley, H. A. Krimm, M. Marisaldi, V. Pal'Shin, D. M. Palmer, D. Svinkin, Y. Terada, A. von Kienlin
Bibliographic record
VenuePhysical Review Letters · 2014
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsCanadian Institute for Theoretical AstrophysicsPerimeter InstituteUniversity of Toronto
FundersIstituto Nazionale di Fisica NucleareMinistero dello Sviluppo EconomicoMax-Planck-GesellschaftAustralian Research CouncilNational Research Foundation of KoreaMinisterio de Economía y CompetitividadCentre National de la Recherche ScientifiqueIndustry CanadaGovern de les Illes BalearsFundacja na rzecz Nauki PolskiejScottish Funding CouncilInstitut des Origines de LyonScottish Universities Physics AllianceHungarian Scientific Research FundLeverhulme TrustNederlandse Organisatie voor Wetenschappelijk OnderzoekCouncil of Scientific and Industrial Research, IndiaScience and Technology Facilities CouncilNational Research FoundationAlfred P. Sloan FoundationNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsPhysicsGravitational waveAstrophysicsLIGONeutron starSkyCoalescence (physics)PopulationBinary numberAstronomyInterplanetary spaceflightGamma-ray burstAlgorithmComputer science
Abstract
We present the results of a search for gravitational waves associated with 223 γ-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M⊙c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.
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How this classification was reachedexpand
Full frame machine prediction
Teacher imitationNot calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.
metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.002
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.005
Threshold uncertainty score0.011
Distilled classifier scores by category (both heads)
| Category | Codex | Gemma |
|---|---|---|
| Metaresearch | 0.000 | 0.002 |
| Meta-epidemiology (narrow) | 0.000 | 0.000 |
| Meta-epidemiology (broad) | 0.000 | 0.000 |
| Bibliometrics | 0.001 | 0.001 |
| Science and technology studies | 0.000 | 0.000 |
| Scholarly communication | 0.001 | 0.000 |
| Open science | 0.000 | 0.000 |
| Research integrity | 0.000 | 0.000 |
| Insufficient payload (model declined to judge) | 0.002 | 0.000 |
Machine scores (provisional)
The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.
Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.
Opus teacher head0.013
GPT teacher head0.247
Teacher spread0.234 · how far apart the two teachers sit on this one work
Validation status
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from itClassification
machine, unvalidatedMachine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.
The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical
How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".
Quick stats
Citations43
Published2014
Admission routes2
Has abstractyes