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Record W2138063398 · doi:10.1103/physrevd.77.062004

Search for gravitational waves associated with 39 gamma-ray bursts using data from the second, third, and fourth LIGO runs

2008· article· en· W2138063398 on OpenAlexfundno aff
B. Abbott, R. Abbott, R. X. Adhikari, J. Agresti, P. Ajith, B. Allen, R. Amin, S. B. Anderson, W. G. Anderson, M. Arain, M. Araya, H. Armandula, M. C. B. Ashley, S. M. Aston, P. Aufmuth, C. Aulbert, S. Ballmer, H. Bantilan, B. C. Barish, C. Barker, D. Barker, B. Barr, M. A. Barton, K. Bayer, Krzysztof Belczyński, S. J. Berukoff, J. Betzwieser, P. T. Beyersdorf, B. Bhawal, I. A. Bilenko, G. Billingsley, R. Biswas, E. Black, K. Blackburn, Lindy Blackburn, D. G. Blair, B. Bland, J. Bogenstahl, L. Bogue, R. Bork, V. Boschi, S. Bose, P. R. Brady, V. B. Braginsky, J. E. Brau, M. Brinkmann, A. F. Brooks, D. Brown, A. Bullington, A. Bunkowski, A. Buonanno, O. Burmeister, D. Busby, William E. Butler, Robert L. Byer, L. Cadonati, G. Cagnoli, J. B. Camp, J. K. Cannizzo, K. C. Cannon, C. A. Cantley, J. Cao, L. Cardenas, K. Carter, M. M. Casey, Giuseppe Castaldi, C. Cepeda, E. Chalkley, P. Charlton, S. Chatterji, S. Chelkowski, Y. Chen, F. Chiadini, A. Taracchini, E. Chin, J. H. Chow, N. Christensen, J. A. Clark, P. Cochrane, Thomas Cokelaer, C. N. Colacino, R. L. Coldwell, M. Coles, R. Conte, D. Cook, T. R. Corbitt, D. M. Coward, D. Coyne, J. D. E. Creighton, R. P. Croce, D. R. M. Crooks, A. M. Cruise, P. Csatorday, A. Cumming, James Dalrymple, E. D’Ambrosio, K. Danzmann, G. S. Davies, E. J. Daw, D. DeBra, J. Degallaix, M. Degree, T. Delker, T. Demma, V. Dergachev, S. Desai, R. DeSalvo, S. Dhurandhar, M. Díaz, J. Dickson, A. Di Credico, G. Diederichs, A. Dietz, H. Ding, E. E. Doomes, R. W. P. Drever, J.-C. Dumas, R. J. Dupuis, J. G. Dwyer, P. Ehrens, Eduardo Espinoza, T. Etzel, M. Evans, T. Evans, S. Fairhurst, Y. Fan, D. Fazi, M. M. Fejer, L. S. Finn, V. Fiumara, N. Fotopoulos, A. Franzen, K. Y. Franzen, A. Freise, R. Frey, T. T. Fricke, P. Fritschel, V. V. Frolov, M. Fyffe, Vincenzo Galdi, K. S. Ganezer, J. A. Garofoli, I. Gholami, J. A. Giaime, S. Giampanis, K. D. Giardina, Keisuke Goda, E. Goetz, L. M. Goggin, G. González, S. Goßler, A. Grant, S. Gras, C. Gray, M. Gray, J. Greenhalgh, A. M. Gretarsson, R. Grosso, H. Grote, S. Grünewald, M. Guenther, R. Gustafson, B. Hage, D. Hammer, C. Hanna, J. Hanson, J. Harms, I. W. Harry, E. D. Harstad, T. Hayler, J. Heefner, Gerhard Heinzel, I. S. Heng, A. Heptonstall, M. Heurs, M. Hewitson, S. Hild, E. Hirose, D. Hoak, D. J. Hosken, J. Hough, E. J. Howell, D. Hoyland, S. H. Huttner, D. R. Ingram, E. Innerhofer, Masahiro Ito, Y. Itoh, A. Ivanov, D. Jackrel, O. Jennrich, Ben A. Johnson, W. W. Johnson, W. R. Johnston, D. I. Jones, Gareth Jones, R. Jones, L. Ju, P. Kalmus, V. Kalogera, Dimitri Kasprzyk, E. Katsavounidis, K. Kawabe, Seiji Kawamura, F. Kawazoe, W. Kells, D. G. Keppel, F. Y. Khalili, C. J. Killow, C. Kim, P. J. King, J. S. Kissel, S. Klimenko, K. Kokeyama, V. Kondrashov, Ravi Kopparapu, D. B. Kozak, B. Krishnan, P. Kwee, Ping Koy Lam, M. Landry, B. Lantz, A. Lazzarini, B. Lee, Mingxing Lei, J. Leiner, V. Leonhardt, I. Leonor, Kenneth G. Libbrecht, A. Libson, P. E. Lindquist, N. A. Lockerbie, J. Logan, M. Longo, M. Lormand, M. Lubinski, H. Lück, B. Machenschalk, M. MacInnis, M. Mageswaran, K. Mailand, M. Malec, V. Mandic, Stefano Maranò, S. Márka, J. Markowitz, E. Maros, I. W. Martin, J. N. Marx, K. Mason, L. Matone, Vincenzo Matta, N. Mavalvala, R. McCarthy, D. E. McClelland, S. C. McGuire, M. McHugh, Kirk McKenzie, J. W. C. McNabb, S. T. McWilliams, T. Meier, A. C. Melissinos, G. Mendell, R. A. Mercer, S. Meshkov, Eirini Messaritaki, C. Messenger, D. Meyers, Е. Е. Михайлов, S. Mitra, V. P. Mitrofanov, G. Mitselmakher, R. Mittleman, O. Miyakawa, Soumya D. Mohanty, G. Moreno, K. Mossavi, C. M. Mow–Lowry, A. Moylan, D. Mudge, G. Mueller, S. Mukherjee, H. Müller‐Ebhardt, J. Münch, P. G. Murray, E. Myers, J. Myers, S. Nagano, T. Nash, G. Newton, A. Nishizawa, F. Nocera, Kenji Numata, P. Nutzman, B. O’Reilly, R. O’Shaughnessy, D. J. Ottaway, H. Overmier, B. J. Owen, Y. Pan, M. A. Papa, V. Parameshwaraiah, C. Parameswariah, P. Patel, M. Pedraza, V. Pierro, I. M. Pinto, M. Pitkin, H. J. Pletsch, M. V. Plissi, F. Postiglione, R. Prix, V. Quetschke, F. J. Raab, D. S. Rabeling, H. Radkins, R. Rahkola, N. Rainer, M. Rakhmanov, M. Ramsunder, K. Rawlins, S. Ray‐Majumder, V. Re, T. Regimbau, H. Rehbein, S. Reid, D. H. Reitze, L. Ribichini, S. Richman, R. Riesen, K. Riles, B. Rivera, N. A. Robertson, C. Robinson, E. L. Robinson, S. Roddy, A. Rodriguez, A. M. Rogan, J. G. Rollins, J. D. Romano, Haisheng Rong, R. K. Route, S. Rowan, A. Rüdiger, Laurent Ruet, P. Russell, K. Ryan, S. Sakata, M. Samidi, L. Sancho de la Jordana, V. Sandberg, G. H. Sanders, V. Sannibale, S. Saraf, P. Sarin, B. S. Sathyaprakash, S. Sato, P. R. Saulson, R. L. Savage, P. Savov, A. Sazonov, Sascha Schediwy, R. Schilling, R. Schnabel, R. M. S. Schofield, B. F. Schutz, P. Schwinberg, S. M. Scott, A. C. Searle, B. Sears, Frank Seifert, D. Sellers, A. S. Sengupta, P. Shawhan, D. H. Shoemaker, A. Sibley, John A. Sidles, X. Siemens, D. Sigg, Sidhartha R. Sinha, A. M. Sintes, B. J. J. Slagmolen, J. Slutsky, J. R. Smith, M. Smith, K. Somiya, K. A. Strain, Natalie E. Strand, D. M. Strom, A. L. Stuver, T. Z. Summerscales, Ke-Xun Sun, M. Sung, P. J. Sutton, Julien Sylvestre, Hirotaka Takahashi, A. Takamori, D. B. Tanner, M. Tarallo, R. Taylor, John G. Thacker, K. A. Thorne, K. S. Thorne, A. Thüring, Massimo Tinto, K. V. Tokmakov, C. Torres, C. Torrie, G. Traylor, Miquel Trias, W. Tyler, D. Ugolini, C. Ungarelli, Karel Urbánek, H. Vahlbruch, M. Vallisneri, M. van Putten, M. Varvella, S. Vass, A. Vecchio, J. Veitch, P. J. Veitch, A. Villar, C. Vorvick, S. P. Vyachanin, S. J. Waldman, L. Wallace, R. L. Ward, K. Watts, D. Webber, A. Weidner, M. Weinert, A. J. Weinstein, R. Weiss, L. Wen, S. Wen, K. Wette, J. T. Whelan, D. M. Whitbeck, S. E. Whitcomb, B. F. Whiting, S. Wiley, C. Wilkinson, Patrick Willems, L. Williams, B. Willke, I. Wilmut, W. Winkler, C. C. Wipf, S. Wise, A. G. Wiseman, G. Woan, D. Woods, R. Wooley, J. Worden, W. L. K. Wu, I. Yakushin, H. Yamamoto, Z. Yan, S. Yoshida, Nicolás Yunes, K. D. Zaleski, M. Zanolin, J. Zhang, L. Zhang, C. Zhao, N. Zotov, M. E. Zucker, H. zur Mühlen, J. Zweizig

Bibliographic record

VenuePhysical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2008
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaAustralian Research CouncilAlexander von Humboldt-StiftungCouncil of Scientific and Industrial Research, IndiaAlfred P. Sloan FoundationNational Aeronautics and Space AdministrationLeverhulme TrustDavid and Lucile Packard FoundationJohn Simon Guggenheim Memorial FoundationNational Science Foundation
KeywordsLIGOGravitational wavePhysicsGamma-ray burstAstrophysicsPopulationAmplitudeWaveformInterferometryAstronomyOpticsQuantum mechanics

Abstract

fetched live from OpenAlex

We present the results of a search for short-duration gravitational-wave bursts associated with 39 gamma-ray bursts (GRBs) detected by gamma-ray satellite experiments during LIGO's S2, S3, and S4 science runs. The search involves calculating the crosscorrelation between two interferometer data streams surrounding the GRB trigger time. We search for associated gravitational radiation from single GRBs, and also apply statistical tests to search for a gravitational-wave signature associated with the whole sample. For the sample examined, we find no evidence for the association of gravitational radiation with GRBs, either on a single-GRB basis or on a statistical basis. Simulating gravitational-wave bursts with sine-Gaussian waveforms, we set upper limits on the root-sum-square of the gravitational-wave strain amplitude of such waveforms at the times of the GRB triggers. We also demonstrate how a sample of several GRBs can be used collectively to set constraints on population models. The small number of GRBs and the significant change in sensitivity of the detectors over the three runs, however, limits the usefulness of a population study for the S2, S3, and S4 runs. Finally, we discuss prospects for the search sensitivity for the ongoing S5 run, and beyond for the next generation of detectors.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not 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)0.001
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 score0.008
Threshold uncertainty score0.016

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0030.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.043
GPT teacher head0.331
Teacher spread0.287 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine 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

Citations86
Published2008
Admission routes1
Has abstractyes

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Same venuePhysical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmologySame topicGamma-ray bursts and supernovaeFrench-language works237,207