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Search for gravitational-wave bursts in LIGO data from the fourth science run
B. Abbott, R. Abbott, R. X. Adhikari, J. Agresti, P. Ajith, B. Allen, R. Amin, S. B. Anderson, W. G. Anderson, M. A. 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, 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, Robert L. Byer, L. Cadonati, G. Cagnoli, J. B. Camp, J. K. Cannizzo, K. C. Cannon, C. A. Cantley, J. Cao, L. Cardenas, M. M. Casey, Giuseppe Castaldi, C. Cepeda, E. Chalkey, P. Charlton, S. Chatterji, S. Chelkowski, Y Chen, F. Chiadini, E. Chin, J. H. Chow, N. Christensen, J. A. Clark, P. Cochrane, Thomas Cokelaer, C. N. Colacino, R. L. Coldwell, R. Conte, D. Cook, T. R. Corbitt, D. M. Coward, D. C. Coyne, J. D. E. Creighton, R. P. Croce, D. R. M. Crooks, A. M. Cruise, A. Cumming, James Dalrymple, E D'Ambrosio, K. Danzmann, G. S. Davies, D. DeBra, J. Degallaix, M. Degree, T. Demma, V. Dergachev, S. Desai, R. DeSalvo, S. Dhurandhar, M Díaz, J. Dickson, A. Di Credico, G. Diederichs, A. Dietz, 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. M. 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, В. В. Фролов, M. Fyffe, Vincenzo Galdi, 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, 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, Ben A. Johnson, W. W. Johnson, 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. Kim, Peter 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, P. E. Lindquist, N. A. Lockerbie, 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, T. Nash, G. Newton, A. Nishizawa, Kenji Numata, B. O’Reilly, R. O’Shaughnessy, D. J. Ottaway, H. Overmier, B. J. Owen, Y. Pan, M. A. Papa, V. Parameshwaraiah, P. Patel, M. Pedraza, Jason S. Pelc, S. Penn, 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, H. Rehbein, S. Reid, D. H. Reitze, L. Ribichini, 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, R. K. Route, S. Rowan, A. Rüdiger, Laurent Ruet, P. Russell, K. Ryan, S. Sakata, M. Samidi, L. Sancho de la Jordana, V. Sandberg, V. Sannibale, S. Saraf, P. Sarin, B. S. Sathyaprakash, S. Sato, P. R. Saulson, R. L. Savage, P. Savov, 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, James A. 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, D. M. Strom, A. L. Stuver, T. Z. Summerscales, K-X Sun, M. Sung, P. J. Sutton, Hirotaka Takahashi, D. B. Tanner, M. Tarallo, R. Taylor, 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. Varvella, S. Vass, A. Vecchio, J. Veitch, P Veitch, A. Villar, C Vorvick, S. P. Vyachanin, S. J. Waldman, L. Wallace, R. L. Ward, K. Watts, D. Webber, Adam M. Weidner, M. Weinert, A. J. Weinstein, R. Weiss, S. Wen, K. Wette, J. T. Whelan, D. M. Whitbeck, S. E. Whitcomb, B. F. Whiting, C. Wilkinson, P A 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, J. Zhang, L. Zhang, C. Zhao, N. Zotov, M. E. Zucker, H. zur Mühlen, J. Zweizig
Why this work is in the frame
A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.
fundA Canadian funder is recorded on the work.
no affNo Canadian affiliation: this work is invisible to an affiliation-only frame.
No Canadian affiliation. An affiliation-only frame, the usual design, would never have seen this work. It is one of the works that make the case for inverting the frame.
Bibliographic record
VenueClassical and Quantum Gravity · 2007
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersScience and Technology Facilities CouncilGovern de les Illes BalearsIstituto Nazionale di Fisica NucleareScottish Funding CouncilScottish Universities Physics AllianceLeverhulme TrustAlexander von Humboldt-StiftungCouncil of Scientific and Industrial Research, IndiaNatural Sciences and Engineering Research Council of CanadaAlfred P. Sloan FoundationNational Science FoundationJohn Simon Guggenheim Memorial FoundationNational Aeronautics and Space Administration
KeywordsLIGOPhysicsGravitational waveAmplitudeSpurious relationshipAstrophysicsAstronomical interferometerSensitivity (control systems)Einstein TelescopeWaveformNoise (video)AstronomyInterferometryOpticsStatisticsQuantum mechanics
Abstract
The fourth science run of the LIGO and GEO 600 gravitational-wave detectors, carried out in early 2005, collected data with significantly lower noise than previous science runs. We report on a search for short-duration gravitationalwave bursts with arbitrary waveform in the 64-1600 Hz frequency range appearing in all three LIGO interferometers. Signal consistency tests, data quality cuts and auxiliary-channel vetoes are applied to reduce the rate of spurious triggers. No gravitational-wave signals are detected in 15.5 days of live observation time; we set a frequentist upper limit of 0.15 day -1 (at 90% confidence level) on the rate of bursts with large enough amplitudes to be detected reliably. The amplitude sensitivity of the search, characterized using Monte Carlo simulations, is several times better than that of previous searches. We also provide rough estimates of the distances at which representative supernova and binary black hole merger signals could be detected with 50% efficiency by this analysis.
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.
Full frame distilled prediction
Teacher imitationNot calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.
metaresearch head score (Codex)0.002
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.428
Threshold uncertainty score0.368
Codex and Gemma teacher scores by category
| Category | Codex | Gemma |
|---|---|---|
| Metaresearch | 0.002 | 0.000 |
| Meta-epidemiology (narrow) | 0.000 | 0.000 |
| Meta-epidemiology (broad) | 0.000 | 0.000 |
| Bibliometrics | 0.000 | 0.000 |
| Science and technology studies | 0.000 | 0.001 |
| Scholarly communication | 0.000 | 0.000 |
| Open science | 0.001 | 0.000 |
| Research integrity | 0.000 | 0.000 |
| Insufficient payload (model declined to judge) | 0.000 | 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 head0.077
GPT teacher head0.387
Teacher spread0.310 · 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 itQuick stats
Citations99
Published2007
Admission routes1
Has abstractyes