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Record W2116856061 · doi:10.1103/physrevd.69.122001

Analysis of LIGO data for gravitational waves from binary neutron stars

2004· article· en· W2116856061 on OpenAlexfundno aff
B. Abbott, R. Abbott, R. X. Adhikari, A. Ageev, B. Allen, R. Amin, S. B. Anderson, W. G. Anderson, M. Araya, H. Armandula, F. Asiri, P. Aufmuth, C. Aulbert, Рамачандран Баласубраманиан, S. W. Ballmer, B. C. Barish, D. Barker, C. Barker-Patton, M. Barnes, B. Barr, M. A. Barton, K. Bayer, Raymond G. Beausoleil, Krzysztof Belczyński, R. Bennett, S. J. Berukoff, J. Betzwieser, B. Bhawal, I. A. Bilenko, G. Billingsley, E. Black, K. Blackburn, B. Bland-Weaver, B. Bochner, L. Bogue, R. Bork, S. Bose, P. R. Brady, V. B. Braginsky, J. E. Brau, D. Brown, S. Brozek, A. Bullington, A. Buonanno, R. Burgess, D. Busby, William E. Butler, Robert L. Byer, L. Cadonati, G. Cagnoli, J. B. Camp, C. A. Cantley, L. Cardenas, K. Carter, M. M. Casey, J. Castiglione, A. Chandler, J. Chapsky, P. Charlton, S. Chatterji, Y. Chen, V. Chickarmane, A. Taracchini, N. Christensen, D. Churches, C. N. Colacino, R. L. Coldwell, M. Coles, D. Cook, T. R. Corbitt, D. Coyne, J. D. E. Creighton, D. R. M. Crooks, P. Csatorday, B. J. Cusack, Curt Cutler, E. D’Ambrosio, K. Danzmann, R. Davies, E. J. Daw, D. DeBra, T. Delker, R. DeSalvo, S. Dhurandhar, M. Díaz, H. Ding, R. W. P. Drever, R. J. Dupuis, C. Ebeling, Jeffrey A. Edlund, P. Ehrens, E. J. Elliffe, T. Etzel, M. Evans, T. M. Evans, Carsten Fallnich, D. Farnham, M. M. Fejer, M. Fine, L. S. Finn, Éanna É. Flanagan, A. Freise, R. Frey, P. Fritschel, В. В. Фролов, M. Fyffe, K. S. Ganezer, J. A. Giaime, A. Gillespie, Keisuke Goda, G. González, S. Goßler, Philippe Grandclément, A. Grant, C. Gray, A. M. Gretarsson, D. Grimmett, H. Grote, S. Grünewald, M. Guenther, E. K. Gustafson, R. Gustafson, W. O. Hamilton, M. Hammond, J. Hanson, C. Hardham, I. W. Harry, A. Hartunian, J. Heefner, Y. Hefetz, Gerhard Heinzel, I. S. Heng, M. Hennessy, N. Hepler, A. Heptonstall, M. Heurs, M Hewitson, Neil Hindman, P. Hoang, J. Hough, M. Hrynevych, W. Hua, Richard Ingley, Masahiro Ito, Y. Itoh, A. Ivanov, O. Jennrich, W. W. Johnson, W. R. Johnston, Lynne Jones, Dieter Jungwirth, V. Kalogera, E. Katsavounidis, K. Kawabe, Seiji Kawamura, W. Kells, Jonathan Kern, A. Khan, S. Killbourn, C. J. Killow, C. Kim, C. King, Peter King, S. Klimenko, P. Kloevekorn, S. Koranda, K. Kötter, J. Kovalik, D. B. Kozak, B. Krishnan, M. Landry, John Langdale, B. Lantz, R. Lawrence, A. Lazzarini, Mingxing Lei, V. Leonhardt, I. Leonor, Kenneth G. Libbrecht, P. E. Lindquist, S. Liu, J. Logan, M. Lormand, M. Lubinski, H. Lück, T. T. Lyons, B. Machenschalk, M. MacInnis, M. Mageswaran, K. Mailand, Walid A. Majid, M. Malec, F.M. Mann, A. Marin, Szabolcs Márka, E. Maros, James Mason, K. Mason, O. Matherny, L. Matone, N. Mavalvala, R. McCarthy, D. E. McClelland, M. McHugh, P. Mcnamara, G. Mendell, S. Meshkov, C. Messenger, V. P. Mitrofanov, G. Mitselmakher, R. Mittleman, O. Miyakawa, S. Miyoki, S. Mohanty, G. Moreno, K. Mossavi, B. Mours, G. Mueller, Suvodip Mukherjee, J. Myers, S. Nagano, T. Nash, Holger Naundorf, R. K. Nayak, G. Newton, F. Nocera, P. Nutzman, T. Olson, B. O’Reilly, D. J. Ottaway, Adrian C. Ottewill, D. Ouimette, H. Overmier, B. J. Owen, M. A. Papa, C. Parameswariah, V. Parameswariah, M. Pedraza, M. Pitkin, M. V. Plissi, M. R. Pratt, V. Quetschke, F. J. Raab, H. Radkins, R. Rahkola, M. Rakhmanov, Shanti Rao, D. Redding, M. W. Regehr, T. Regimbau, K. T. Reilly, K. Reithmaier, D. H. Reitze, S. Richman, R. Riesen, K. Riles, Anthony Rizzi, D. I. Robertson, N. A. Robertson, L. Robison, S. Roddy, J. G. Rollins, J. D. Romano, J. Romie, Haisheng Rong, D. Rose, E. Rotthoff, S. Rowan, A. Rüdiger, P. Russell, K. Ryan, I. Salzman, G. H. Sanders, V. Sannibale, B. S. Sathyaprakash, P. R. Saulson, R. L. Savage, A. Sazonov, R. Schilling, Kevin C. Schlaufman, V. Schmidt, R. Schofield, M. Schrempel, B. F. Schutz, P. Schwinberg, S. M. Scott, A. C. Searle, B. Sears, S. Seel, A. S. Sengupta, Charles Shapiro, P. Shawhan, D. H. Shoemaker, Q. Z. Shu, A. Sibley, X. Siemens, L. Sievers, D. Sigg, A. M. Sintes, K. D. Skeldon, J. R. Smith, M. Smith, P. Sneddon, Robert Spero, G. Stapfer, K. A. Strain, D. Strom, A. L. Stuver, T. Z. Summerscales, M. C. Sumner, P. J. Sutton, Julien Sylvestre, A. Takamori, D. B. Tanner, H. Tariq, Ian Taylor, R. Taylor, K. S. Thorne, M. Tibbits, S. Tilav, Massimo Tinto, K. V. Tokmakov, C. Torres, C. Torrie, S. Traeger, G. Traylor, W. Tyler, D. Ugolini, M. Vallisneri, M. van Putten, S. Vass, A. Vecchio, C. Vorvick, S. P. Vyachanin, L. Wallace, H. Walther, R. L. Ward, Brent Ware, K. Watts, D. Webber, A. Weidner, U. Weiland, Allan J. Weinstein, R. Weiss, H. Welling, L. Wen, S. Wen, J. T. Whelan, S. E. Whitcomb, B. F. Whiting, P. A. Willems, P. R. Williams, R. Williams, B. Willke, A. Wilson, B. J. Winjum, W. Winkler, S. Wise, A. G. Wiseman, G. Woan, R. Wooley, J. Worden, I. Yakushin, H. Yamamoto, S. Yoshida, I. Zawischa, L. Zhang, N. Zotov, M. E. Zucker, J. Zweizig

Bibliographic record

VenuePhysical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2004
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersAustralian Research CouncilNatural Sciences and Engineering Research Council of CanadaCouncil of Scientific and Industrial Research, IndiaAlfred P. Sloan FoundationNational Science FoundationJohn Simon Guggenheim Memorial FoundationDavid and Lucile Packard Foundation
KeywordsLIGOPhysicsMilky WayGravitational waveAstronomical interferometerAstrophysicsAstronomyGalaxyNeutron starBinary numberInterferometryBinary starGlobular clusterGravitational-wave observatoryStars

Abstract

fetched live from OpenAlex

We report on a search for gravitational waves from coalescing compact binary systems in the Milky Way and the Magellanic Clouds. The analysis uses data taken by two of the three LIGO interferometers during the first LIGO science run and illustrates a method of setting upper limits on inspiral event rates using interferometer data. The analysis pipeline is described with particular attention to data selection and coincidence between the two interferometers. We establish an observational upper limit of $\mathcal{R}<1.7\ifmmode\times\else\texttimes\fi{}{10}^{2}$ per year per Milky Way Equivalent Galaxy (MWEG), with 90% confidence, on the coalescence rate of binary systems in which each component has a mass in the range $1--3{M}_{\ensuremath{\bigodot}}.$

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)0.002
metaresearch head score (Gemma)0.009
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 score0.007
Threshold uncertainty score0.012

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.009
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0070.006
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.031
GPT teacher head0.374
Teacher spread0.343 · 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

Citations198
Published2004
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 topicPulsars and Gravitational Waves ResearchFrench-language works237,207