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Joint LIGO and TAMA300 search for gravitational waves from inspiralling neutron star binaries
B. Abbott, R. Abbott, R. X. Adhikari, A. Ageev, J. Agresti, P. Ajith, B. Allen, J. Allen, R. Amin, S. B. Anderson, W. G. Anderson, M. C. Araya, H. Armandula, M. C. B. Ashley, F. Asiri, P. Aufmuth, C. Aulbert, Рамачандран Баласубраманиан, S. Ballmer, B. C. Barish, C. Barker, D. Barker, 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, Lindy Blackburn, B. Bland, B. Bochner, L. Bogue, R. Bork, S. Bose, P. R. Brady, V. B. Braginsky, J. E. Brau, D. Brown, A. Bullington, A. Bunkowski, A. Buonanno, R. Burgess, D. Busby, William E. Butler, Robert L. Byer, L. Cadonati, G. Cagnoli, J. B. Camp, J. K. Cannizzo, K. C. Cannon, C. A. Cantley, Jianshu Cao, L. Cardenas, K. Carter, M. M. Casey, J. Castiglione, A. Chandler, J. Chapsky, P. Charlton, S. Chatterji, S. Chelkowski, Y. Chen, V. Chickarmane, A. Taracchini, N. Christensen, D. Churches, Thomas Cokelaer, C. N. Colacino, R. L. Coldwell, M. Coles, D. Cook, T. R. Corbitt, D. C. Coyne, J. D. E. Creighton, D. R. M. Crooks, P. Csatorday, B. J. Cusack, Curt Cutler, James Dalrymple, E. D’Ambrosio, K. Danzmann, G. S. Davies, E. J. Daw, D. DeBra, T. Delker, V. Dergachev, S. Desai, R. DeSalvo, S. Dhurandhar, A. Di Credico, M. C. Díaz, H. Ding, R. W. P. Drever, R. J. Dupuis, Jeffrey A. Edlund, P. Ehrens, E. J. Elliffe, T. Etzel, M. Evans, T. M. Evans, S. Fairhurst, Carsten Fallnich, D. Farnham, M. M. Fejer, T. Findley, M. Fine, L. S. Finn, K. Y. Franzen, A. Freise, R. Frey, P. Fritschel, V. V. Frolov, M. Fyffe, K. S. Ganezer, J. A. Garofoli, J. A. Giaime, A. Gillespie, Keisuke Goda, L. M. Goggin, G. González, S. Goßler, P. 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, C. Hanna, J. Hanson, C. Hardham, J. Harms, I. W. Harry, A. Hartunian, J. Heefner, Y. Hefetz, Gerhard Heinzel, I. S. Heng, M. Hennessy, N. Hepler, A. Heptonstall, M. Heurs, M. Hewitson, S. Hild, Neil Hindman, P. Hoang, J. Hough, M. Hrynevych, W. Hua, Masahiro Ito, Y. Itoh, A. Ivanov, O. Jennrich, Ben A. Johnson, W. W. Johnson, W. R. Johnston, D. I. Jones, Gareth Jones, Lynne Jones, Dieter Jungwirth, V. Kalogera, E. Katsavounidis, K. Kawabe, W. Kells, Jonathan Kern, A. Khan, S. Killbourn, C. J. Killow, C. Kim, C. King, P. J. King, S. Klimenko, S. Koranda, K. Kötter, J. Kovalik, D. B. Kozak, B. Krishnan, M. Landry, John Langdale, B. Lantz, R. Lawrence, A. Lazzarini, Mingxing Lei, I. Leonor, Kenneth G. Libbrecht, A. Libson, P. E. Lindquist, S. Liu, J. Logan, M. Lormand, M. Lubinski, H. Lück, M. Luna, T. T. Lyons, B. Machenschalk, M. MacInnis, M. Mageswaran, K. Mailand, Walid A. Majid, M. Malec, V. Mandic, F.M. Mann, A. Marin, S. Márka, E. Maros, James Mason, K. Mason, O. Matherny, L. Matone, N. Mavalvala, R. McCarthy, D. E. McClelland, M. McHugh, J. W. C. McNabb, A. C. Melissinos, G. Mendell, R. A. Mercer, S. Meshkov, Eirini Messaritaki, C. Messenger, Е. Е. Михайлов, S. Mitra, V. P. Mitrofanov, G. Mitselmakher, R. Mittleman, O. Miyakawa, Soumya D. Mohanty, G. Moreno, K. Mossavi, G. Mueller, S. Mukherjee, P. G. Murray, E. Myers, J. Myers, S. Nagano, T. Nash, R. K. Nayak, G. Newton, F. Nocera, J. S. Noel, P. Nutzman, T. Olson, B. O’Reilly, D. J. Ottaway, Adrian C. Ottewill, D. Ouimette, H. Overmier, B. J. Owen, Y. Pan, M. A. Papa, V. Parameshwaraiah, C. Parameswariah, M. Pedraza, S. Penn, M. Pitkin, M. V. Plissi, R. Prix, V. Quetschke, F. J. Raab, H. Radkins, R. Rahkola, M. Rakhmanov, Shanti Rao, K. Rawlins, S. Ray‐Majumder, V. Re, D. Redding, M. W. Regehr, T. Regimbau, S. Reid, K. T. Reilly, K. Reithmaier, D. H. Reitze, S. Richman, R. Riesen, K. Riles, B. Rivera, Anthony Rizzi, D. I. Robertson, N. A. Robertson, C. Robinson, L. Robison, S. Roddy, A. Rodriguez, J. G. Rollins, J. D. Romano, Haisheng Rong, D. Rose, E. Rotthoff, S. Rowan, A. Rüdiger, Laurent Ruet, Pamela J. Russell, K. Ryan, I. Salzman, V. Sandberg, G. H. Sanders, V. Sannibale, P. Sarin, B. S. Sathyaprakash, P. R. Saulson, R. L. Savage, A. Sazonov, R. Schilling, Kevin C. Schlaufman, V. Schmidt, R. Schnabel, R. M. S. Schofield, B. F. Schutz, P. Schwinberg, S. M. Scott, Shawn Seader, A. C. Searle, B. Sears, S. Seel, Frank Seifert, D. Sellers, A. S. Sengupta, Charles Shapiro, P. Shawhan, D. H. Shoemaker, Q. Z. Shu, A. Sibley, X. Siemens, L. Sievers, D. Sigg, A. M. Sintes, J. R. Smith, M. Smith, P. Sneddon, Robert Spero, O. Spjeld, G. Stapfer, D. Steussy, K. A. Strain, D. Strom, A. L. Stuver, T. Z. Summerscales, M. C. Sumner, M. Sung, P. J. Sutton, Julien Sylvestre, D. B. Tanner, H. Tariq, M. Tarallo, Ian Taylor, R. Taylor, K. A. Thorne, K. S. Thorne, M. Tibbits, S. Tilav, Massimo Tinto, K. V. Tokmakov, C. Torres, C. Torrie, G. Traylor, W. Tyler, D. Ugolini, C. Ungarelli, M. Vallisneri, M. van Putten, S. Vass, A. Vecchio, J. Veitch, C. Vorvick, S. P. Vyachanin, L. Wallace, H. Walther, R. L. Ward, B. Ware, K. Watts, D. Webber, A. Weidner, U. Weiland, A. J. Weinstein, R. Weiss, H. Welling, L. Wen, S. Wen, K. Wette, J. T. Whelan, S. E. Whitcomb, B. F. Whiting, S. Wiley, C. Wilkinson, P. A. Willems, P. R. Williams, R. Williams, B. Willke, G. Wilson, B. J. Winjum, W. Winkler, S. Wise, A. G. Wiseman, G. Woan, D. Woods, R. Wooley, J. Worden, W. L. K. Wu, I. Yakushin, H. Yamamoto, S. Yoshida, K. D. Zaleski, M. Zanolin, I. Zawischa, L. Zhang, R. Zhu, N. Zotov, M. E. Zucker, J. Zweizig, Masaki Ando, K. Arai, A Araya, Hideki Asada, Y. Aso, P. T. Beyersdorf, Youhei Fujiki, Masa‐Katsu Fujimoto, R. Fujita, Mitsuhiro Fukushima, Toshifumi Futamase, Y. Hamuro, T. Haruyama, K. Hayama, Hideo Iguchi, Yukiyoshi Iida, Kunihito Ioka, Hideki Ishitsuka, N. Kamikubota, N. Kanda, T. Kaneyama, Y. Karasawa, K. Kasahara, T. Kasai, Mayu Katsuki, S. Kawamura, F. Kawazoe, Y. Kojima, K. Kokeyama, Kazuhiro Kondo, Yoshihide Kozai, Hideaki Kudoh, K. Kuroda, T. Kuwabara, Namio Matsuda, N. Mio, Kazuyuki Miura, Shoken M. Miyama, S. Miyoki, H. Mizusawa, Shigenori Moriwaki, M. Musha, Y. Nagayama, K. Nakagawa, T. Nakamura, Hiroyuki Nakano, Ken-ichi Nakao, Yuhiko Nishi, Kenji Numata, Y. Ogawa, N. Ohishi, Akira Okutomi, K. Oohara, S. Otsuka, Y. Saito, S. Sakata, Misao Sasaki, N. Sato, S. Sato, Yoshihiro Sato, K. Sato, A. Sekido, N. Seto, M. Shibata, H. Shinkai, T. Shintomi, K. Soida, K. Somiya, T. Suzuki, Hideyuki Tagoshi, H. Takahashi, R. Takahashi, A. Takamori, Shuzo Takemoto, Keiji Takeno, Takahiro Tanaka, K. Taniguchi, T. Tanji, Daisuke Tatsumi, S. Telada, Masao Tokunari, T. Tomaru, K. Tsubono, Nobuhiro TSUDA, Y. Tsunesada, Takashi Uchiyama, K-i Ueda, A. Ueda, K. Waseda, A. Yamamoto, Kazuhiro Yamamoto, Takashi Yamazaki, Yuriko Yanagi, J Yokoyama, T. Yoshida, Z.-H. Zhu
Bibliographic record
VenuePhysical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2006
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersAustralian Research CouncilNatural Sciences and Engineering Research Council of CanadaJapan Society for the Promotion of ScienceMinistry of Education, Culture, Sports, Science and TechnologyDavid and Lucile Packard FoundationLeverhulme TrustCouncil of Scientific and Industrial Research, IndiaAlfred P. Sloan FoundationJohn Simon Guggenheim Memorial FoundationNational Science Foundation
KeywordsLIGOGravitational waveNeutron starPhysicsAstronomyAstrophysicsMilky WayGravitational-wave observatoryGalaxyBinary numberBinary starStars
Abstract
We search for coincident gravitational wave signals from inspiralling neutron star binaries using LIGO and TAMA300 data taken during early 2003. Using a simple trigger exchange method, we perform an intercollaboration coincidence search during times when TAMA300 and only one of the LIGO sites were operational. We find no evidence of any gravitational wave signals. We place an observational upper limit on the rate of binary neutron star coalescence with component masses between 1 and $3{M}_{\ensuremath{\bigodot}}$ of 49 per year per Milky Way equivalent galaxy at a 90% confidence level. The methods developed during this search will find application in future network inspiral analyses.
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 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)0.001
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 score0.003
Threshold uncertainty score0.006
Distilled classifier scores by category (both heads)
| Category | Codex | Gemma |
|---|---|---|
| Metaresearch | 0.001 | 0.002 |
| Meta-epidemiology (narrow) | 0.000 | 0.000 |
| Meta-epidemiology (broad) | 0.001 | 0.000 |
| Bibliometrics | 0.002 | 0.002 |
| Science and technology studies | 0.001 | 0.000 |
| Scholarly communication | 0.001 | 0.000 |
| Open science | 0.000 | 0.001 |
| Research integrity | 0.001 | 0.000 |
| Insufficient payload (model declined to judge) | 0.001 | 0.001 |
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 head0.027
GPT teacher head0.351
Teacher spread0.323 · 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
Citations50
Published2006
Admission routes1
Has abstractyes