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Record W2139035778 · doi:10.1103/physrevd.76.022001

First cross-correlation analysis of interferometric and resonant-bar gravitational-wave data for stochastic backgrounds

2007· article· en· W2139035778 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, 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, M. Burgamy, 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, A. Taracchini, 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. C. 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. 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, 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, W. O. Hamilton, 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, 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, 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, B. J. McCaulley, 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, Phillip Miller, S. Mitra, V. P. Mitrofanov, G. Mitselmakher, R. Mittleman, O. Miyakawa, Soumya D. Mohanty, V. Moody, 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, D. Nettles, G. Newton, A. Nishizawa, Kenji Numata, B. O’Reilly, R. O’Shaughnessy, D. J. Ottaway, H. Overmier, B. J. Owen, Ho Jung Paik, Y. Pan, M. A. Papa, V. Parameshwaraiah, P. Patel, M. Pedraza, 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, 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, D. M. Strom, A. L. Stuver, T. Z. Summerscales, Ke-Xun 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, K. V. Tokmakov, C. Torres, G. Traylor, Miquel Trias, W. Tyler, D. Ugolini, C. Ungarelli, Karel Urbánek, H. Vahlbruch, M. Vallisneri, M. Varvella, S. Vass, A. Vecchio, J. Veitch, A. Villar, C. Vorvick, S. P. Vyachanin, S. J. Waldman, L. Wallace, R. L. Ward, K. Watts, Jordan S. Weaver, D. Webber, Albin Weber, A. 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, 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, Wenhao Wu, I. Yakushin, H. Yamamoto, Z. Yan, S. Yoshida, Nicolás Yunes, M. Zanolin, J. Zhang, L. Zhang, P. 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 · 2007
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaLeverhulme TrustAlexander von Humboldt-StiftungCouncil of Scientific and Industrial Research, IndiaAlfred P. Sloan FoundationNational Science FoundationJohn Simon Guggenheim Memorial FoundationNational Aeronautics and Space Administration
KeywordsLIGOGravitational wavePhysicsInterferometryOmegaSensitivity (control systems)Bar (unit)Sign (mathematics)Limit (mathematics)Range (aeronautics)Confidence intervalDetectorComputational physicsOpticsStatisticsAstrophysicsMathematical analysisQuantum mechanicsMathematicsElectronic engineering

Abstract

fetched live from OpenAlex

Data from the LIGO Livingston interferometer and the ALLEGRO resonant-bar detector, taken during LIGO's fourth science run, were examined for cross correlations indicative of a stochastic gravitational-wave background in the frequency range 850--950 Hz, with most of the sensitivity arising between 905 and 925 Hz. ALLEGRO was operated in three different orientations during the experiment to modulate the relative sign of gravitational-wave and environmental correlations. No statistically significant correlations were seen in any of the orientations, and the results were used to set a Bayesian 90% confidence level upper limit of ${\ensuremath{\Omega}}_{\mathrm{gw}}(f)\ensuremath{\le}1.02$, which corresponds to a gravitational-wave strain at 915 Hz of $1.5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}23}\text{ }\text{ }{\mathrm{Hz}}^{\ensuremath{-}1/2}$. In the traditional units of ${h}_{100}^{2}{\ensuremath{\Omega}}_{\mathrm{gw}}(f)$, this is a limit of 0.53, 2 orders of magnitude better than the previous direct limit at these frequencies. The method was also validated with successful extraction of simulated signals injected in hardware and software.

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)0.004
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.011

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.004
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.002
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0020.001

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 head0.041
GPT teacher head0.392
Teacher spread0.350 · 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 designSimulation or modeling
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".

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Citations52
Published2007
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