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Record W3022884152 · doi:10.48550/arxiv.1604.00439

The Sensitivity of the Advanced LIGO Detectors at the Beginning of Gravitational Wave Astronomy

2016· article· en· W3022884152 on OpenAlexfundno aff
Д. В. Мартынов, E. D. Hall, B. P. Abbott, R. Abbott, T. D. Abbott, C. Adams, R. X. Adhikari, R. A. Anderson, S. B. Anderson, K. Arai, M. A. Arain, S. M. Aston, Larry Austin, S. Ballmer, M. Barbet, D. Barker, B. Barr, J. Bartlett, M. A. Barton, I. Bartos, J. C. Batch, A. S. Bell, Ilya Belopolski, J. Bergman, J. Betzwieser, G. Billingsley, J. Birch, C. Biwer, E. Black, C. D. Blair, C. Bogan, R. Bork, D. O. Bridges, A. F. Brooks, C. Celerier, G. Ciani, F. Clara, D. Cook, S. T. Countryman, M. J. Cowart, D. C. Coyne, A. Cumming, L. Cunningham, M. Damjanic, R. Dannenberg, K. Danzmann, E. J. Daw, D. DeBra, R. T. DeRosa, R. DeSalvo, K. L. Dooley, S. Doravari, J. C. Driggers, S. E. Dwyer, A. Effler, T. Etzel, T. M. Evans, M. Factourovich, H. Fair, D. Feldbaum, R. P. Fisher, M. Frede, V. V. Frolov, P. Fulda, M. Fyffe, Vincenzo Galdi, J. A. Giaime, K. D. Giardina, Joseph Gleason, R. Goetz, C. Gray, R. J. S. Greenhalgh, H. Grote, C. Guido, K. E. Gushwa, E. K. Gustafson, R. Gustafson, G. Hammond, J. Hanks, J. Hanson, T. Hardwick, I. W. Harry, J. Heefner, M. C. Heintze, A. W. Heptonstall, D. Hoak, J. Hough, A. Ivanov, K. Izumi, M. Jacobson, E. James, R. W. L. Jones, S. Kandhasamy, S. Karki, M. Kasprzack, S. Kaufer, K. Kawabe, W. Kells, N. Kijbunchoo, E. J. King, Peter King, D. L. Kinzel, J. S. Kissel, K. Kokeyama, W. Z. Korth, A. Królak, M. Landry, B. Lantz, B. M. Levine, J. B. Lewis, N. A. Lockerbie, M. Lormand, M. Lubinski, A. P. Lundgren, T. MacDonald, D. M. Macleod, M. Mageswaran, K. Mailand, A. S. Markosyan, E. Maros, I. W. Martin, R. M. Martin, J. N. Marx, T. J. Massinger, R. McCarthy, D. E. McClelland, S. McCormick, G. McIntyre, J. McIver, E. L. Merilh, M. S. Meyer, P. M. Meyers, G. Moreno, C. Mueller, G. Mueller, A. Mullavey, J. Münch, L. K. Nuttall, J. Oberling, P. Oppermann, Richard J. Oram, C. Osthelder, D. J. Ottaway, H. Overmier, J. R. Palamos, H. R. Paris, W. Parker, Z. Patrick, A. Pele, S. Penn, M. Phelps, M. Pickenpack, I. M. Pinto, J. Poeld, M. Principe, L. Prokhorov, O. Puncken, V. Quetschke, E. A. Quintero, F. J. Raab, H. Radkins, P. Raffai, C. Ramet, C. M. Reed, S. Reid, D. H. Reitze, N. A. Robertson, J. G. Rollins, V. J. Roma, J. H. Romie, S. Rowan, K. Ryan, T. Sadecki, E. J. Sanchez, V. Sandberg, V. Sannibale, R. L. Savage, R. M. S. Schofield, Brad Schultz, P. Schwinberg, James A. Sellers, A. Sêvigny, D. A. Shaddock, Z. Shao, B. Shapiro, P. Shawhan, D. Sigg, B. J. J. Slagmolen, J. R. Smith, M. Smith, N. D. Smith-Lefebvre, B. Sorazu, A. Staley, A. Stochino, K. A. Strain, Richard W. Taylor, M. Thomas, P. Thomas, K. A. Thorne, E. Thrane, C. I. Torrie, G. Traylor, G. Vajente, G. Valdés, A. A. van Veggel, M. Vargas, A. Vecchio, P. J. Veitch, K. Venkateswara, T. Vo, C. Vorvick, M. Walker, R. L. Ward, J. Warner, B. Weaver, T. Welborn, C. Wilkinson, P. A. Willems, L. Williams, B. Willke, L. Winkelmann, C. C. Wipf, J. Worden, Guanglei Wu, H. Yamamoto, C. C. Yancey, L. Zhang, J. Zweizig

Bibliographic record

VenueWhite Rose Research Online (University of Leeds, The University of Sheffield, University of York) · 2016
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersDivision of Human Resource DevelopmentIstituto Nazionale di Fisica NucleareMinistero dello Sviluppo EconomicoMinistry of Education, IndiaNational Research Foundation of KoreaMinisterio de Economía y CompetitividadCouncil of Scientific and Industrial Research, IndiaNederlandse Organisatie voor Wetenschappelijk OnderzoekCentre National de la Recherche ScientifiqueIndustry CanadaScience and Technology Facilities CouncilNational Research FoundationGovern de les Illes BalearsEuropean CommissionScience and Engineering Research BoardInstitut des Origines de LyonScottish Universities Physics AllianceRussian Foundation for Basic ResearchScottish Funding CouncilHungarian Scientific Research FundLeverhulme TrustNational Science Foundation
KeywordsLIGOPhysicsAstronomyGravitational waveGravitational-wave astronomySensitivity (control systems)DetectorGravitational-wave observatoryAstrophysicsEinstein TelescopeOptics

Abstract

fetched live from OpenAlex

The Laser Interferometer Gravitational Wave Observatory (LIGO) consists of two widely separated 4 km laser interferometers designed to detect gravitational waves from distant astrophysical sources in the frequency range from 10 Hz to 10 kHz. The first observation run of the Advanced LIGO detectors started in September 2015 and ended in January 2016. A strain sensitivity of better than $10^{-23}/\sqrt{\text{Hz}}$ was achieved around 100 Hz. Understanding both the fundamental and the technical noise sources was critical for increasing the observable volume in the universe. The average distance at which coalescing binary black hole systems with individual masses of 30 $M_\odot$ could be detected was 1.3 Gpc. Similarly, the range for binary neutron star inspirals was about 75 Mpc. With respect to the initial detectors, the observable volume of Universe increased respectively by a factor 69 and 43. These improvements allowed Advanced LIGO to detect the gravitational wave signal from the binary black hole coalescence, known as GW150914.

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)0.004
metaresearch head score (Gemma)0.007
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0040.007
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.001
Science and technology studies0.0010.001
Scholarly communication0.0020.002
Open science0.0010.002
Research integrity0.0020.002
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 head0.021
GPT teacher head0.266
Teacher spread0.245 · 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 designBench or experimental
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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Citations0
Published2016
Admission routes1
Has abstractyes

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