Effects of waveform model systematics on the interpretation of GW150914

Bibliographic Details
Main Author: Abbott, B. P.
Publication Date: 2017
Other Authors: Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, B., Allocca, A., Altin, P. A., Ananyeva, A., Anderson, S. B., Anderson, W. G., Appert, S., Arai, K., Araya, M. C., Areeda, J. S., Arnaud, N., Arun, K. G., Ascenzi, S., Ashton, G., Ast, M., Aston, S. M., Astone, P., Aufmuth, P., Aulbert, C., Avila-Alvarez, A., Babak, S., Bacon, P., Bader, M. K. M., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Barayoga, J. C., Barclay, S. E., Barish, B. C., Barker, D., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. C., Baune, C., Bavigadda, V., Bazzan, M., Beer, C., Bejger, M., Belahcene, I., Belgin, M., Bell, A. S., Berger, B. K., Bergmann, G., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhagwat, S., Bhandare, R., Bilenko, I. A., Billingsley, G., Billman, C. R., Birch, J., Birney, R., Birnholtz, O., Biscans, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M. A., Blackburn, J. K., Blackman, J., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bock, O., Boer, M., Bogaert, G., Bohe, A., Bondu, F., Bonnand, R., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Braginsky, V. B., Branchesi, M., Brau, J. E., Briant, T., Brillet, A., Brinkmann, M., Brisson, V., Brockill, P., Broida, J. E., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Brunett, S., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Bustillo, J. Caldern, Callister, T. A., Calloni, E., Camp, J. B., Cannon, K. C., Cao, H., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Diaz, J. Casanueva, Casentini, C., Caudill, S., Cavaglia, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Baiardi, L. Cerboni, Cerretani, G., Cesarini, E., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande-Mottin, E., Cheeseboro, B. D., Chen, H. Y., Chen, Y., Cheng, H-P, Chincarini, A., Chiummo, A., Chmiel, T., Cho, H. S., Cho, M., Chow, J. H., Christensen, N., Chu, Q., Chua, A. J. K., Chua, S., Chung, S., Ciani, G., Clara, F., Clark, J. A., Cleva, F., Cocchieri, C., Coccia, E., Cohadon, P-F, Colla, A., Collette, C. G., Cominsky, L., Constancio, M., Conti, L., Cooper, S. J., Corbitt, T. R., Cornish, N., Corsi, A., Cortese, S., Costa, C. A., Coughlin, M. W., Coughlin, S. B., Coulon, J-P, Countryman, S. T., Couvares, P., Covas, P. B., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Creighton, J. D. E., Creighton, T. D., Cripe, J., Crowder, S. G., Cullen, T. J., Cumming, A., Cunningham, L., Cuoco, E., Dal Canton, T., Danilishin, S. L., D'Antonio, S., Danzmann, K., Dasgupta, A., Costa, C. F. Da Silva, Dattilo, V., Dave, I., Davier, M., Davies, G. S., Davis, D., Daw, E. J., Day, B., Day, R., De, S., Debra, D., Debreczeni, G., Degallaix, J., De laurentis, M., Deleglise, S., Del Pozzo, W., Denker, T., Dent, T., Dergachev, V., De Rosa, R., DeRosa, R. T., DeSalvo, R., Devenson, J., Devine, R. C., Dhurandhar, S., Diaz, M. C., Di Fiore, L., Di Giovanni, M., Di Girolamo, T., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Doctor, Z., Dolique, V., Donovan, F., Dooley, K. L., Doravari, S., Dorrington, I., Douglas, R., Alvarez, M. Dovale, Downes, T. P., Drago, M., Drever, R. W. P., Driggers, J. C., Du, Z., Ducrot, M., Dwyer, S. E., Edo, T. B., Edwards, M. C., Effler, A., Eggenstein, H-B, Ehrens, P., Eichholz, J., Eikenberry, S. S., Eisenstein, R. A., Essick, R. C., Etienne, Z., Etzel, T., Evans, M., Evans, T. M., Everett, R., Factourovich, M., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Farinon, S., Farr, B., Farr, W. M., Fauchon-Jones, E. J., Favata, M., Fays, M., Fehrmann, H., Fejer, M. M., Galiana, A. Fernandez, Ferrante, I., Ferreira, E. C., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. P., Flaminio, R., Fletcher, M., Fong, H., Forsyth, S. S., Fournier, J-D, Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fries, E. M., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H., Gadre, B. U., Gaebel, S. M., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, F., Gaur, G., Gayathri, V., Gehrels, N., Gemme, G., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghonge, S., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giaime, J. A., Giardina, K. D., Giazotto, A., Gill, K., Glaefke, A., Goetz, E., Goetz, R., Gondan, L., Gonzalez, G., Castro, J. M. Gonzalez, Gopakumar, A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., Grado, A., Graef, C., Granata, M., Grant, A., Gras, S., Gray, C., Greco, G., Green, A. C., Groot, P., Grote, H., Grunewald, S., Guidi, G. M., Guo, X., Gupta, A., Gupta, M. K., Gushwa, K. E., Gustafson, E. K., Gustafson, R., Hacker, J. J., Hall, B. R., Hall, E. D., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hannam, M. D., Hanson, J., Hardwick, T., Harms, J., Harry, G. M., Harry, I. W., Hart, M. J., Hartman, M. T., Haster, C-J, Haughian, K., Healy, J., Heidmann, A., Heintze, M. C., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Heng, I. S., Hennig, J., Henry, J., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Hofman, D., Holt, K., Holz, D. E., Hopkins, P., Hough, J., Houston, E. A., Howell, E. J., Hu, Y. M., Huerta, E. A., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Huynh-Dinh, T., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isac, J-M, Isi, M., Isogai, T., Iyer, B. R., Izumi, K., Jacqmin, T., Jani, K., Jaranowski, P., Jawahar, S., Jimenez-Forteza, F., Johnson, W. W., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., Junker, J., Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Karki, S., Karvinen, K. S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., Kefelian, F., Keitel, D., Kelley, D. B., Kennedy, R., Key, J. S., Khalili, F. Y., Khan, I., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, Chunglee, Kim, J. C., Kim, Whansun, Kim, W., Kim, Y-M, Kimbrell, S. J., King, E. J., King, P. J., Kirchhoff, R., Kissel, J. S., Klein, B., Kleybolte, L., Klimenko, S., Koch, P., Koehlenbeck, S. M., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Kraemer, C., Kringel, V., Krishnan, B., Krolak, A., Kuehn, G., Kumar, P., Kumar, R., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lang, R. N., Lange, J., Lantz, B., Lanza, R. 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J., Yu, Hang, Yu, Haocun, Yvert, M., Zadrozny, A., Zangrando, L., Zanolin, M., Zendri, J-P, Zevin, M., Zhang, L., Zhang, M., Zhang, T., Zhang, Y., Zhao, C., Zhou, M., Zhou, Z., Zhu, S. J., Zhu, X. J., Zucker, M. E., Zweizig, J., Boyle, M., Chu, T., Hemberger, D., Hinder, I., Kidder, L. E., Ossokine, S., Scheel, M., Szilagyi, B., Teukolsky, S., Vinuales, A. Vano, LIGO Sci Collaboration, Virgo Collaboration
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Download full: http://dx.doi.org/10.1088/1361-6382/aa6854
http://hdl.handle.net/11449/162706
Summary: Parameter estimates of GW150914 were obtained using Bayesian inference, based on three semi-analytic waveform models for binary black hole coalescences. These waveform models differ from each other in their treatment of black hole spins, and all three models make some simplifying assumptions, notably to neglect sub-dominant waveform harmonic modes and orbital eccentricity. Furthermore, while the models are calibrated to agree with waveforms obtained by full numerical solutions of Einstein's equations, any such calibration is accurate only to some non-zero tolerance and is limited by the accuracy of the underlying phenomenology, availability, quality, and parameter-space coverage of numerical simulations. This paper complements the original analyses of GW150914 with an investigation of the effects of possible systematic errors in the waveform models on estimates of its source parameters. To test for systematic errors we repeat the original Bayesian analysis on mock signals from numerical simulations of a series of binary configurations with parameters similar to those found for GW150914. Overall, we find no evidence for a systematic bias relative to the statistical error of the original parameter recovery of GW150914 due to modeling approximations or modeling inaccuracies. However, parameter biases are found to occur for some configurations disfavored by the data of GW150914: for binaries inclined edge-on to the detector over a small range of choices of polarization angles, and also for eccentricities greater than similar to 0.05. For signals with higher signal-to-noise ratio than GW150914, or in other regions of the binary parameter space (lower masses, larger mass ratios, or higher spins), we expect that systematic errors in current waveform models may impact gravitational-wave measurements, making more accurate models desirable for future observations.
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spelling Effects of waveform model systematics on the interpretation of GW150914gravitational wavesnumerical relativityparameter estimationwaveform modelssystematic errorsGW150914Parameter estimates of GW150914 were obtained using Bayesian inference, based on three semi-analytic waveform models for binary black hole coalescences. These waveform models differ from each other in their treatment of black hole spins, and all three models make some simplifying assumptions, notably to neglect sub-dominant waveform harmonic modes and orbital eccentricity. Furthermore, while the models are calibrated to agree with waveforms obtained by full numerical solutions of Einstein's equations, any such calibration is accurate only to some non-zero tolerance and is limited by the accuracy of the underlying phenomenology, availability, quality, and parameter-space coverage of numerical simulations. This paper complements the original analyses of GW150914 with an investigation of the effects of possible systematic errors in the waveform models on estimates of its source parameters. To test for systematic errors we repeat the original Bayesian analysis on mock signals from numerical simulations of a series of binary configurations with parameters similar to those found for GW150914. Overall, we find no evidence for a systematic bias relative to the statistical error of the original parameter recovery of GW150914 due to modeling approximations or modeling inaccuracies. However, parameter biases are found to occur for some configurations disfavored by the data of GW150914: for binaries inclined edge-on to the detector over a small range of choices of polarization angles, and also for eccentricities greater than similar to 0.05. For signals with higher signal-to-noise ratio than GW150914, or in other regions of the binary parameter space (lower masses, larger mass ratios, or higher spins), we expect that systematic errors in current waveform models may impact gravitational-wave measurements, making more accurate models desirable for future observations.Netherlands Organisation for Scientific ResearchCouncil of Scientific and Industrial Research of IndiaDepartment of Science and Technology, IndiaScience & Engineering Research Board (SERB), IndiaMinistry of Human Resource Development, IndiaSpanish Ministerio de Economia y CompetitividadConselleria d'Economia i Competitivitat of the Govern de les Illes BalearsConselleria d'Educacio, Cultura i Universitats of the Govern de les Illes BalearsNational Science Centre of PolandEuropean CommissionRoyal SocietyScottish Funding CouncilScottish Universities Physics AllianceHungarian Scientific Research Fund (OTKA)Lyon Institute of Origins (LIO)National Research Foundation of KoreaIndustry CanadaProvince of Ontario through the Ministry of Economic Development and InnovationNatural Science and Engineering Research Council CanadaCanadian Institute for Advanced ResearchBrazilian Ministry of Science, Technology, and InnovationFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Russian Foundation for Basic ResearchLeverhulme TrustResearch CorporationMinistry of Science and Technology (MOST), TaiwanKavli FoundationResearch Corporation for Science AdvancementSherman Fairchild FoundationCALTECH, LIGO, Pasadena, CA 91125 USALouisiana State Univ, Baton Rouge, LA 70803 USAAmer Univ, Washington, DC 20016 USAUniv Salerno, Fisciano, I-84084 Salerno, ItalyIst Nazl Fis Nucl, Sez Napoli, Complesso Univ Monte S Angelo, I-80126 Naples, ItalyUniv Florida, Gainesville, FL 32611 USALIGO Livingston Observ, Livingston, LA 70754 USAUniv Savoie Mt Blanc, CNRS IN2P3, Lab Annecy le Vieux Phys Particules LAPP, F-74941 Annecy Le Vieux, FranceUniv Sannio Benevento, I-82100 Benevento, ItalyMax Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, GermanyNikhef, Sci Pk, NL-1098 XG Amsterdam, NetherlandsMIT, LIGO, 77 Massachusetts Ave, Cambridge, MA 02139 USAInst Nacl Pesquisas Espaciais, BR-12227010 Sao Jose Dos Campos, SP, BrazilIst Nazl Fis Nucl, Gran Sasso Sci Inst, I-67100 Laquila, ItalyIst Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, ItalyInteruniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, IndiaTata Inst Fundamental Res, Int Ctr Theoret Sci, Bengaluru 560089, IndiaUniv Wisconsin Milwaukee, Milwaukee, WI 53201 USALeibniz Univ Hannover, D-30167 Hannover, GermanyUniv Pisa, I-56127 Pisa, ItalyIst Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, ItalyAustralian Natl Univ, Canberra, ACT 0200, AustraliaCalif State Univ Fullerton, Fullerton, CA 92831 USAUniv Paris Saclay, CNRS IN2P3, Univ Paris Sud, LAL, F-91898 Orsay, FranceChennai Math Inst, Chennai 603103, Tamil Nadu, IndiaUniv Roma Tor Vergata, I-00133 Rome, ItalyUniv Hamburg, D-22761 Hamburg, GermanyIst Nazl Fis Nucl, Sez Roma, I-00185 Rome, ItalyMax Planck Gravitat Phys, Albert Einstein Inst, D-14476 Potsdam, GermanyUniv Paris Diderot, APC, CNRS IN2P3, CEA Irfu,Observ Paris,Sorbonne Paris Cite, F-75205 Paris 13, FranceWest Virginia Univ, Morgantown, WV 26506 USAUniv Perugia, I-06123 Perugia, ItalyIst Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, ItalyEGO, I-56021 Pisa, ItalySyracuse Univ, Syracuse, NY 13244 USAUniv Glasgow, SUPA, Glasgow G12 8QQ, Lanark, ScotlandLIGO Hanford Observ, Richland, WA 99352 USARMKI, Wigner RCP, Konkoly Thege Miklos Ut 29-33, H-1121 Budapest, HungaryColumbia Univ, New York, NY 10027 USAStanford Univ, Stanford, CA 94305 USAUniv Padua, Dipartimento Fis & Astron, I-35131 Padua, ItalyIst Nazl Fis Nucl, Sez Padova, I-35131 Padua, ItalyPolish Acad Sci, Nicolaus Copernicus Astron Ctr, PL-00716 Warsaw, PolandGeorgia Inst Technol, Ctr Relativist Astrophys, Atlanta, GA 30332 USAGeorgia Inst Technol, Sch Phys, Atlanta, GA 30332 USAUniv Birmingham, 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M.Siellez, K.Siemens, X.Sieniawska, M.Sigg, D.Silva, A. D.Singer, A.Singer, L. P.Singh, A.Singh, R.Singhal, A.Sintes, A. M.Slagmolen, B. J. J.Smith, B.Smith, J. R.Smith, R. J. E.Son, E. J.Sorazu, B.Sorrentino, F.Souradeep, T.Spencer, A. P.Srivastava, A. K.Staley, A.Steinke, M.Steinlechner, J.Steinlechner, S.Steinmeyer, D.Stephens, B. C.Stevenson, S. P.Stone, R.Strain, K. A.Straniero, N.Stratta, G.Strigin, S. E.Sturani, R. [UNESP]Stuver, A. L.Summerscales, T. Z.Sun, L.Sunil, S.Sutton, P. J.Swinkels, B. L.Szczepanczyk, M. J.Tacca, M.Talukder, D.Tanner, D. B.Tapai, M.Taracchini, A.Taylor, R.Theeg, T.Thomas, E. G.Thomas, M.Thomas, P.Thorne, K. A.Thrane, E.Tippens, T.Tiwari, S.Tiwari, V.Tokmakov, K. V.Toland, K.Tomlinson, C.Tonelli, M.Tornasi, Z.Torrie, C. I.Toyro, D.Travasso, F.Traylor, G.Trifiro, D.Trinastic, J.Tringali, M. C.Trozzo, L.Tse, M.Tso, R.Turconi, M.Tuyenbayev, D.Ugolini, D.Unnikrishnan, C. S.Urban, A. L.Usman, S. A.Vahlbruch, H.Vajente, G.Valdes, G.van Bakel, N.van Beuzekom, M.van den Brand, J. F. J.Van den Broeck, C.Vander-Hyde, D. C.van der Schaaf, L.van Heijningen, J. V.van Veggel, A. A.Vardaro, M.Varma, V.Vass, S.Vasuth, M.Vecchio, A.Vedovato, G.Veitch, J.Veitch, P. J.Venkateswara, K.Venugopalan, G.Verkindt, D.Vetrano, F.Vicere, A.Viets, A. D.Vinciguerra, S.Vine, D. J.Vinet, J-YVitale, S.Vo, T.Vocca, H.Vorvick, C.Voss, D. V.Vousden, W. D.Vyatchanin, S. P.Wade, A. R.Wade, L. E.Wade, M.Walker, M.Wallace, L.Walsh, S.Wang, G.Wang, H.Wang, M.Wang, Y.Ward, R. L.Warner, J.Was, M.Watchi, J.Weaver, B.Wei, L-WWeinert, M.Weinstein, A. J.Weiss, R.Wen, L.Wessels, P.Westphal, T.Wette, K.Whelan, J. T.Whiting, B. F.Whittle, C.Williams, D.Williams, R. D.Williamson, A. R.Willis, J. L.Willke, B.Wimmer, M. H.Winkler, W.Wipf, C. C.Wittel, H.Woan, G.Woehler, J.Worden, J.Wright, J. L.Wu, D. S.Wu, G.Yam, W.Yamamoto, H.Yancey, C. C.Yap, M. J.Yu, HangYu, HaocunYvert, M.Zadrozny, A.Zangrando, L.Zanolin, M.Zendri, J-PZevin, M.Zhang, L.Zhang, M.Zhang, T.Zhang, Y.Zhao, C.Zhou, M.Zhou, Z.Zhu, S. J.Zhu, X. J.Zucker, M. E.Zweizig, J.Boyle, M.Chu, T.Hemberger, D.Hinder, I.Kidder, L. E.Ossokine, S.Scheel, M.Szilagyi, B.Teukolsky, S.Vinuales, A. VanoLIGO Sci CollaborationVirgo Collaboration2018-11-26T17:26:40Z2018-11-26T17:26:40Z2017-05-18info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article48application/pdfhttp://dx.doi.org/10.1088/1361-6382/aa6854Classical And Quantum Gravity. Bristol: Iop Publishing Ltd, v. 34, n. 10, 48 p., 2017.0264-9381http://hdl.handle.net/11449/16270610.1088/1361-6382/aa6854WOS:000399335900001WOS000399335900001.pdf97564145500755650000-0001-9038-2951Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengClassical And Quantum Gravity1,809info:eu-repo/semantics/openAccess2024-11-25T15:03:23Zoai:repositorio.unesp.br:11449/162706Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestrepositoriounesp@unesp.bropendoar:29462024-11-25T15:03:23Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Effects of waveform model systematics on the interpretation of GW150914
title Effects of waveform model systematics on the interpretation of GW150914
spellingShingle Effects of waveform model systematics on the interpretation of GW150914
Abbott, B. P.
gravitational waves
numerical relativity
parameter estimation
waveform models
systematic errors
GW150914
title_short Effects of waveform model systematics on the interpretation of GW150914
title_full Effects of waveform model systematics on the interpretation of GW150914
title_fullStr Effects of waveform model systematics on the interpretation of GW150914
title_full_unstemmed Effects of waveform model systematics on the interpretation of GW150914
title_sort Effects of waveform model systematics on the interpretation of GW150914
author Abbott, B. P.
author_facet Abbott, B. P.
Abbott, R.
Abbott, T. D.
Abernathy, M. R.
Acernese, F.
Ackley, K.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R. X.
Adya, V. B.
Affeldt, C.
Agathos, M.
Agatsuma, K.
Aggarwal, N.
Aguiar, O. D.
Aiello, L.
Ain, A.
Ajith, P.
Allen, B.
Allocca, A.
Altin, P. A.
Ananyeva, A.
Anderson, S. B.
Anderson, W. G.
Appert, S.
Arai, K.
Araya, M. C.
Areeda, J. S.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Aufmuth, P.
Aulbert, C.
Avila-Alvarez, A.
Babak, S.
Bacon, P.
Bader, M. K. M.
Baker, P. T.
Baldaccini, F.
Ballardin, G.
Ballmer, S. W.
Barayoga, J. C.
Barclay, S. E.
Barish, B. C.
Barker, D.
Barone, F.
Barr, B.
Barsotti, L.
Barsuglia, M.
Barta, D.
Bartlett, J.
Bartos, I.
Bassiri, R.
Basti, A.
Batch, J. C.
Baune, C.
Bavigadda, V.
Bazzan, M.
Beer, C.
Bejger, M.
Belahcene, I.
Belgin, M.
Bell, A. S.
Berger, B. K.
Bergmann, G.
Berry, C. P. L.
Bersanetti, D.
Bertolini, A.
Betzwieser, J.
Bhagwat, S.
Bhandare, R.
Bilenko, I. A.
Billingsley, G.
Billman, C. R.
Birch, J.
Birney, R.
Birnholtz, O.
Biscans, S.
Bisht, A.
Bitossi, M.
Biwer, C.
Bizouard, M. A.
Blackburn, J. K.
Blackman, J.
Blair, C. D.
Blair, D. G.
Blair, R. M.
Bloemen, S.
Bock, O.
Boer, M.
Bogaert, G.
Bohe, A.
Bondu, F.
Bonnand, R.
Boom, B. A.
Bork, R.
Boschi, V.
Bose, S.
Bouffanais, Y.
Bozzi, A.
Bradaschia, C.
Brady, P. R.
Braginsky, V. B.
Branchesi, M.
Brau, J. E.
Briant, T.
Brillet, A.
Brinkmann, M.
Brisson, V.
Brockill, P.
Broida, J. E.
Brooks, A. F.
Brown, D. A.
Brown, D. D.
Brown, N. M.
Brunett, S.
Buchanan, C. C.
Buikema, A.
Bulik, T.
Bulten, H. J.
Buonanno, A.
Buskulic, D.
Buy, C.
Byer, R. L.
Cabero, M.
Cadonati, L.
Cagnoli, G.
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Bustillo, J. Caldern
Callister, T. A.
Calloni, E.
Camp, J. B.
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Diaz, J. Casanueva
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Charlton, P.
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Chen, Y.
Cheng, H-P
Chincarini, A.
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Chmiel, T.
Cho, H. S.
Cho, M.
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Christensen, N.
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Countryman, S. T.
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Creighton, J. D. E.
Creighton, T. D.
Cripe, J.
Crowder, S. G.
Cullen, T. J.
Cumming, A.
Cunningham, L.
Cuoco, E.
Dal Canton, T.
Danilishin, S. L.
D'Antonio, S.
Danzmann, K.
Dasgupta, A.
Costa, C. F. Da Silva
Dattilo, V.
Dave, I.
Davier, M.
Davies, G. S.
Davis, D.
Daw, E. J.
Day, B.
Day, R.
De, S.
Debra, D.
Debreczeni, G.
Degallaix, J.
De laurentis, M.
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Del Pozzo, W.
Denker, T.
Dent, T.
Dergachev, V.
De Rosa, R.
DeRosa, R. T.
DeSalvo, R.
Devenson, J.
Devine, R. C.
Dhurandhar, S.
Diaz, M. C.
Di Fiore, L.
Di Giovanni, M.
Di Girolamo, T.
Di Lieto, A.
Di Pace, S.
Di Palma, I.
Di Virgilio, A.
Doctor, Z.
Dolique, V.
Donovan, F.
Dooley, K. L.
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Dorrington, I.
Douglas, R.
Alvarez, M. Dovale
Downes, T. P.
Drago, M.
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Driggers, J. C.
Du, Z.
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Eggenstein, H-B
Ehrens, P.
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Eikenberry, S. S.
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Etienne, Z.
Etzel, T.
Evans, M.
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Everett, R.
Factourovich, M.
Fafone, V.
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Fairhurst, S.
Fan, X.
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Farr, W. M.
Fauchon-Jones, E. J.
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Fays, M.
Fehrmann, H.
Fejer, M. M.
Galiana, A. Fernandez
Ferrante, I.
Ferreira, E. C.
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Fiori, I.
Fiorucci, D.
Fisher, R. P.
Flaminio, R.
Fletcher, M.
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Forsyth, S. S.
Fournier, J-D
Frasca, S.
Frasconi, F.
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Freise, A.
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Frey, V.
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Fritschel, P.
Frolov, V. V.
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Gayathri, V.
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Gemme, G.
Genin, E.
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George, J.
Gergely, L.
Germain, V.
Ghonge, S.
Ghosh, Abhirup
Ghosh, Archisman
Ghosh, S.
Giaime, J. A.
Giardina, K. D.
Giazotto, A.
Gill, K.
Glaefke, A.
Goetz, E.
Goetz, R.
Gondan, L.
Gonzalez, G.
Castro, J. M. Gonzalez
Gopakumar, A.
Gorodetsky, M. L.
Gossan, S. E.
Gosselin, M.
Gouaty, R.
Grado, A.
Graef, C.
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Grant, A.
Gras, S.
Gray, C.
Greco, G.
Green, A. C.
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Grunewald, S.
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Guo, X.
Gupta, A.
Gupta, M. K.
Gushwa, K. E.
Gustafson, E. K.
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Hacker, J. J.
Hall, B. R.
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Vinuales, A. Vano
LIGO Sci Collaboration
Virgo Collaboration
author_role author
author2 Abbott, R.
Abbott, T. D.
Abernathy, M. R.
Acernese, F.
Ackley, K.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R. X.
Adya, V. B.
Affeldt, C.
Agathos, M.
Agatsuma, K.
Aggarwal, N.
Aguiar, O. D.
Aiello, L.
Ain, A.
Ajith, P.
Allen, B.
Allocca, A.
Altin, P. A.
Ananyeva, A.
Anderson, S. B.
Anderson, W. G.
Appert, S.
Arai, K.
Araya, M. C.
Areeda, J. S.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Aufmuth, P.
Aulbert, C.
Avila-Alvarez, A.
Babak, S.
Bacon, P.
Bader, M. K. M.
Baker, P. T.
Baldaccini, F.
Ballardin, G.
Ballmer, S. W.
Barayoga, J. C.
Barclay, S. E.
Barish, B. C.
Barker, D.
Barone, F.
Barr, B.
Barsotti, L.
Barsuglia, M.
Barta, D.
Bartlett, J.
Bartos, I.
Bassiri, R.
Basti, A.
Batch, J. C.
Baune, C.
Bavigadda, V.
Bazzan, M.
Beer, C.
Bejger, M.
Belahcene, I.
Belgin, M.
Bell, A. S.
Berger, B. K.
Bergmann, G.
Berry, C. P. L.
Bersanetti, D.
Bertolini, A.
Betzwieser, J.
Bhagwat, S.
Bhandare, R.
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Billingsley, G.
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Birch, J.
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Biscans, S.
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Blackburn, J. K.
Blackman, J.
Blair, C. D.
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Blair, R. M.
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Bohe, A.
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Boom, B. A.
Bork, R.
Boschi, V.
Bose, S.
Bouffanais, Y.
Bozzi, A.
Bradaschia, C.
Brady, P. R.
Braginsky, V. B.
Branchesi, M.
Brau, J. E.
Briant, T.
Brillet, A.
Brinkmann, M.
Brisson, V.
Brockill, P.
Broida, J. E.
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Dasgupta, A.
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Gergely, L.
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Ghosh, Archisman
Ghosh, S.
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Gopakumar, A.
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Kim, Chunglee
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Kim, Whansun
Kim, W.
Kim, Y-M
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Murray, P. G.
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Newton, G.
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Nielsen, A. B.
Nissanke, S.
Nitz, A.
Noack, A.
Nocera, F.
Nolting, D.
Normandin, M. E. N.
Nuttall, L. K.
Oberling, J.
Ochsner, E.
Oelker, E.
Ogin, G. H.
Oh, J. J.
Oh, S. H.
Ohme, F.
Oliver, M.
Oppermann, P.
Oram, Richard J.
O'Reilly, B.
O'Shaughnessy, R.
Ottaway, D. J.
Overmier, H.
Owen, B. J.
Pace, A. E.
Page, J.
Pai, A.
Pai, S. A.
Palamos, J. R.
Palashov, O.
Palomba, C.
Pal-Singh, A.
Pan, H.
Pankow, C.
Pannarale, F.
Pant, B. C.
Paoletti, F.
Paoli, A.
Papa, M. A.
Paris, H. R.
Parker, W.
Pascucci, D.
Pasqualetti, A.
Passaquieti, R.
Passuello, D.
Patricelli, B.
Pearlstone, B. L.
Pedraza, M.
Pedurand, R.
Pekowsky, L.
Pele, A.
Penn, S.
Perez, C. J.
Perreca, A.
Perri, L. M.
Pfeiffer, H. P.
Phelps, M.
Piccinni, O. J.
Pichot, M.
Piergiovanni, F.
Pierro, V.
Pillant, G.
Pinard, L.
Pinto, I. M.
Pitkin, M.
Poe, M.
Poggiani, R.
Popolizio, P.
Post, A.
Powell, J.
Prasad, J.
Pratt, J. W. W.
Predoi, V.
Prestegard, T.
Prijatelj, M.
Principe, M.
Privitera, S.
Prodi, G. A.
Prokhorov, L. G.
Puncken, O.
Punturo, M.
Puppo, P.
Puerrer, M.
Qi, H.
Qin, J.
Qiu, S.
Quetschke, V.
Quintero, E. A.
Quitzow-James, R.
Raab, F. J.
Rabeling, D. S.
Radkins, H.
Raffai, P.
Raja, S.
Rajan, C.
Rakhmanov, M.
Rapagnani, P.
Raymond, V.
Razzano, M.
Re, V.
Read, J.
Regimbau, T.
Rei, L.
Reid, S.
Reitze, D. H.
Rew, H.
Reyes, S. D.
Rhoades, E.
Ricci, F.
Riles, K.
Rizzo, M.
Robertson, N. A.
Robie, R.
Robinet, F.
Rocchi, A.
Rolland, L.
Rollins, J. G.
Roma, V. J.
Romano, J. D.
Romano, R.
Romie, J. H.
Rosinska, D.
Rowan, S.
Ruediger, A.
Ruggi, P.
Ryan, K.
Sachdev, S.
Sadecki, T.
Sadeghian, L.
Sakellariadou, M.
Salconi, L.
Saleem, M.
Salemi, F.
Samajdar, A.
Sammut, L.
Sampson, L. M.
Sanchez, E. J.
Sandberg, V.
Sanders, J. R.
Sassolas, B.
Sathyaprakash, B. S.
Saulson, P. R.
Sauter, O.
Savage, R. L.
Sawadsky, A.
Schale, P.
Scheuer, J.
Schmidt, E.
Schmidt, J.
Schmidt, P.
Schnabel, R.
Schofield, R. M. S.
Schoenbeck, A.
Schreiber, E.
Schuette, D.
Schutz, B. F.
Schwalbe, S. G.
Scott, J.
Scott, S. M.
Sellers, D.
Sengupta, A. S.
Sentenac, D.
Sequino, V.
Sergeev, A.
Setyawati, Y.
Shaddock, D. A.
Shaffer, T. J.
Shahriar, M. S.
Shapiro, B.
Shawhan, P.
Sheperd, A.
Shoemaker, D. H.
Shoemaker, D. M.
Siellez, K.
Siemens, X.
Sieniawska, M.
Sigg, D.
Silva, A. D.
Singer, A.
Singer, L. P.
Singh, A.
Singh, R.
Singhal, A.
Sintes, A. M.
Slagmolen, B. J. J.
Smith, B.
Smith, J. R.
Smith, R. J. E.
Son, E. J.
Sorazu, B.
Sorrentino, F.
Souradeep, T.
Spencer, A. P.
Srivastava, A. K.
Staley, A.
Steinke, M.
Steinlechner, J.
Steinlechner, S.
Steinmeyer, D.
Stephens, B. C.
Stevenson, S. P.
Stone, R.
Strain, K. A.
Straniero, N.
Stratta, G.
Strigin, S. E.
Sturani, R. [UNESP]
Stuver, A. L.
Summerscales, T. Z.
Sun, L.
Sunil, S.
Sutton, P. J.
Swinkels, B. L.
Szczepanczyk, M. J.
Tacca, M.
Talukder, D.
Tanner, D. B.
Tapai, M.
Taracchini, A.
Taylor, R.
Theeg, T.
Thomas, E. G.
Thomas, M.
Thomas, P.
Thorne, K. A.
Thrane, E.
Tippens, T.
Tiwari, S.
Tiwari, V.
Tokmakov, K. V.
Toland, K.
Tomlinson, C.
Tonelli, M.
Tornasi, Z.
Torrie, C. I.
Toyro, D.
Travasso, F.
Traylor, G.
Trifiro, D.
Trinastic, J.
Tringali, M. C.
Trozzo, L.
Tse, M.
Tso, R.
Turconi, M.
Tuyenbayev, D.
Ugolini, D.
Unnikrishnan, C. S.
Urban, A. L.
Usman, S. A.
Vahlbruch, H.
Vajente, G.
Valdes, G.
van Bakel, N.
van Beuzekom, M.
van den Brand, J. F. J.
Van den Broeck, C.
Vander-Hyde, D. C.
van der Schaaf, L.
van Heijningen, J. V.
van Veggel, A. A.
Vardaro, M.
Varma, V.
Vass, S.
Vasuth, M.
Vecchio, A.
Vedovato, G.
Veitch, J.
Veitch, P. J.
Venkateswara, K.
Venugopalan, G.
Verkindt, D.
Vetrano, F.
Vicere, A.
Viets, A. D.
Vinciguerra, S.
Vine, D. J.
Vinet, J-Y
Vitale, S.
Vo, T.
Vocca, H.
Vorvick, C.
Voss, D. V.
Vousden, W. D.
Vyatchanin, S. P.
Wade, A. R.
Wade, L. E.
Wade, M.
Walker, M.
Wallace, L.
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Wang, G.
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Wang, Y.
Ward, R. L.
Warner, J.
Was, M.
Watchi, J.
Weaver, B.
Wei, L-W
Weinert, M.
Weinstein, A. J.
Weiss, R.
Wen, L.
Wessels, P.
Westphal, T.
Wette, K.
Whelan, J. T.
Whiting, B. F.
Whittle, C.
Williams, D.
Williams, R. D.
Williamson, A. R.
Willis, J. L.
Willke, B.
Wimmer, M. H.
Winkler, W.
Wipf, C. C.
Wittel, H.
Woan, G.
Woehler, J.
Worden, J.
Wright, J. L.
Wu, D. S.
Wu, G.
Yam, W.
Yamamoto, H.
Yancey, C. C.
Yap, M. J.
Yu, Hang
Yu, Haocun
Yvert, M.
Zadrozny, A.
Zangrando, L.
Zanolin, M.
Zendri, J-P
Zevin, M.
Zhang, L.
Zhang, M.
Zhang, T.
Zhang, Y.
Zhao, C.
Zhou, M.
Zhou, Z.
Zhu, S. J.
Zhu, X. J.
Zucker, M. E.
Zweizig, J.
Boyle, M.
Chu, T.
Hemberger, D.
Hinder, I.
Kidder, L. E.
Ossokine, S.
Scheel, M.
Szilagyi, B.
Teukolsky, S.
Vinuales, A. Vano
LIGO Sci Collaboration
Virgo Collaboration
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dc.contributor.none.fl_str_mv CALTECH
Louisiana State Univ
Amer Univ
Univ Salerno
Ist Nazl Fis Nucl
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LIGO Livingston Observ
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dc.contributor.author.fl_str_mv Abbott, B. P.
Abbott, R.
Abbott, T. D.
Abernathy, M. R.
Acernese, F.
Ackley, K.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R. X.
Adya, V. B.
Affeldt, C.
Agathos, M.
Agatsuma, K.
Aggarwal, N.
Aguiar, O. D.
Aiello, L.
Ain, A.
Ajith, P.
Allen, B.
Allocca, A.
Altin, P. A.
Ananyeva, A.
Anderson, S. B.
Anderson, W. G.
Appert, S.
Arai, K.
Araya, M. C.
Areeda, J. S.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Aufmuth, P.
Aulbert, C.
Avila-Alvarez, A.
Babak, S.
Bacon, P.
Bader, M. K. M.
Baker, P. T.
Baldaccini, F.
Ballardin, G.
Ballmer, S. W.
Barayoga, J. C.
Barclay, S. E.
Barish, B. C.
Barker, D.
Barone, F.
Barr, B.
Barsotti, L.
Barsuglia, M.
Barta, D.
Bartlett, J.
Bartos, I.
Bassiri, R.
Basti, A.
Batch, J. C.
Baune, C.
Bavigadda, V.
Bazzan, M.
Beer, C.
Bejger, M.
Belahcene, I.
Belgin, M.
Bell, A. S.
Berger, B. K.
Bergmann, G.
Berry, C. P. L.
Bersanetti, D.
Bertolini, A.
Betzwieser, J.
Bhagwat, S.
Bhandare, R.
Bilenko, I. A.
Billingsley, G.
Billman, C. R.
Birch, J.
Birney, R.
Birnholtz, O.
Biscans, S.
Bisht, A.
Bitossi, M.
Biwer, C.
Bizouard, M. A.
Blackburn, J. K.
Blackman, J.
Blair, C. D.
Blair, D. G.
Blair, R. M.
Bloemen, S.
Bock, O.
Boer, M.
Bogaert, G.
Bohe, A.
Bondu, F.
Bonnand, R.
Boom, B. A.
Bork, R.
Boschi, V.
Bose, S.
Bouffanais, Y.
Bozzi, A.
Bradaschia, C.
Brady, P. R.
Braginsky, V. B.
Branchesi, M.
Brau, J. E.
Briant, T.
Brillet, A.
Brinkmann, M.
Brisson, V.
Brockill, P.
Broida, J. E.
Brooks, A. F.
Brown, D. A.
Brown, D. D.
Brown, N. M.
Brunett, S.
Buchanan, C. C.
Buikema, A.
Bulik, T.
Bulten, H. J.
Buonanno, A.
Buskulic, D.
Buy, C.
Byer, R. L.
Cabero, M.
Cadonati, L.
Cagnoli, G.
Cahillane, C.
Bustillo, J. Caldern
Callister, T. A.
Calloni, E.
Camp, J. B.
Cannon, K. C.
Cao, H.
Cao, J.
Capano, C. D.
Capocasa, E.
Carbognani, F.
Caride, S.
Diaz, J. Casanueva
Casentini, C.
Caudill, S.
Cavaglia, M.
Cavalier, F.
Cavalieri, R.
Cella, G.
Cepeda, C. B.
Baiardi, L. Cerboni
Cerretani, G.
Cesarini, E.
Chamberlin, S. J.
Chan, M.
Chao, S.
Charlton, P.
Chassande-Mottin, E.
Cheeseboro, B. D.
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Cripe, J.
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Cullen, T. J.
Cumming, A.
Cunningham, L.
Cuoco, E.
Dal Canton, T.
Danilishin, S. L.
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Danzmann, K.
Dasgupta, A.
Costa, C. F. Da Silva
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Dave, I.
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Davis, D.
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Vinuales, A. Vano
LIGO Sci Collaboration
Virgo Collaboration
dc.subject.por.fl_str_mv gravitational waves
numerical relativity
parameter estimation
waveform models
systematic errors
GW150914
topic gravitational waves
numerical relativity
parameter estimation
waveform models
systematic errors
GW150914
description Parameter estimates of GW150914 were obtained using Bayesian inference, based on three semi-analytic waveform models for binary black hole coalescences. These waveform models differ from each other in their treatment of black hole spins, and all three models make some simplifying assumptions, notably to neglect sub-dominant waveform harmonic modes and orbital eccentricity. Furthermore, while the models are calibrated to agree with waveforms obtained by full numerical solutions of Einstein's equations, any such calibration is accurate only to some non-zero tolerance and is limited by the accuracy of the underlying phenomenology, availability, quality, and parameter-space coverage of numerical simulations. This paper complements the original analyses of GW150914 with an investigation of the effects of possible systematic errors in the waveform models on estimates of its source parameters. To test for systematic errors we repeat the original Bayesian analysis on mock signals from numerical simulations of a series of binary configurations with parameters similar to those found for GW150914. Overall, we find no evidence for a systematic bias relative to the statistical error of the original parameter recovery of GW150914 due to modeling approximations or modeling inaccuracies. However, parameter biases are found to occur for some configurations disfavored by the data of GW150914: for binaries inclined edge-on to the detector over a small range of choices of polarization angles, and also for eccentricities greater than similar to 0.05. For signals with higher signal-to-noise ratio than GW150914, or in other regions of the binary parameter space (lower masses, larger mass ratios, or higher spins), we expect that systematic errors in current waveform models may impact gravitational-wave measurements, making more accurate models desirable for future observations.
publishDate 2017
dc.date.none.fl_str_mv 2017-05-18
2018-11-26T17:26:40Z
2018-11-26T17:26:40Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1088/1361-6382/aa6854
Classical And Quantum Gravity. Bristol: Iop Publishing Ltd, v. 34, n. 10, 48 p., 2017.
0264-9381
http://hdl.handle.net/11449/162706
10.1088/1361-6382/aa6854
WOS:000399335900001
WOS000399335900001.pdf
9756414550075565
0000-0001-9038-2951
url http://dx.doi.org/10.1088/1361-6382/aa6854
http://hdl.handle.net/11449/162706
identifier_str_mv Classical And Quantum Gravity. Bristol: Iop Publishing Ltd, v. 34, n. 10, 48 p., 2017.
0264-9381
10.1088/1361-6382/aa6854
WOS:000399335900001
WOS000399335900001.pdf
9756414550075565
0000-0001-9038-2951
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Classical And Quantum Gravity
1,809
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 48
application/pdf
dc.publisher.none.fl_str_mv Iop Publishing Ltd
publisher.none.fl_str_mv Iop Publishing Ltd
dc.source.none.fl_str_mv Web of Science
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv repositoriounesp@unesp.br
_version_ 1834484530710315008