THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914

Detalhes bibliográficos
Autor(a) principal: Abbott, B. P.
Data de Publicação: 2016
Outros Autores: 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., Anderson, S. B., Anderson, W. G., Arai, K., Araya, M. C., Arceneaux, C. C., Areeda, J. S., Arnaud, N., Arun, K. G., Ascenzi, S., Ashton, G., Ast, M., Aston, S. M., Astone, P., Aufmuth, P., Aulbert, C., 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., Behnke, B., Bejger, M., Bell, A. S., Bell, C. J., Berger, B. K., Bergman, J., Bergmann, G., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhagwat, S., Bhandare, R., Bilenko, I. A., Billingsley, G., Birch, J., Birney, R., Biscans, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M. A., Blackburn, J. K., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bock, O., Bodiya, T. P., Boer, M., Bogaert, G., Bogan, C., Bohe, A., Bojtos, P., Bond, C., 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., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cadonati, L., Cagnoli, G., Cahillane, C., Calderon Bustillo, J., Callister, T., Calloni, E., Camp, J. B., Cannon, K. C., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Diaz, J. 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Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.3847/2041-8205/833/1/L1
http://hdl.handle.net/11449/162809
Resumo: A transient gravitational-wave signal, GW150914, was identified in the twin Advanced LIGO detectors on 2015 September 2015 at 09: 50: 45 UTC. To assess the implications of this discovery, the detectors remained in operation with unchanged configurations over a period of 39 days around the time of the signal. At the detection statistic threshold corresponding to that observed for GW150914, our search of the 16 days of simultaneous two-detector observational data is estimated to have a false-alarm rate (FAR) of <4.9 x 10(-6) yr(-1), yielding a p-value for GW150914 of <2 x 10(-7). Parameter estimation follow-up on this trigger identifies its source as a binary black hole (BBH) merger with component masses (m(1), m(2)) = (36(-4)(+5), 29(-4)(+4))M-circle dot at redshift z = 0.09(-0.04)(+0.03) (median and 90% credible range). Here, we report on the constraints these observations place on the rate of BBH coalescences. Considering only GW150914, assuming that all BBHs in the universe have the same masses and spins as this event, imposing a search FAR threshold of 1 per 100 years, and assuming that the BBH merger rate is constant in the comoving frame, we infer a 90% credible range of merger rates between 2-53 Gpc(-3) yr(-1)(comoving frame). Incorporating all search triggers that pass a much lower threshold while accounting for the uncertainty in the astrophysical origin of each trigger, we estimate a higher rate, ranging from 13-600 Gpc(-3) yr(-1) depending on assumptions about the BBH mass distribution. All together, our various rate estimates fall in the conservative range 2-600 Gpc(-3) yr(-1).
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spelling THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914black holesgravitational wavesstars: massiveA transient gravitational-wave signal, GW150914, was identified in the twin Advanced LIGO detectors on 2015 September 2015 at 09: 50: 45 UTC. To assess the implications of this discovery, the detectors remained in operation with unchanged configurations over a period of 39 days around the time of the signal. At the detection statistic threshold corresponding to that observed for GW150914, our search of the 16 days of simultaneous two-detector observational data is estimated to have a false-alarm rate (FAR) of <4.9 x 10(-6) yr(-1), yielding a p-value for GW150914 of <2 x 10(-7). Parameter estimation follow-up on this trigger identifies its source as a binary black hole (BBH) merger with component masses (m(1), m(2)) = (36(-4)(+5), 29(-4)(+4))M-circle dot at redshift z = 0.09(-0.04)(+0.03) (median and 90% credible range). Here, we report on the constraints these observations place on the rate of BBH coalescences. Considering only GW150914, assuming that all BBHs in the universe have the same masses and spins as this event, imposing a search FAR threshold of 1 per 100 years, and assuming that the BBH merger rate is constant in the comoving frame, we infer a 90% credible range of merger rates between 2-53 Gpc(-3) yr(-1)(comoving frame). Incorporating all search triggers that pass a much lower threshold while accounting for the uncertainty in the astrophysical origin of each trigger, we estimate a higher rate, ranging from 13-600 Gpc(-3) yr(-1) depending on assumptions about the BBH mass distribution. All together, our various rate estimates fall in the conservative range 2-600 Gpc(-3) yr(-1).Council 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 CompetitivitatConselleria 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 InnovationRussian Foundation for Basic ResearchLeverhulme TrustMinistry of Science and Technology (MOST), TaiwanKavli FoundationScience and Technology Facilities CouncilCALTECH, LIGO, Pasadena, CA 91125 USALouisiana State Univ, Baton Rouge, LA 70803 USAUniv Salerno, I-84084 Salerno, ItalyComplesso Univ Monte S Angelo, Sez Napoli, Ist Nazl Fis Nucl, I-80126 Naples, ItalyUniv Florida, Gainesville, FL 32611 USALIGO Livingston Observ, Livingston, LA 70754 USAUniv Savoie Mont Blanc, CNRS IN2P3, LAPP, F-74941 Annecy Le Vieux, FranceMax Planck Inst Gravitatphys, 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, Sao Jose dos Campos, BR-12227010 Sao Paulo, BrazilGran Sasso Sci Inst, Ist Nazl Fis Nucl, I-67100 Laquila, ItalyIst Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, ItalyInteruniv Ctr for Astron & Astrophys, Pune 411007, Maharashtra, IndiaTata Inst Fundamental Res, Int Ctr Theoret Sci, Bangalore 560012, Karnataka, IndiaUniv Wisconsin, 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, AustraliaUniv Mississippi, University, MS 38677 USACalif State Univ Fullerton, Fullerton, CA 92831 USAUniv Paris 11, LAL, CNRS IN2P3, Univ Paris Saclay, F-91400 Orsay, FranceChennai Math Inst, Madras 603103, Tamil Nadu, IndiaUniv Roma Tor Vergata, I-00133 Rome, ItalyUniv Southampton, Southampton SO17 1BJ, Hants, EnglandUniv Hamburg, D-22761 Hamburg, GermanyIst Nazl Fis Nucl, Sez Roma, I-00185 Rome, ItalyMax Planck Inst Gravitatphys, Albert Einstein Inst, D-14476 Potsdam, GermanyUniv Paris Diderot, APC, AstroParticule & Cosmol, CNRS IN2P3,CEA Irfu,Observ Paris,Sorbonne Paris C, F-75205 Paris, FranceMontana State Univ, Bozeman, MT 59717 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, ItalyUniv Padua, Sez Padova, I-35131 Padua, ItalyCAMK PAN, PL-00716 Warsaw, PolandUniv Birmingham, Birmingham B15 2TT, W Midlands, EnglandUniv Genoa, I-16146 Genoa, ItalyIst Nazl Fis Nucl, Sez Genova, I-16146 Genoa, ItalyRRCAT, Indore 452013, Madhya Pradesh, IndiaLomonosov Moscow State Univ, Fac Phys, Moscow 119991, RussiaUniv West Scotland, SUPA, Paisley PA1 2BE, Renfrew, ScotlandUniv Western Australia, Nedlands, WA 6009, AustraliaRadboud Univ Nijmegen, Dept Astrophys, IMAPP, POB 9010, NL-6500 GL Nijmegen, NetherlandsUniv Cote Azur, Artemis, CNRS, Observ Cote Azur, F-34229 Nice 4, FranceMTA Eotvos Univ, Lendulet Astrophys Res Grp, H-1117 Budapest, HungaryUniv Rennes 1, Inst Phys Rennes, 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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.Anderson, S. B.Anderson, W. G.Arai, K.Araya, M. C.Arceneaux, C. C.Areeda, J. S.Arnaud, N.Arun, K. G.Ascenzi, S.Ashton, G.Ast, M.Aston, S. M.Astone, P.Aufmuth, P.Aulbert, C.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.Behnke, B.Bejger, M.Bell, A. S.Bell, C. J.Berger, B. K.Bergman, J.Bergmann, G.Berry, C. P. L.Bersanetti, D.Bertolini, A.Betzwieser, J.Bhagwat, S.Bhandare, R.Bilenko, I. A.Billingsley, G.Birch, J.Birney, R.Biscans, S.Bisht, A.Bitossi, M.Biwer, C.Bizouard, M. A.Blackburn, J. K.Blair, C. D.Blair, D. G.Blair, R. 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Bristol: Iop Publishing Ltd, v. 833, n. 1, 8 p., 2016.2041-8205http://hdl.handle.net/11449/16280910.3847/2041-8205/833/1/L1WOS:000401603900001WOS000401603900001.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAstrophysical Journal Letters3,186info:eu-repo/semantics/openAccess2023-12-15T06:14:47Zoai:repositorio.unesp.br:11449/162809Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T20:21:59.230058Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914
title THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914
spellingShingle THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914
Abbott, B. P.
black holes
gravitational waves
stars: massive
title_short THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914
title_full THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914
title_fullStr THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914
title_full_unstemmed THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914
title_sort THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING 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.
Anderson, S. B.
Anderson, W. G.
Arai, K.
Araya, M. C.
Arceneaux, C. C.
Areeda, J. S.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Aufmuth, P.
Aulbert, C.
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.
Behnke, B.
Bejger, M.
Bell, A. S.
Bell, C. J.
Berger, B. K.
Bergman, J.
Bergmann, G.
Berry, C. P. L.
Bersanetti, D.
Bertolini, A.
Betzwieser, J.
Bhagwat, S.
Bhandare, R.
Bilenko, I. A.
Billingsley, G.
Birch, J.
Birney, R.
Biscans, S.
Bisht, A.
Bitossi, M.
Biwer, C.
Bizouard, M. A.
Blackburn, J. K.
Blair, C. D.
Blair, D. G.
Blair, R. M.
Bloemen, S.
Bock, O.
Bodiya, T. P.
Boer, M.
Bogaert, G.
Bogan, C.
Bohe, A.
Bojtos, P.
Bond, C.
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.
Brooks, A. F.
Brown, D. A.
Brown, D. D.
Brown, N. M.
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Piergiovanni, F.
Pierro, V.
Pillant, G.
Pinard, L.
Pinto, I. M.
Pitkin, M.
Poggiani, R.
Popolizio, P.
Porter, E. K.
Post, A.
Powell, J.
Prasad, J.
Predoi, V.
Premachandra, S. S.
Prestegard, T.
Price, L. R.
Prijatelj, M.
Principe, M.
Privitera, S.
Prodi, G. A.
Prokhorov, L.
Puncken, O.
Punturo, M.
Puppo, P.
Puerrer, M.
Qi, H.
Qin, J.
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Raab, F. J.
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Radkins, H.
Raffai, P.
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Rakhmanov, M.
Rapagnani, P.
Raymond, V.
Razzano, M.
Re, V.
Read, J.
Reed, C. M.
Regimbau, T.
Rei, L.
Reid, S.
Reitze, D. H.
Rew, H.
Reyes, S. D.
Ricci, F.
Riles, K.
Robertson, N. A.
Robie, R.
Robinet, F.
Rocchi, A.
Rolland, L.
Rollins, J. G.
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Romano, R.
Romanov, G.
Romie, J. H.
Rosinska, D.
Rowan, S.
Ruediger, A.
Ruggi, P.
Ryan, K.
Sachdev, S.
Sadecki, T.
Sadeghian, L.
Salconi, L.
Saleem, M.
Salemi, F.
Samajdar, A.
Sammut, L.
Sampson, L.
Sanchez, E. J.
Sandberg, V.
Sandeen, B.
Sanders, J. R.
Sassolas, B.
Sathyaprakash, B. S.
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Sauter, O.
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Schofield, R. M. S.
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Schutz, B. F.
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Scott, S. M.
Sellers, D.
Sengupta, A. S.
Sentenac, D.
Sequino, V.
Sergeev, A.
Serna, G.
Setyawati, Y.
Sevigny, A.
Shaddock, D. A.
Shah, S.
Shahriar, M. S.
Shaltev, M.
Shao, Z.
Shapiro, B.
Shawhan, P.
Sheperd, A.
Shoemaker, D. H.
Shoemaker, D. M.
Siellez, K.
Siemens, X.
Sigg, D.
Silva, A. D.
Simakov, D.
Singer, A.
Singer, L. P.
Singh, A.
Singh, R.
Singhal, A.
Sintes, A. M.
Slagmolen, B. J. J.
Smith, J. R.
Smith, N. D.
Smith, R. J. E.
Son, E. J.
Sorazu, B.
Sorrentino, F.
Souradeep, T.
Srivastava, A. K.
Staley, A.
Steinke, M.
Steinlechner, J.
Steinlechner, S.
Steinmeyer, D.
Stephens, B. C.
Stevenson, S.
Stone, R.
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Stratta, G.
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Strigin, S.
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Stuver, A. L.
Summerscales, T. Z.
Sun, L.
Sutton, P. J.
Swinkels, B. L.
Szczepanczyk, M. J.
Tacca, M.
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Tanner, D. B.
Tapai, M.
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Taracchini, A.
Taylor, R.
Theeg, T.
Thirugnanasambandam, M. P.
Thomas, E. G.
Thomas, M.
Thomas, P.
Thorne, K. A.
Thorne, K. S.
Thrane, E.
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Tiwari, V.
Tokmakov, K. V.
Tomlinson, C.
Tonelli, M.
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Torrie, C. I.
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Tringali, M. C.
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Tse, M.
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Tuyenbayev, D.
Ugolini, D.
Unnikrishnan, C. S.
Urban, A. L.
Usman, S. A.
Vahlbruch, H.
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Valdes, G.
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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.
Vass, S.
Vasuth, M.
Vaulin, R.
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Vedovato, G.
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Veitch, P. J.
Venkateswara, K.
Verkindt, D.
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Vicere, A.
Vinciguerra, S.
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Vinet, J. -Y.
Vitale, S.
Vo, T.
Vocca, H.
Vorvick, C.
Voss, D.
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, X.
Wang, Y.
Ward, R. L.
Warner, J.
Was, M.
Weaver, B.
Wei, L. -W.
Weinert, M.
Weinstein, A. J.
Weiss, R.
Welborn, T.
Wen, L.
Wesels, P.
Westphal, T.
Wette, K.
Whelan, J. T.
White, D. J.
Whiting, B. F.
Williams, R. D.
Williamson, A. R.
Willis, J. L.
Willke, B.
Wimmer, M. H.
Winkler, W.
Wipf, C. C.
Wittel, H.
Woan, G.
Worden, J.
Wright, J. L.
Wu, G.
Yablon, J.
Yam, W.
Yamamoto, H.
Yancey, C. C.
Yap, M. J.
Yu, H.
Yvert, M.
Zadrozny, A.
Zangrando, L.
Zanolin, M.
Zendri, J. -P.
Zevin, M.
Zhang, F.
Zhang, L.
Zhang, M.
Zhang, Y.
Zhao, C.
Zhou, M.
Zhou, Z.
Zhu, X. J.
Zucker, M. E.
Zuraw, S. E.
Zweizig, J.
LIGO Scientific Collaboration
Vigro 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.
Anderson, S. B.
Anderson, W. G.
Arai, K.
Araya, M. C.
Arceneaux, C. C.
Areeda, J. S.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Aufmuth, P.
Aulbert, C.
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.
Behnke, B.
Bejger, M.
Bell, A. S.
Bell, C. J.
Berger, B. K.
Bergman, J.
Bergmann, G.
Berry, C. P. L.
Bersanetti, D.
Bertolini, A.
Betzwieser, J.
Bhagwat, S.
Bhandare, R.
Bilenko, I. A.
Billingsley, G.
Birch, J.
Birney, R.
Biscans, S.
Bisht, A.
Bitossi, M.
Biwer, C.
Bizouard, M. A.
Blackburn, J. K.
Blair, C. D.
Blair, D. G.
Blair, R. M.
Bloemen, S.
Bock, O.
Bodiya, T. P.
Boer, M.
Bogaert, G.
Bogan, C.
Bohe, A.
Bojtos, P.
Bond, C.
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.
Brooks, A. F.
Brown, D. A.
Brown, D. D.
Brown, N. M.
Buchanan, C. C.
Buikema, A.
Bulik, T.
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Buonanno, A.
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Buy, C.
Byer, R. L.
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Cagnoli, G.
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Calderon Bustillo, J.
Callister, T.
Calloni, E.
Camp, J. B.
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Cao, J.
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Capocasa, E.
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Caride, S.
Diaz, J. Casanueva
Casentini, C.
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Cavalier, F.
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Cella, G.
Cepeda, C. B.
Baiardi, L. Cerboni
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Cesarini, E.
Chakraborty, R.
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Chamberlin, S. J.
Chan, M.
Chao, S.
Charlton, P.
Chassande-Mottin, E.
Chen, H. Y.
Chen, Y.
Cheng, C.
Chincarini, A.
Chiummo, A.
Cho, H. S.
Cho, M.
Chow, J. H.
Christensen, N.
Chu, Q.
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Cleva, F.
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Cohadon, P. -F.
Colla, A.
Collette, C. G.
Cominsky, L.
Constancio, M.
Conte, A.
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Cook, D.
Corbitt, T. R.
Cornish, N.
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Coughlin, M. W.
Coughlin, S. B.
Coulon, J. -P.
Countryman, S. T.
Couvares, P.
Cowan, E. E.
Coward, D. M.
Cowart, M. J.
Coyne, D. C.
Coyne, R.
Craig, K.
Creighton, J. D. E.
Cripe, J.
Crowder, S. G.
Cumming, A.
Cunningham, L.
Cuoco, E.
Dal Canton, T.
Danilishin, S. L.
D'Antonio, S.
Danzmann, K.
Darman, N. S.
Dattilo, V.
Dave, I.
Daveloza, H. P.
Davier, M.
Davies, G. S.
Daw, E. J.
Day, R.
De, S.
DeBra, D.
Debreczeni, G.
Degallaix, J.
De Laurentis, M.
Deleglise, S.
Del Pozzo, W.
Denker, T.
Dent, T.
Dereli, H.
Dergachev, V.
De Rosa, R.
DeRosa, R. T.
DeSalvo, R.
Dhurandhar, S.
Diaz, M. C.
Di Fiore, L.
Di Giovanni, M.
Di Lieto, A.
Di Pace, S.
Di Palma, I.
Di Virgilio, A.
Dojcinoski, G.
Dolique, V.
Donovan, F.
Dooley, K. L.
Doravari, S.
Douglas, R.
Downes, T. P.
Drago, M.
Drever, R. W. P.
Driggers, J. C.
Du, Z.
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Dwyer, S. E.
Edo, T. B.
Edwards, M. C.
Effler, A.
Eggenstein, H. -B.
Ehrens, P.
Eichholz, J.
Eikenberry, S. S.
Engels, W.
Essick, R. C.
Etzel, T.
Evans, M.
Evans, T. M.
Everett, R.
Factourovich, M.
Fafone, V.
Fair, H.
Fairhurst, S.
Fan, X.
Fang, Q.
Farinon, S.
Farr, B.
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Favata, M.
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Fehrmann, H.
Fejer, M. M.
Ferrante, I.
Ferreira, E. C.
Ferrini, F.
Fidecaro, F.
Fiori, I.
Fiorucci, D.
Fisher, R. P.
Flaminio, R.
Fletcher, M.
Fong, H.
Fournier, J. -D.
Franco, S.
Frasca, S.
Frasconi, F.
Frei, Z.
Freise, A.
Frey, R.
Frey, V.
Fricke, T. T.
Fritschel, P.
Frolov, V. V.
Fulda, P.
Fyffe, M.
Gabbard, H. A. G.
Gair, J. R.
Gammaitoni, L.
Gaonkar, S. G.
Garufi, F.
Gatto, A.
Gaur, G.
Gehrels, N.
Gemme, G.
Gendre, B.
Genin, E.
Gennai, A.
George, J.
Gergely, L.
Germain, V.
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.
Gordon, N. A.
Gorodetsky, M. L.
Gossan, S. E.
Gosselin, M.
Gouaty, R.
Graef, C.
Graff, P. B.
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.
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.
Heidmann, A.
Heintze, M. C.
Heitmann, H.
Hello, P.
Hemming, G.
Hendry, M.
Heng, I. S.
Hennig, J.
Heptonstall, A. W.
Heurs, M.
Hild, S.
Hoak, D.
Hodge, K. A.
Hofman, D.
Hollitt, S. E.
Holt, K.
Holz, D. E.
Hopkins, P.
Hosken, D. J.
Hough, J.
Houston, E. A.
Howell, E. J.
Hu, Y. M.
Huang, S.
Huerta, E. A.
Huet, D.
Hughey, B.
Husa, S.
Huttner, S. H.
Huynh-Dinh, T.
Idrisy, A.
Indik, N.
Ingram, D. R.
Inta, R.
Isa, H. N.
Isac, J. -M.
Isi, M.
Islas, G.
Isogai, T.
Iyer, B. R.
Izumi, K.
Jacqmin, T.
Jang, H.
Jani, K.
Jaranowski, P.
Jawahar, S.
Jimenez-Forteza, F.
Johnson, W. W.
Jones, D. I.
Jones, R.
Jonker, R. J. G.
Ju, L.
Haris, K.
Kalaghatgi, C. V.
Kalogera, V.
Kandhasamy, S.
Kang, G.
Kanner, J. B.
Karki, S.
Kasprzack, M.
Katsavounidis, E.
Katzman, W.
Kaufer, S.
Kaur, T.
Kawabe, K.
Kawazoe, F.
Kefelian, F.
Kehl, M. S.
Keitel, D.
Kelley, D. B.
Kells, W.
Kennedy, R.
Key, J. S.
Khalaidovski, A.
Khalili, F. Y.
Khan, I.
Khan, S.
Khan, Z.
Khazanov, E. A.
Kijbunchoo, N.
Kim, C.
Kim, J.
Kim, K.
Kim, Nam-Gyu
Kim, Namjun
Kim, Y. -M.
King, E. J.
King, P. J.
Kinzel, D. L.
Kissel, J. S.
Kleybolte, L.
Klimenko, S.
Koehlenbeck, S. M.
Kokeyama, K.
Koley, S.
Kondrashov, V.
Kontos, A.
Korobko, M.
Korth, W. Z.
Kowalska, I.
Kozak, D. B.
Kringel, V.
Krishnan, B.
Krolak, A.
Krueger, C.
Kuehn, G.
Kumar, P.
Kuo, L.
Kutynia, A.
Lackey, B. D.
Landry, M.
Lange, J.
Lantz, B.
Lasky, P. D.
Lazzarini, A.
Lazzaro, C.
Leaci, P.
Leavey, S.
Lebigot, E. O.
Lee, C. H.
Lee, H. K.
Lee, H. M.
Lee, K.
Lenon, A.
Leonardi, M.
Leong, J. R.
Leroy, N.
Letendre, N.
Levin, Y.
Levine, B. M.
Li, T. G. F.
Libson, A.
Littenberg, T. B.
Lockerbie, N. A.
Logue, J.
Lombardi, A. L.
Lord, J. E.
Lorenzini, M.
Loriette, V.
Lormand, M.
Losurdo, G.
Lough, J. D.
Lueck, H.
Lundgren, A. P.
Luo, J.
Lynch, R.
Ma, Y.
MacDonald, T.
Machenschalk, B.
Maclnnis, M.
Macleod, D. M.
Magana-Sandoval, F.
Magee, R. M.
Mageswaran, M.
Majorana, E.
Maksimovic, I.
Malvezzi, V.
Man, N.
Mandel, I.
Mandic, V.
Mangano, V.
Mansell, G. L.
Manske, M.
Mantovani, M.
Marchesoni, F.
Marion, F.
Marka, S.
Marka, Z.
Markosyan, A. S.
Maros, E.
Martelli, F.
Martellini, L.
Martin, I. W.
Martin, R. M.
Martynov, D. V.
Marx, J. N.
Mason, K.
Masserot, A.
Massinger, T. J.
Masso-Reid, M.
Matichard, F.
Matone, L.
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Mazumder, N.
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McCarthy, R.
McClelland, D. E.
McCormick, S.
McGuire, S. C.
Mclntyre, G.
Mclver, J.
McManus, D. J.
McWilliams, S. T.
Meacher, D.
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Meidam, J.
Melatos, A.
Mendell, G.
Mendoza-Gandara, D.
Mercer, R. A.
Merilh, E.
Merzougui, M.
Meshkov, S.
Messenger, C.
Messick, C.
Meyers, P. M.
Mezzani, F.
Miao, H.
Michel, C.
Middleton, H.
Mikhailov, E. E.
Milano, L.
Miller, J.
Millhouse, M.
Minenkov, Y.
Ming, J.
Mirshekari, S. [UNESP]
Mishra, C.
Mitra, S.
Mitrofanov, V. P.
Mitselmakher, G.
Mittleman, R.
Moggi, A.
Mohan, M.
Mohapatra, S. R. P.
Montani, M.
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Moore, C. J.
Moraru, D.
Moreno, G.
Morriss, S. R.
Mossavi, K.
Mours, B.
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Mueller, C. L.
Mueller, G.
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Mukherjee, Arunava
Mukherjee, D.
Mukherjee, S.
Mukund, N.
Mullavey, A.
Munch, J.
Murphy, D. J.
Murray, P. G.
Mytidis, A.
Nardecchia, I.
Naticchioni, L.
Nayak, R. K.
Necula, V.
Nedkova, K.
Nelemans, G.
Neri, M.
Neunzert, A.
Newton, G.
Nguyen, T. T.
Nielsen, A. B.
Nissanke, S.
Nitz, A.
Nocera, F.
Nolting, D.
Normandin, M. E.
Nuttall, L. K.
Oberling, J.
Ochsner, E.
O'Dell, J.
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.
Ottens, R. S.
Overmier, H.
Owen, B. 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.
Patrick, Z.
Pearlstone, B. L.
Pedraza, M.
Pedurand, R.
Pekowsky, L.
Pele, A.
Penn, S.
Perreca, A.
Phelps, M.
Piccinni, O.
Pichot, M.
Piergiovanni, F.
Pierro, V.
Pillant, G.
Pinard, L.
Pinto, I. M.
Pitkin, M.
Poggiani, R.
Popolizio, P.
Porter, E. K.
Post, A.
Powell, J.
Prasad, J.
Predoi, V.
Premachandra, S. S.
Prestegard, T.
Price, L. R.
Prijatelj, M.
Principe, M.
Privitera, S.
Prodi, G. A.
Prokhorov, L.
Puncken, O.
Punturo, M.
Puppo, P.
Puerrer, M.
Qi, H.
Qin, J.
Quetschke, V.
Quintero, E. A.
Quitzow-James, R.
Raab, F. J.
Rabeling, D. S.
Radkins, H.
Raffai, P.
Raja, S.
Rakhmanov, M.
Rapagnani, P.
Raymond, V.
Razzano, M.
Re, V.
Read, J.
Reed, C. M.
Regimbau, T.
Rei, L.
Reid, S.
Reitze, D. H.
Rew, H.
Reyes, S. D.
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Riles, K.
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Robinet, F.
Rocchi, A.
Rolland, L.
Rollins, J. G.
Roma, V. J.
Romano, R.
Romanov, G.
Romie, J. H.
Rosinska, D.
Rowan, S.
Ruediger, A.
Ruggi, P.
Ryan, K.
Sachdev, S.
Sadecki, T.
Sadeghian, L.
Salconi, L.
Saleem, M.
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Samajdar, A.
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Sengupta, A. S.
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Singhal, A.
Sintes, A. M.
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Smith, N. D.
Smith, R. J. E.
Son, E. J.
Sorazu, B.
Sorrentino, F.
Souradeep, T.
Srivastava, A. K.
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Steinke, M.
Steinlechner, J.
Steinlechner, S.
Steinmeyer, D.
Stephens, B. C.
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Stone, R.
Strain, K. A.
Straniero, N.
Stratta, G.
Strauss, N. A.
Strigin, S.
Sturani, R. [UNESP]
Stuver, A. L.
Summerscales, T. Z.
Sun, L.
Sutton, P. J.
Swinkels, B. L.
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Tacca, M.
Talukder, D.
Tanner, D. B.
Tapai, M.
Tarabrin, S. P.
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Theeg, T.
Thirugnanasambandam, M. P.
Thomas, E. G.
Thomas, M.
Thomas, P.
Thorne, K. A.
Thorne, K. S.
Thrane, E.
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Tiwari, V.
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Tonelli, M.
Torres, C. V.
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Trifiro, D.
Tringali, M. C.
Trozzo, L.
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Turconi, M.
Tuyenbayev, D.
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Unnikrishnan, C. S.
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Vajente, G.
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Vecchio, A.
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Williamson, A. R.
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Wipf, C. C.
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Woan, G.
Worden, J.
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Yvert, M.
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Zangrando, L.
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Zendri, J. -P.
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Zhang, Y.
Zhao, C.
Zhou, M.
Zhou, Z.
Zhu, X. J.
Zucker, M. E.
Zuraw, S. E.
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LIGO Scientific Collaboration
Vigro Collaboration
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dc.contributor.none.fl_str_mv CALTECH
Louisiana State Univ
Univ Salerno
Complesso Univ Monte S Angelo
Univ Florida
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Max Planck Inst Gravitatphys
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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.
Anderson, S. B.
Anderson, W. G.
Arai, K.
Araya, M. C.
Arceneaux, C. C.
Areeda, J. S.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Aufmuth, P.
Aulbert, C.
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.
Behnke, B.
Bejger, M.
Bell, A. S.
Bell, C. J.
Berger, B. K.
Bergman, J.
Bergmann, G.
Berry, C. P. L.
Bersanetti, D.
Bertolini, A.
Betzwieser, J.
Bhagwat, S.
Bhandare, R.
Bilenko, I. A.
Billingsley, G.
Birch, J.
Birney, R.
Biscans, S.
Bisht, A.
Bitossi, M.
Biwer, C.
Bizouard, M. A.
Blackburn, J. K.
Blair, C. D.
Blair, D. G.
Blair, R. M.
Bloemen, S.
Bock, O.
Bodiya, T. P.
Boer, M.
Bogaert, G.
Bogan, C.
Bohe, A.
Bojtos, P.
Bond, C.
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.
Brooks, A. F.
Brown, D. A.
Brown, D. D.
Brown, N. M.
Buchanan, C. C.
Buikema, A.
Bulik, T.
Bulten, H. J.
Buonanno, A.
Buskulic, D.
Buy, C.
Byer, R. L.
Cadonati, L.
Cagnoli, G.
Cahillane, C.
Calderon Bustillo, J.
Callister, T.
Calloni, E.
Camp, J. B.
Cannon, K. C.
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.
Chakraborty, R.
Chalermsongsak, T.
Chamberlin, S. J.
Chan, M.
Chao, S.
Charlton, P.
Chassande-Mottin, E.
Chen, H. Y.
Chen, Y.
Cheng, C.
Chincarini, A.
Chiummo, A.
Cho, H. S.
Cho, M.
Chow, J. H.
Christensen, N.
Chu, Q.
Chua, S.
Chung, S.
Ciani, G.
Clara, F.
Clark, J. A.
Cleva, F.
Coccia, E.
Cohadon, P. -F.
Colla, A.
Collette, C. G.
Cominsky, L.
Constancio, M.
Conte, A.
Conti, L.
Cook, D.
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.
Cowan, E. E.
Coward, D. M.
Cowart, M. J.
Coyne, D. C.
Coyne, R.
Craig, K.
Creighton, J. D. E.
Cripe, J.
Crowder, S. G.
Cumming, A.
Cunningham, L.
Cuoco, E.
Dal Canton, T.
Danilishin, S. L.
D'Antonio, S.
Danzmann, K.
Darman, N. S.
Dattilo, V.
Dave, I.
Daveloza, H. P.
Davier, M.
Davies, G. S.
Daw, E. J.
Day, R.
De, S.
DeBra, D.
Debreczeni, G.
Degallaix, J.
De Laurentis, M.
Deleglise, S.
Del Pozzo, W.
Denker, T.
Dent, T.
Dereli, H.
Dergachev, V.
De Rosa, R.
DeRosa, R. T.
DeSalvo, R.
Dhurandhar, S.
Diaz, M. C.
Di Fiore, L.
Di Giovanni, M.
Di Lieto, A.
Di Pace, S.
Di Palma, I.
Di Virgilio, A.
Dojcinoski, G.
Dolique, V.
Donovan, F.
Dooley, K. L.
Doravari, S.
Douglas, R.
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.
Engels, W.
Essick, R. C.
Etzel, T.
Evans, M.
Evans, T. M.
Everett, R.
Factourovich, M.
Fafone, V.
Fair, H.
Fairhurst, S.
Fan, X.
Fang, Q.
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Yu, H.
Yvert, M.
Zadrozny, A.
Zangrando, L.
Zanolin, M.
Zendri, J. -P.
Zevin, M.
Zhang, F.
Zhang, L.
Zhang, M.
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Zweizig, J.
LIGO Scientific Collaboration
Vigro Collaboration
dc.subject.por.fl_str_mv black holes
gravitational waves
stars: massive
topic black holes
gravitational waves
stars: massive
description A transient gravitational-wave signal, GW150914, was identified in the twin Advanced LIGO detectors on 2015 September 2015 at 09: 50: 45 UTC. To assess the implications of this discovery, the detectors remained in operation with unchanged configurations over a period of 39 days around the time of the signal. At the detection statistic threshold corresponding to that observed for GW150914, our search of the 16 days of simultaneous two-detector observational data is estimated to have a false-alarm rate (FAR) of <4.9 x 10(-6) yr(-1), yielding a p-value for GW150914 of <2 x 10(-7). Parameter estimation follow-up on this trigger identifies its source as a binary black hole (BBH) merger with component masses (m(1), m(2)) = (36(-4)(+5), 29(-4)(+4))M-circle dot at redshift z = 0.09(-0.04)(+0.03) (median and 90% credible range). Here, we report on the constraints these observations place on the rate of BBH coalescences. Considering only GW150914, assuming that all BBHs in the universe have the same masses and spins as this event, imposing a search FAR threshold of 1 per 100 years, and assuming that the BBH merger rate is constant in the comoving frame, we infer a 90% credible range of merger rates between 2-53 Gpc(-3) yr(-1)(comoving frame). Incorporating all search triggers that pass a much lower threshold while accounting for the uncertainty in the astrophysical origin of each trigger, we estimate a higher rate, ranging from 13-600 Gpc(-3) yr(-1) depending on assumptions about the BBH mass distribution. All together, our various rate estimates fall in the conservative range 2-600 Gpc(-3) yr(-1).
publishDate 2016
dc.date.none.fl_str_mv 2016-12-10
2018-11-26T17:31:29Z
2018-11-26T17:31:29Z
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/10.3847/2041-8205/833/1/L1
Astrophysical Journal Letters. Bristol: Iop Publishing Ltd, v. 833, n. 1, 8 p., 2016.
2041-8205
http://hdl.handle.net/11449/162809
10.3847/2041-8205/833/1/L1
WOS:000401603900001
WOS000401603900001.pdf
url http://dx.doi.org/10.3847/2041-8205/833/1/L1
http://hdl.handle.net/11449/162809
identifier_str_mv Astrophysical Journal Letters. Bristol: Iop Publishing Ltd, v. 833, n. 1, 8 p., 2016.
2041-8205
10.3847/2041-8205/833/1/L1
WOS:000401603900001
WOS000401603900001.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Astrophysical Journal Letters
3,186
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 8
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
_version_ 1808129193512271872