Directly comparing GW150914 with numerical solutions of Einstein’s equations for binary black hole coalescence
B. P. Abbott(California Institute of Technology), B. Barr(University of Glasgow), S. Babak, P. Aufmuth(Leibniz University Hannover), O. D. Aguiar(Instituto Nacional de Pesquisas Espaciais), C. Aulbert(Max Planck Institute for Gravitational Physics), M. C. Araya(California Institute of Technology), S. Ascenzi(Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata), R. X. Adhikari, W. G. Anderson(University of Wisconsin–Milwaukee), F. Acernese(University of Salerno), M. Ast(Universität Hamburg), K. Ackley(University of Warwick), C. Affeldt(Max Planck Institute for Gravitational Physics), B. Allen(Max Planck Institute for Gravitational Physics), P. Bacon(Centre National de la Recherche Scientifique), B. C. Barish(California Institute of Technology), P. Addesso(University of Sannio), F. Barone(University of Salerno), A. Allocca(Massachusetts Institute of Technology), P. Astone(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), P. T. Baker(Widener University), N. Arnaud(Université Paris-Sud), A. Ain(University of Antwerp), S. M. Aston(LIGO Scientific Collaboration), G. Ashton(ARC Centre of Excellence for Gravitational Wave Discovery), L. Aiello(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso), P. Ajith(Tata Institute of Fundamental Research), C. C. Arceneaux(University of Mississippi), G. Ballardin(European Gravitational Observatory), J. S. Areeda(California State University, Fullerton), K. Arai(California Institute of Technology), P. A. Altin(Australian National University), S. E. Barclay(University of Glasgow), V. B. Adya(Max Planck Institute for Gravitational Physics), S. B. Anderson(California Institute of Technology), D. Barker, J. C. Barayoga(California Institute of Technology), M. R. Abernathy(California Institute of Technology), C. Adams(LIGO Scientific Collaboration), R. Abbott(National Heart Foundation of Australia), M. K. M. Bader(National Institute for Subatomic Physics), T. Adams(Centre National de la Recherche Scientifique), F. Baldaccini(University of Perugia), N. Aggarwal(Massachusetts Institute of Technology), K. Agatsuma(National Institute for Subatomic Physics), S. W. Ballmer(Syracuse University), K. G. Arun(Chennai Mathematical Institute), T. D. Abbott(Louisiana State University), M. Agathos(National Institute for Subatomic Physics)
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