Improved Analysis of GW150914 Using a Fully Spin-Precessing Waveform Model
B. P. Abbott(California Institute of Technology), B. Barr(University of Glasgow), M. Agathos(National Institute for Subatomic Physics), S. Babak, K. Agatsuma(National Institute for Subatomic Physics), J. C. Barayoga(California Institute of Technology), O. D. Aguiar(Instituto Nacional de Pesquisas Espaciais), R. X. Adhikari(California Institute of Technology), 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), W. G. Anderson(University of Wisconsin–Milwaukee), M. Ast(Universität Hamburg), K. Ackley(University of Warwick), B. Allen(Max Planck Institute for Gravitational Physics), P. Bacon(Centre National de la Recherche Scientifique), S. B. Anderson(California Institute of Technology), P. Addesso(University of Sannio), T. D. Abbott(Louisiana State University), 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), G. Ashton(ARC Centre of Excellence for Gravitational Wave Discovery), L. Aiello(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso), B. C. Barish(California Institute of Technology), P. Ajith(Tata Institute of Fundamental Research), C. C. Arceneaux(University of Mississippi), P. Aufmuth(Max Planck Institute for Gravitational Physics), J. S. Areeda(California State University, Fullerton), C. Affeldt(Max Planck Institute for Gravitational Physics), 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), D. Barker, M. R. Abernathy(California Institute of Technology), G. Ballardin(European Gravitational Observatory), M. K. M. Bader(National Institute for Subatomic Physics), C. Adams(LIGO Scientific Collaboration), R. Abbott(National Heart Foundation of Australia), T. Adams(Centre National de la Recherche Scientifique), F. Baldaccini(University of Perugia), N. Aggarwal(Massachusetts Institute of Technology), S. W. Ballmer(Syracuse University), F. Acernese(University of Salerno), S. M. Aston(LIGO Scientific Collaboration), K. G. Arun(Chennai Mathematical Institute)
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