ASTROPHYSICAL IMPLICATIONS OF THE BINARY BLACK HOLE MERGER GW150914
B. P. Abbott(California Institute of Technology), B. Barr(University of Glasgow), K. G. Arun(Chennai Mathematical Institute), M. Agathos(National Institute for Subatomic Physics), S. Babak, K. Agatsuma(National Institute for Subatomic Physics), O. D. Aguiar(Instituto Nacional de Pesquisas Espaciais), M. C. Araya(California Institute of Technology), C. Aulbert(Max Planck Institute for Gravitational Physics), S. Ascenzi(Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata), R. X. Adhikari, 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), 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), 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), P. Aufmuth(Max Planck Institute for Gravitational Physics), 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), S. B. Anderson(California Institute of Technology), D. Barker, J. C. Barayoga(California Institute of Technology), 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), T. Adams(Centre National de la Recherche Scientifique), F. Baldaccini(University of Perugia), S. W. Ballmer(Syracuse University), N. Aggarwal(Massachusetts Institute of Technology), S. M. Aston(LIGO Scientific Collaboration), T. D. Abbott(Louisiana State University), J. S. Areeda(University of Genoa), R. Abbott(California Institute of Technology), F. Acernese(University of Salerno)
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