Narrow-band search for gravitational waves from known pulsars using the second LIGO observing run
B. P. Abbott(California Institute of Technology), F. Baldaccini(University of Perugia), S. Babak, K. Agatsuma(National Institute for Subatomic Physics), O. D. Aguiar(Instituto Nacional de Pesquisas Espaciais), S. Ascenzi(Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata), R. X. Adhikari, W. G. Anderson(University of Wisconsin–Milwaukee), M. Arène(Centre National de la Recherche Scientifique), K. Ackley(University of Warwick), B. Allen(Max Planck Institute for Gravitational Physics), P. Bacon(Centre National de la Recherche Scientifique), F. Aubin(Centre National de la Recherche Scientifique), M. C. Araya(California Institute of Technology), A. Allocca(Massachusetts Institute of Technology), P. Astone(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), A. Ananyeva(California Institute of Technology), P. T. Baker(Widener University), S. Antier(Centre National de la Recherche Scientifique), M. Á. Aloy(Universitat de València), 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), V. Avendano(Montclair State University), P. Ajith(Tata Institute of Fundamental Research), T. D. Abbott(Louisiana State University), K. AultONeal(Embry–Riddle Aeronautical University), A. Amato(Université Claude Bernard Lyon 1), P. Aufmuth(Max Planck Institute for Gravitational Physics), S. V. Angelova(University of the West of Scotland), 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), F. Badaracco(Centre National de la Recherche Scientifique), A. Avila-Alvarez(California State University, Fullerton), V. B. Adya(Max Planck Institute for Gravitational Physics), S. Appert(California Institute of Technology), S. B. Anderson(California Institute of Technology), C. Adams(LIGO Scientific Collaboration), R. Abbott(National Heart Foundation of Australia), C. Austin(Louisiana State University), M. K. M. Bader(National Institute for Subatomic Physics), S. Abraham(Inter-University Centre for Astronomy and Astrophysics), N. Aggarwal(Massachusetts Institute of Technology), F. Acernese(University of Salerno), S. Bae(Korea Institute of Science & Technology Information), M. Agathos(National Institute for Subatomic Physics)
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