Skip to main content
Article
Supplement: The Rate Of Binary Black Hole Mergers Inferred From Advanced Ligo Observations Surrounding Gw150914
Astrophysical Journal, Supplement Series
  • B. P. Abbott, California Institute of Technology
  • R. Abbott, California Institute of Technology
  • T. D. Abbott, Louisiana State University
  • M. R. Abernathy, California Institute of Technology
  • F. Acernese, Università di Salerno
  • K. Ackley, University of Florida
  • C. Adams, LIGO Livingston
  • T. Adams, Université Savoie Mont Blanc
  • P. Addesso, Università di Salerno
  • R. X. Adhikari, California Institute of Technology
  • V. B. Adya, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • C. Affeldt, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • M. Agathos, FOM-Institute of Subatomic Physics - NIKHEF
  • K. Agatsuma, FOM-Institute of Subatomic Physics - NIKHEF
  • N. Aggarwal, LIGO, Massachusetts Institute of Technology
  • O. D. Aguiar, Instituto Nacional de Pesquisas Espaciais
  • L. Aiello, Istituto Nazionale di Fisica Nucleare - INFN
  • A. Ain, Inter-University Centre for Astronomy and Astrophysics India
  • P. Ajith, Tata Institute of Fundamental Research, Mumbai
  • B. Allen, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • A. Allocca, Università di Pisa
  • P. A. Altin, The Australian National University
  • S. B. Anderson, California Institute of Technology
  • W. G. Anderson, University of Wisconsin-Milwaukee
  • K. Arai, California Institute of Technology
  • M. C. Araya, California Institute of Technology
  • C. C. Arceneaux, University of Mississippi
  • J. S. Areeda, California State University, Fullerton
  • N. Arnaud, Laboratoire de l'Accélérateur Linéaire
  • K. G. Arun, Chennai Mathematical Institute
  • S. Ascenzi, Istituto Nazionale di Fisica Nucleare - INFN
  • Tiffany Z. Summerscales, Andrews University
Document Type
Article
Publication Date
12-1-2016
Keywords
  • gravitational waves,
  • stars: black holes
Abstract

© 2016. The American Astronomical Society. All rights reserved.. This article provides supplemental information for a Letter reporting the rate of (BBH) coalescences inferred from 16 days of coincident Advanced LIGO observations surrounding the transient (GW) signal GW150914. In that work we reported various rate estimates whose 90% confidence intervals fell in the range 2-600 Gpc-3yr-1. Here we give details on our method and computations, including information about our search pipelines, a derivation of our likelihood function for the analysis, a description of the astrophysical search trigger distribution expected from merging BBHs, details on our computational methods, a description of the effects and our model for calibration uncertainty, and an analytic method for estimating our detector sensitivity, which is calibrated to our measurements.

DOI
https://doi.org/10.3847/0067-0049/227/2/14
First Department
Physics
Acknowledgements
Retrieved January 28, 2021 from https://iopscience.iop.org/article/10.3847/0067-0049/227/2/14/pdf
Citation Information
B. P. Abbott, R. Abbott, T. D. Abbott, M. R. Abernathy, et al.. "Supplement: The Rate Of Binary Black Hole Mergers Inferred From Advanced Ligo Observations Surrounding Gw150914" Astrophysical Journal, Supplement Series Vol. 227 Iss. 2 (2016)
Available at: http://works.bepress.com/tiffany_summerscales/212/