Authors

B. P. Abbott, California Institute of TechnologyFollow
R. Abbott, California Institute of TechnologyFollow
T. D. Abbott, Louisiana State UniversityFollow
M. R. Abernathy, American UniversityFollow
F. Acernese, Università degli Studi di SalernoFollow
K. Ackley, University of FloridaFollow
C. Adams, LIGO LivingstonFollow
T. Adams, Université Savoie Mont BlancFollow
P. Addesso, Università degli Studi del SannioFollow
R. X. Adhikari, California Institute of TechnologyFollow
V. B. Adya, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)Follow
C. Affeldt, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)Follow
M. Agathos, FOM-Institute of Subatomic Physics - NIKHEFFollow
K. Agatsuma, FOM-Institute of Subatomic Physics - NIKHEFFollow
N. Aggarwal, LIGO, Massachusetts Institute of TechnologyFollow
O. D. Aguiar, Instituto Nacional de Pesquisas EspaciaisFollow
L. Aiello, Istituto Nazionale di Fisica Nucleare - INFNFollow
A. Ain, Inter-University Centre for Astronomy and Astrophysics IndiaFollow
P. Ajith, Tata Institute of Fundamental Research, MumbaiFollow
B. Allen, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)Follow
A. Allocca, Università di PisaFollow
P. A. Altin, The Australian National UniversityFollow
A. Ananyeva, California Institute of TechnologyFollow
S. B. Anderson, California Institute of TechnologyFollow
W. G. Anderson, University of Wisconsin-MilwaukeeFollow
S. Appert, California Institute of Technology
K. Arai, California Institute of Technology
M. C. Araya, California Institute of Technology
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
G. Ashton, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)

Document Type

Article

Publication Date

12-10-2017

Abstract

There is an error in Equation?(4) of the original paper, which should instead be (Formula Presented) This makes it consistent with Equation?(3) of Aasi et al. (2014), which was actually used when calculating the value of the Q22 upper limits from the h0 upper limits for the results of this paper.

Publication Source (Journal or Book title)

Astrophysical Journal

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