Authors

M. Constancio, Instituto Nacional de Pesquisas Espaciais
J. Aasi, California Institute of TechnologyFollow
J. Abadie, California Institute of TechnologyFollow
B. P. Abbott, California Institute of TechnologyFollow
R. Abbott, California Institute of TechnologyFollow
T. Abbott, Louisiana State UniversityFollow
M. R. Abernathy, California Institute of TechnologyFollow
T. Accadia, Université Savoie Mont BlancFollow
F. Acernese, Istituto Nazionale di Fisica Nucleare, Sezione di NapoliFollow
C. Adams, LIGO LivingstonFollow
T. Adams, Cardiff UniversityFollow
R. X. Adhikari, California Institute of TechnologyFollow
C. Affeldt, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)Follow
M. Agathos, FOM-Institute of Subatomic Physics - NIKHEFFollow
N. Aggarwal, Massachusetts Institute of TechnologyFollow
O. D. Aguiar, Instituto Nacional de Pesquisas EspaciaisFollow
P. Ajith, California Institute of TechnologyFollow
B. Allen, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)Follow
A. Allocca, Istituto Nazionale di Fisica Nucleare, Sezione di PisaFollow
E. Amador Ceron, University of Wisconsin-MilwaukeeFollow
D. Amariutei, University of FloridaFollow
R. A. Anderson, California Institute of TechnologyFollow
S. B. Anderson, California Institute of TechnologyFollow
W. G. Anderson, University of Wisconsin-MilwaukeeFollow
K. Arai, California Institute of Technology
M. C. Araya, California Institute of Technology
C. Arceneaux, University of Mississippi
J. Areeda, California State University, Fullerton
S. Ast, Gottfried Wilhelm Leibniz Universität Hannover
S. M. Aston, LIGO Livingston
P. Astone, Istituto Nazionale di Fisica Nucleare - INFN
P. Aufmuth, Gottfried Wilhelm Leibniz Universität Hannover
C. Aulbert, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)

Document Type

Article

Publication Date

1-1-2014

Abstract

During the Laser Interferometer Gravitational-wave Observatory and Virgo joint science runs in 2009-2010, gravitational wave (GW) data from three interferometer detectors were analyzed within minutes to select GW candidate events and infer their apparent sky positions. Target coordinates were transmitted to several telescopes for follow-up observations aimed at the detection of an associated optical transient. Images were obtained for eight such GW candidates. We present the methods used to analyze the image data as well as the transient search results. No optical transient was identified with a convincing association with any of these candidates, and none of the GW triggers showed strong evidence for being astrophysical in nature. We compare the sensitivities of these observations to several model light curves from possible sources of interest, and discuss prospects for future joint GW-optical observations of this type. © 2014. The American Astronomical Society. All rights reserved.

Publication Source (Journal or Book title)

Astrophysical Journal, Supplement Series

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