Characterization of Transient Noise In Advanced LIGO Relevant to Gravitational Wave Signal GW150914
Document Type
Article
Publication Date
6-6-2016
Journal / Book Title
Classical and Quantum Gravity
Abstract
On 14 September 2015, a gravitational wave signal from a coalescing black hole binary system was observed by the Advanced LIGO detectors. This paper describes the transient noise backgrounds used to determine the significance of the event (designated GW150914) and presents the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around the time of the event. The detectors were operating nominally at the time of GW150914. We have ruled out environmental influences and non-Gaussian instrument noise at either LIGO detector as the cause of the observed gravitational wave signal.
DOI
10.1088/0264-9381/33/13/134001
MSU Digital Commons Citation
The LIGO Scientific Collaboration; The Virgo Collaboration; Favata, Marc; Ghosh, Shaon; and Martin, Rodica, "Characterization of Transient Noise In Advanced LIGO Relevant to Gravitational Wave Signal GW150914" (2016). Department of Physics and Astronomy Faculty Scholarship and Creative Works. 25.
https://digitalcommons.montclair.edu/physics-astron-facpubs/25
Published Citation
Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., ... & Baiardi, L. C. (2016). Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914. Classical and Quantum Gravity, 33(13), 134001.
Comments
This article is a collaboration between the LIGO Scientific Collaboration and the Virgo Collaboration. Additional authors may be found on the publication.
This is an Open Access article under a Creative Commons Attribution International License.