2016/02/11 by The LIGO Scientific Collaboration, the Virgo Collaboration · 1 voice
Physics and Astronomy · #astro-ph.HE #astro-ph.IM #gr-qc #physics.ins-det
paper · pdf · doi:10.1088/0264-9381/33/13/134001
arxiv published 2016/02/11 · arxiv created 2016/06/04 · arxiv updated 2016/06/04
On September 14, 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.