Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914

Document #:

LIGO-P1500238-v24

Document type:

P - Publications

Abstract:

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.

Files in Document:

• P1500238_GW150914_noise_characterization.pdf (file is not accessible)

Other Files:

• P1500238.tar.gz (file is not accessible)

Topics:

• Detector Characterization

Author Groups:

• LVC

Keywords:

GW150914

Referenced by:

• LIGO-L1500138-v6: LLO, LHO site status for GW150914
• LIGO-T1600011-v3: Data Quality Vetoes Applied to the Analysis of GW150914
• LIGO-T1600030-v2: LIGO-P1500238 figure images and data
• LIGO-P150914-v14: Observation of Gravitational Waves from a Binary Black Hole Merger

Publication Information:

Preprint posted on the arXiv: http://arxiv.org/abs/1602.03844
Open access publication in CQG: http://iopscience.iop.org/article/10.1088/0264-9381/33/13/134001