Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
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 investigati...
Similar Items
-
ASTROPHYSICAL IMPLICATIONS OF THE BINARY BLACK HOLE MERGER GW150914
by: LIGO Scientific Collaboration, et al.
Published: (2016) -
Effects of waveform model systematics on the interpretation of GW150914
by: Aggarwal, Nancy, et al.
Published: (2019) -
LOCALIZATION AND BROADBAND FOLLOW-UP OF THE GRAVITATIONAL-WAVE TRANSIENT GW150914
by: Aggarwal, Nancy, et al.
Published: (2018) -
THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914
by: LIGO Collaboration, et al.
Published: (2018) -
The basic physics of the binary black hole merger GW150914
by: Aggarwal, Nancy, et al.
Published: (2019)