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

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autorschaft

  • The LIGO Scientific Collaboration
  • Virgo Collaboration
  • Karsten Danzmann
  • Michele Heurs
  • Fumiko Kawazoe
  • Harald Lück
  • Daniel Steinmeyer
  • Henning Fedor Cornelius Vahlbruch
  • Benno Willke
  • Holger Wittel
  • Bruce Allen
  • A. Bisht
  • Timo Denker
  • Stefan Kaufer
  • Christian Krüger
  • J. D. Lough
  • A. Sawadsky

Externe Organisationen

  • California Institute of Technology (Caltech)
  • Louisiana State University
  • Universita di Salerno
  • Università degli Studi di Napoli Federico II
  • University of Florida
  • University of Mississippi
  • Universite de Savoie
  • Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
  • Nationaal instituut voor subatomaire fysica (Nikhef)
  • LIGO Laboratory
  • Instituto Nacional de Pesquisas Espaciais
  • Istituto Nazionale di Fisica Nucleare (INFN)
  • Inter-University Centre for Astronomy and Astrophysics India
  • Washington State University Pullman
  • Syracuse University
  • University of Birmingham
  • University of Glasgow
  • Hanyang University
  • Carleton College
  • Australian National University
  • University of Melbourne
  • Tsinghua University
  • University of Western Australia
  • Observatoire de la Côte d’Azur (OCA)
  • Rochester Institute of Technology
  • Northwestern University
  • University of Wisconsin Milwaukee
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer134001
FachzeitschriftClassical and quantum gravity
Jahrgang33
Ausgabenummer13
PublikationsstatusVeröffentlicht - 6 Juni 2016

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.

ASJC Scopus Sachgebiete

Zitieren

Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914. / The LIGO Scientific Collaboration; Virgo Collaboration; Danzmann, Karsten et al.
in: Classical and quantum gravity, Jahrgang 33, Nr. 13, 134001, 06.06.2016.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

The LIGO Scientific Collaboration, Virgo Collaboration, Danzmann, K, Heurs, M, Kawazoe, F, Lück, H, Steinmeyer, D, Vahlbruch, HFC, Willke, B, Wittel, H, Allen, B, Bisht, A, Denker, T, Kaufer, S, Krüger, C, Lough, JD & Sawadsky, A 2016, 'Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914', Classical and quantum gravity, Jg. 33, Nr. 13, 134001. https://doi.org/10.1088/0264-9381/33/13/134001, https://doi.org/10.15488/2383
The LIGO Scientific Collaboration, Virgo Collaboration, Danzmann, K., Heurs, M., Kawazoe, F., Lück, H., Steinmeyer, D., Vahlbruch, H. F. C., Willke, B., Wittel, H., Allen, B., Bisht, A., Denker, T., Kaufer, S., Krüger, C., Lough, J. D., & Sawadsky, A. (2016). Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914. Classical and quantum gravity, 33(13), Artikel 134001. https://doi.org/10.1088/0264-9381/33/13/134001, https://doi.org/10.15488/2383
The LIGO Scientific Collaboration, Virgo Collaboration, Danzmann K, Heurs M, Kawazoe F, Lück H et al. Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914. Classical and quantum gravity. 2016 Jun 6;33(13):134001. doi: 10.1088/0264-9381/33/13/134001, 10.15488/2383
The LIGO Scientific Collaboration ; Virgo Collaboration ; Danzmann, Karsten et al. / Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914. in: Classical and quantum gravity. 2016 ; Jahrgang 33, Nr. 13.
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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.",
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TY - JOUR

T1 - Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914

AU - The LIGO Scientific Collaboration

AU - The Virgo Collaboration

AU - Abbott, B. P.

AU - Abbott, R.

AU - Abbott, T. D.

AU - Abernathy, M. R.

AU - Acernese, F.

AU - Ackley, K.

AU - Adamo, M.

AU - Adams, C.

AU - Adams, T.

AU - Addesso, P.

AU - Adhikari, R. X.

AU - Adya, V. B.

AU - Affeldt, C.

AU - Agathos, M.

AU - Agatsuma, K.

AU - Aggarwal, N.

AU - Aguiar, O. D.

AU - Aiello, L.

AU - Ain, A.

AU - Bose, S.

AU - Brown, D. A.

AU - Chen, Y.

AU - Danilishin, S. L.

AU - Danzmann, Karsten

AU - Fricke, T. T.

AU - Hanke, M. M.

AU - Hennig, J.

AU - Heurs, Michele

AU - Kawazoe, Fumiko

AU - Lee, H. K.

AU - Lück, Harald

AU - Luo, J.

AU - Nguyen, T. T.

AU - Schmidt, J.

AU - Schmidt, P.

AU - Shaltev, M.

AU - Steinmeyer, Daniel

AU - Sun, L.

AU - Vahlbruch, Henning Fedor Cornelius

AU - Wang, M.

AU - Wang, X.

AU - Wang, Y.

AU - Wei, L. W.

AU - Willke, Benno

AU - Wittel, Holger

AU - Zhang, L.

AU - Zhang, Y.

AU - Zhou, M.

AU - Allen, Bruce

AU - Bisht, A.

AU - Denker, Timo

AU - Kaufer, Stefan

AU - Krüger, Christian

AU - Lough, J. D.

AU - Sawadsky, A.

PY - 2016/6/6

Y1 - 2016/6/6

N2 - 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.

AB - 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.

KW - detector characterization

KW - gravitational waves

KW - GW150914

UR - http://www.scopus.com/inward/record.url?scp=84976413609&partnerID=8YFLogxK

U2 - 10.1088/0264-9381/33/13/134001

DO - 10.1088/0264-9381/33/13/134001

M3 - Article

AN - SCOPUS:84976413609

VL - 33

JO - Classical and quantum gravity

JF - Classical and quantum gravity

SN - 0264-9381

IS - 13

M1 - 134001

ER -

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