Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model

Research output: Contribution to journalArticleResearchpeer review

Authors

  • The LIGO Scientific Collaboration
  • The Virgo Collaboration
  • Shtefan Danilishin
  • Karsten Danzmann
  • Michele Heurs
  • Harald Lück
  • Daniel Steinmeyer
  • Henning Fedor Cornelius Vahlbruch
  • Li-Wei Wei
  • Holger Wittel
  • Peter Aufmuth
  • Stefan Kaufer
  • Aparna Bisht
  • Nina Bode
  • James Lough
  • Dirk Schütte
  • A. Sawadsky
  • D. S. Wu
  • Maximilian H. Wimmer
  • W. Winkler
  • J. Woehler

External Research Organisations

  • California Institute of Caltech (Caltech)
  • Louisiana State University
  • Universita di Salerno
  • Monte S. Angelo University Federico II
  • University of Florida
  • Universite de Savoie
  • University of Sannio
  • Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • University of Mississippi
  • University of Illinois at Urbana-Champaign
  • National Institute for Subatomic Physics (Nikhef)
  • LIGO Laboratory
  • Instituto Nacional de Pesquisas Espaciais
  • Gran Sasso Science Institute
  • Istituto Nazionale di Fisica Nucleare (INFN)
  • Inter-University Centre for Astronomy and Astrophysics India
  • Tata Institute of Fundamental Research (TIFR HYD)
  • Carson College of Business
  • University of Birmingham
  • University of Glasgow
  • Inje University
  • Australian National University
  • Embry Riddle Aeronautical University
  • Radboud University Nijmegen (RU)
  • University of Melbourne
  • University of Western Australia
  • Rochester Institute of Technology
  • Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA)
  • Northwestern University
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Details

Original languageEnglish
Article number122003
Number of pages20
JournalPhysical Review D
Volume95
Issue number12
Publication statusPublished - 27 Jun 2017

ASJC Scopus subject areas

Cite this

Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model. / The LIGO Scientific Collaboration; The Virgo Collaboration; Danilishin, Shtefan et al.
In: Physical Review D, Vol. 95, No. 12, 122003, 27.06.2017.

Research output: Contribution to journalArticleResearchpeer review

The LIGO Scientific Collaboration, The Virgo Collaboration, Danilishin, S, Danzmann, K, Heurs, M, Lück, H, Steinmeyer, D, Vahlbruch, HFC, Wei, L-W, Wittel, H, Aufmuth, P, Kaufer, S, Bisht, A, Bode, N, Lough, J, Schütte, D, Sawadsky, A, Wu, DS, Wimmer, MH, Winkler, W & Woehler, J 2017, 'Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model', Physical Review D, vol. 95, no. 12, 122003. https://doi.org/10.1103/PhysRevD.95.122003, https://doi.org/10.15488/12008
The LIGO Scientific Collaboration, The Virgo Collaboration, Danilishin, S., Danzmann, K., Heurs, M., Lück, H., Steinmeyer, D., Vahlbruch, H. F. C., Wei, L.-W., Wittel, H., Aufmuth, P., Kaufer, S., Bisht, A., Bode, N., Lough, J., Schütte, D., Sawadsky, A., Wu, D. S., Wimmer, M. H., ... Woehler, J. (2017). Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model. Physical Review D, 95(12), Article 122003. https://doi.org/10.1103/PhysRevD.95.122003, https://doi.org/10.15488/12008
The LIGO Scientific Collaboration, The Virgo Collaboration, Danilishin S, Danzmann K, Heurs M, Lück H et al. Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model. Physical Review D. 2017 Jun 27;95(12):122003. doi: 10.1103/PhysRevD.95.122003, 10.15488/12008
The LIGO Scientific Collaboration ; The Virgo Collaboration ; Danilishin, Shtefan et al. / Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model. In: Physical Review D. 2017 ; Vol. 95, No. 12.
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@article{df07851ab90a4faf8a7384cb7d161ce6,
title = "Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model",
author = "{The LIGO Scientific Collaboration} and {The Virgo Collaboration} and Abbott, {B. P.} and R. Abbott and Abbott, {T. D.} and F. Acernese and K. Ackley and C. Adams and T. Adams and P. Addesso and Adhikari, {R. X.} and Adya, {V. B.} and C. Affeldt and M. Afrough and B. Agarwal and K. Agatsuma and N. Aggarwal and Aguiar, {O. D.} and L. Aiello and A. Ain and P. Ajith and S. Bose and Brown, {D. A.} and Y. Chen and Cheng, {H. P.} and Shtefan Danilishin and Karsten Danzmann and Hanke, {M. M.} and J. Hennig and Michele Heurs and S. Kumar and Lee, {H. W.} and Harald L{\"u}ck and Nguyen, {T. T.} and E. Schmidt and J. Schmidt and P. Schmidt and Daniel Steinmeyer and L. Sun and Vahlbruch, {Henning Fedor Cornelius} and M. Wang and Y. Wang and Li-Wei Wei and Benno Willke and Holger Wittel and L. Zhang and Zhang, {Y. H.} and M. Zhou and Peter Aufmuth and Stefan Kaufer and Aparna Bisht and Nina Bode and James Lough and Dirk Sch{\"u}tte and A. Sawadsky and Wu, {D. S.} and Wimmer, {Maximilian H.} and W. Winkler and J. Woehler",
note = "Funding information: The authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organization for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Economia y Competitividad, the Vicepresidncia i Conselleria d Innovacion, Recerca i Turisme and the Conselleria d Educacion i Universitat del Govern de les Illes Balears, the National Science Centre of Poland, the European Commission, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, and Innovation, International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), Russian Foundation for Basic Research, the Leverhulme Trust, the Research Corporation, Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS and the State of Niedersachsen/Germany for provision of computational resources. This is LIGO document LIGO-P1700019.",
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month = jun,
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Download

TY - JOUR

T1 - Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model

AU - The LIGO Scientific Collaboration

AU - The Virgo Collaboration

AU - Abbott, B. P.

AU - Abbott, R.

AU - Abbott, T. D.

AU - Acernese, F.

AU - Ackley, K.

AU - Adams, C.

AU - Adams, T.

AU - Addesso, P.

AU - Adhikari, R. X.

AU - Adya, V. B.

AU - Affeldt, C.

AU - Afrough, M.

AU - Agarwal, B.

AU - Agatsuma, K.

AU - Aggarwal, N.

AU - Aguiar, O. D.

AU - Aiello, L.

AU - Ain, A.

AU - Ajith, P.

AU - Bose, S.

AU - Brown, D. A.

AU - Chen, Y.

AU - Cheng, H. P.

AU - Danilishin, Shtefan

AU - Danzmann, Karsten

AU - Hanke, M. M.

AU - Hennig, J.

AU - Heurs, Michele

AU - Kumar, S.

AU - Lee, H. W.

AU - Lück, Harald

AU - Nguyen, T. T.

AU - Schmidt, E.

AU - Schmidt, J.

AU - Schmidt, P.

AU - Steinmeyer, Daniel

AU - Sun, L.

AU - Vahlbruch, Henning Fedor Cornelius

AU - Wang, M.

AU - Wang, Y.

AU - Wei, Li-Wei

AU - Willke, Benno

AU - Wittel, Holger

AU - Zhang, L.

AU - Zhang, Y. H.

AU - Zhou, M.

AU - Aufmuth, Peter

AU - Kaufer, Stefan

AU - Bisht, Aparna

AU - Bode, Nina

AU - Lough, James

AU - Schütte, Dirk

AU - Sawadsky, A.

AU - Wu, D. S.

AU - Wimmer, Maximilian H.

AU - Winkler, W.

AU - Woehler, J.

N1 - Funding information: The authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organization for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Economia y Competitividad, the Vicepresidncia i Conselleria d Innovacion, Recerca i Turisme and the Conselleria d Educacion i Universitat del Govern de les Illes Balears, the National Science Centre of Poland, the European Commission, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, and Innovation, International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), Russian Foundation for Basic Research, the Leverhulme Trust, the Research Corporation, Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS and the State of Niedersachsen/Germany for provision of computational resources. This is LIGO document LIGO-P1700019.

PY - 2017/6/27

Y1 - 2017/6/27

UR - http://www.scopus.com/inward/record.url?scp=85022327286&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.95.122003

DO - 10.1103/PhysRevD.95.122003

M3 - Article

AN - SCOPUS:85022327286

VL - 95

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 12

M1 - 122003

ER -

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