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 -