Gravitational waves from Scorpius X-1: A comparison of search methods and prospects for detection with advanced detectors
C Messenger, HJ Bulten, SG Crowder, V Dergachev, DK Galloway, E Goetz, RJG Jonker, PD Lasky, GD Meadors, A Melatos, S Premachandra, K Riles, L Sammut, EH Thrane, JT Whelan, Y Zhang
Physical Review D | AMER PHYSICAL SOC | Published : 2015
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Awarded by NSF
Awarded by Australian Research Council (ARC) Discovery Project
Awarded by Science and Technology Facilities Council
The authors are grateful to Badri Krishnan, Paola Leaci, and Reinhard Prix for useful discussions and comments. Y. Z. acknowledges the hospitality of the Max Planck Institute for Gravitational Physics (Albert Einstein Institute) in Hannover, Germany. S. G. C. was supported by NSF Grant No. PHY-1204944. J. T. W. was supported by NSF Grants No. PHY-0855494 and No. PHY-1207010. Y. Z. was supported by NSF Grant No. PHY-1207010. K. R., E. G., and G. D. M. were supported by NSF Grants No. PHY-0855422 and No. PHY-1205173. E. G. and G. D. M. have also been supported by the Max Planck Institute for Gravitational Physics (Albert Einstein Institute) in Hannover, Germany. G. D. M. conducted some analyses on the LIGO Data Grid clusters at the California Institute of Technology and LIGO Hanford Observatory. P. D. L. and A. M. were supported by Australian Research Council (ARC) Discovery Project DP110103347. P. D. L. is also supported by ARC DP140102578. H. J. B. and R. J. are supported by the research programme of the Foundation for Fundamental Research on Matter (FOM), which is part of the Netherlands Organisation for Scientific Research (NWO). C. M. is supported by a Glasgow University Lord Kelvin Adam Smith Fellowship and the Science and Technology Facilities Council (Grant No. ST/L000946/1). The analysis for several of the searches in this project were performed on the Atlas computing cluster at AEI Hannover, which was funded by the Max Planck Society and the State of Niedersachsen, Germany. This paper has been assigned LIGO Document Number LIGO-P1400217-x3.