Search strategies for long gravitational-wave transients: Hidden Markov model tracking and seedless clustering
Sharan Banagiri, Ling Sun, Michael W Coughlin, Andrew Melatos
Physical Review D | AMER PHYSICAL SOC | Published : 2019
Awarded by NSF
Awarded by National Science Foundation
Awarded by Australian Research Council (ARC)
Awarded by ARC Centre of Excellence for Gravitational Wave Discovery
We are grateful to Maxime Fays, Rich Ormiston, Stuart Anderson and Vuk Mandic for comments and informative discussions. S. B. acknowledges support in part by the Hoff Lu Fellowship at the university of Minnesota, and by NSF Grant No. PHY-1806630. L. S. is a member of the LIGO Laboratory. M. W. C. is supported by the David and Ellen Lee Postdoctoral Fellowship at the California Institute of Technology. The authors are thankful for the computing resources provided by LIGO Laboratory. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation, and operates under cooperative agreement No. PHY-0757058. Advanced LIGO was built under Grant No. PHY-0823459. The research was also supported by Australian Research Council (ARC) Discovery Project DP170103625 and the ARC Centre of Excellence for Gravitational Wave Discovery CE170100004. This paper carries LIGO Document Number LIGO-P1900047.