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Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network

Chow, Jong; Chua, Sheon; Inta, Ra; Lam, Ping Koy; McClelland, David; Miller, John; Mow-Lowry, C; Mullavey, Adam; Nguyen, Thanh; Scott, Susan M; Smith-Lefebvre, Nicolas; Strigin, S; Torrie, Calum; Summerscales, T.Z.; Susmithan, S; Talukder, D; Vass, S; Veitch, Peter John; Waldman, Sam J; Wallace, L; Allen, B; Wang, Xiaofeng; Wen, L; Whitcomb, Stanley Ernest; Whiting, B F; Zhang, L; Ottaway, D J; Stefszky, Michael; Wade, Andrew; Abadie, J; Abbott, B; Shaddock, Daniel; Abbott, Robert; Adams, C; Adhikari, Rana; Aasi, J; Acernese, F; Barone, F; Basti, A; Beker, M G; Blom, M; Bulten, H.J.; Barker, D; Evans, M; Factourovich, M; Genin, E; Kawabe, Keita; Landry, M; Mandic, V.; Meadors, G.D.; Schofield, R; Vinet, J-Y; Vorvick, C; Anderson, S B; Arai, Koji; Araya, M; Barsotti, L; Bartos, I; Beyersdorf, P T; Bilenko, I A; Billingsley, G; Slagmolen, Bram; Blackburn, James Kent; Blair, David Gerald; Bork, R; Bose, S; Owen, Benjamin; Braginsky, V; Brau, J E; Byer, Robert L; Camp, J; Cao, J; Corbitt, T; Charlton, Philip; Chung, C. T.Y.; Cook, D; Coward, D; Dhurandhar, S; Coyne, D; Creighton, J D E; DeBra, D; Dumas, J-C; Dwyer, Sheila; Ehrens, P; Etzel, T; Heefner, J; Fairhurst, S; Finn, Lee; Frey, R; Fritschel, Peter; Frolov, V; Kells, W; Fyffe, M; Giaime, J; Gray, C; Greenhalgh, R. J. S.; Heptonstall, A; Gustafson, R; Hammer, D; Hanson, J; Hewitson, M; King, P; Howell, E; Kalogera, V; Katsavounidis, E; Kissel, Jeffrey S; Kozak, D; Lantz, B; Melatos, Andrew; Lazzarini, A; Leonor, I; Lindquist, P; Lockerbie, N.A.; Lormand, M; Pedraza, M; Lubinski, M; MacInnis, M; Mageswaran, M; Mailand, K; Maros, E; Marx, Jay; Mavalvala, Nergis; Melissinos, A; Mendell, G; Meshkov, S; Mitrofanov, V P; Mittleman, R; Penn, S; Reed, C M; Riles, K; Sammut, L; Sathyaprakash, B; Saulson, P; Schwinberg, P; Shapiro, Brett; Shoemaker, D; Siemens, X; Sigg, D; Sintes, A

Description

Compact binary systems with neutron stars or black holes are one of the most promising sources for ground-based gravitational-wave detectors. Gravitational radiation encodes rich information about source physics; thus parameter estimation and model select

CollectionsANU Research Publications
Date published: 2013
Type: Journal article
URI: http://hdl.handle.net/1885/77780
Source: Physical Review D-Particles, Fields, Gravitation and Cosmology
DOI: 10.1103/PhysRevD.88.062001

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