Calibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914
Altin, Paul; Chow, Jong; Mansell, Georgia; McClelland, David; McManus, David; Nguyen, Thanh; Rabeling, David; Scott, Susan M; Shaddock, Daniel; Abbott, B; Abbott, Robert; Abbott, T; Ackley, K; Adhikari, Rana; Barish, Barry; Barsotti, L; Berger, B K; Bilenko, I A; Billingsley, G; Blackburn, James Kent; Blair, David Gerald; Bork, R; Braginsky, V; Cannon, Kipp; Coward, D; Dhurandhar, S; Ehrens, P; Etzel, T; Fairhurst, S; Favata, Marc; Frei, Z; Fritschel, Peter; Gehrels, N; Giaime, J; Heptonstall, A; Howell, E; Huttner, S.H.; Kells, W; Korth, W. Zach; Kozak, D; Lasky, P. D.; Lazzarini, A; Lockerbie, N.A.; Mageswaran, M; Maros, E; Martynov, D; Matichard, F; Mavalvala, Nergis; Melatos, Andrew; Mendell, G; Meshkov, S; Oelker, E; Ottaway, D J; Pedraza, M; Penn, S; Reed, C M; Reitze, D; Sammut, L; Saulson, P; Sigg, D; Sintes, A; Souradeep, T; Strain, Ken A; Strigin, S; Summerscales, T.Z.; Slagmolen, Bram; Wade, Andrew; Ward, Robert; Qin, Jiayi; Yap, Min Jet
In Advanced LIGO, detection and astrophysical source parameter estimation of the binary black hole merger GW150914 requires a calibrated estimate of the gravitational-wave strain sensed by the detectors. Producing an estimate from each detector’s differential arm length control loop readout signals requires applying time domain filters, which are designed from a frequency domain model of the detector’s gravitational-wave response. The gravitational-wave response model is determined by the...[Show more]
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|Source:||Physical Review D|
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