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NTIS 바로가기Classical and quantum gravity, v.34 no.10, 2017년, pp.104002 -
Abbott, B P (LIGO, California Institute of Technology, Pasadena, CA 91125, United States of America) , Abbott, R (LIGO, California Institute of Technology, Pasadena, CA 91125, United States of America) , Abbott, T D (Louisiana State University, Baton Rouge, LA 70803, United States of America) , Abernathy, M R (American University, Washington, DC 20016, United States of America) , Acernese, F (Università) , Ackley, K (di Salerno, Fisciano, I-84084 Salerno, Italy) , Adams, C (University of Florida, Gainesville, FL 32611, United States of America) , Adams, T (LIGO Livingston Observatory, Livingston, LA 70754, United States of America) , Addesso, P (Laboratoire d’Annecy-le-Vieux de Physique des Particules (LAPP), Université) , Adhikari, R X (Savoie Mont Blanc, CNRS) , Adya, V B (University of Sannio at Benevento, I-82100 Benevento, Italy) , Affeldt, C (LIGO, California Institute of Technology, Pasadena, CA 91125, United States of America) , Agathos, M (Albert-Einstein-Institut, Max-Planck-Institut fü) , Agatsuma, K (r Gravitationsphysik, D-30167 Hannover, Germany) , Aggarwal, N (Albert-Einstein-Institut, Max-Planck-Institut fü) , Aguiar, O D (r) , Aiello, L , Ain, A , Ajith, P , Allen, B , Allocca, A , Altin, P A , Ananyeva, A , Anderson, S B , Anderson, W G , Appert, S , Arai, K , Araya, M C , Areeda, J S , Arnaud, N , Arun, K G , Ascenzi, S , Ashton, G , Ast, M , Aston, S M , Astone, P , Aufmuth, P , Aulbert, C , Avila-Alvarez, A , Babak, S , Bacon, P , Bader, M K M , Baker, P T , Baldaccini, F , Ballardin, G , Ballmer, S W , Barayoga, J C , Barclay, S E , Barish, B C , Barker, D , Barone, F , Barr, B , Barsotti, L , Barsuglia, M , Barta, D , Bartlett, J , Bartos, I , Bassiri, R , Basti, A , Batch, J C , Baune, C , Bavigadda, V , Bazzan, M , Beer, C , Bejger, M , Belahcene, I , Belgin, M , Bell, A S , Berger, B K , Bergmann, G , Berry, C P L , Bersanetti, D , Bertolini, A , Betzwieser, J , Bhagwat, S , Bhandare, R
Parameter estimates of GW150914 were obtained using Bayesian inference, based on three semi-analytic waveform models for binary black hole coalescences. These waveform models differ from each other in their treatment of black hole spins, and all three models make some simplifying assumptions, notabl...
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