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NTIS 바로가기Physical review letters, v.125 no.10, 2020년, pp.101102 -
Abbott, R. (California Institute of Technology) , Abbott, T. D. (Louisiana State University) , Abraham, S. (Inter-University Centre for Astronomy and Astrophysics) , Acernese, F. (Università) , Ackley, K. (di Salerno) , Adams, C. (Monash University) , Adhikari, R. X. (LIGO Livingston Observatory) , Adya, V. B. (California Institute of Technology) , Affeldt, C. (Australian National University) , Agathos, M. (Max Planck Institute for Gravitational Physics (Albert Einstein Institute)) , Agatsuma, K. (Friedrich-Schiller-Universitä) , Aggarwal, N. (t Jena) , Aguiar, O. D. (University of Birmingham) , Aich, A. (Northwestern University) , Aiello, L. (Instituto Nacional de Pesquisas Espaciais) , Ain, A. (The University of Texas Rio Grande Valley) , Ajith, P. (Gran Sasso Science Institute (GSSI)) , Akcay, S. (Inter-University Centre for Astronomy and Astrophysics) , Allen, G. (Tata Institute of Fundamental Research) , Allocca, A. (Friedrich-Schiller-Universitä) , Altin, P. A. (t Jena) , Amato, A. (University of Illinois at Urbana-Champaign) , Anand, S. (INFN) , Ananyeva, A. (Australian National University) , Anderson, S. B. (Université) , Anderson, W. G. (de Lyon) , Angelova, S. V. (California Institute of Technology) , Ansoldi, S. (California Institute of Technology) , Antier, S. (California Institute of Technology) , Appert, S. (University of Wisconsin-Milwaukee) , Arai, K. (University of Strathclyde) , Araya, M. C. , Areeda, J. S. , Arène, M. , Arnaud, N. , Aronson, S. M. , Arun, K. G. , Asali, Y. , Ascenzi, S. , Ashton, G. , Aston, S. M. , Astone, P. , Aubin, F. , Aufmuth, P. , AultONeal, K. , Austin, C. , Avendano, V. , Babak, S. , Bacon, P. , Badaracco, F. , Bader, M. K. M. , Bae, S. , Baer, A. M. , Baird, J. , Baldaccini, F. , Ballardin, G. , Ballmer, S. W. , Bals, A. , Balsamo, A. , Baltus, G. , Banagiri, S. , Bankar, D. , Bankar, R. S. , Barayoga, J. C. , Barbieri, C. , Barish, B. C. , Barker, D. , Barkett, K. , Barneo, P. , Barone, F. , Barr, B.
On May 21, 2019 at 03:02:29 UTC Advanced LIGO and Advanced Virgo observed a short duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise ratio of 14.7, and an estimated false-alarm rate of 1 in 4900 yr using a search sensitive to generic transients. If GW190521 i...
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