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|a dc
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|a Martynov, D. V.
|e author
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|a Massachusetts Institute of Technology. Department of Physics
|e contributor
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|a LIGO
|q (Observatory : Massachusetts Institute of Technology)
|e contributor
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|a MIT Kavli Institute for Astrophysics and Space Research
|e contributor
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|a Barsotti, Lisa
|e contributor
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|a Biscans, Sebastien
|e contributor
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|a Evans, Matthew J
|e contributor
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1 |
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|a Foley, Stephany
|e contributor
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|a Fritschel, Peter K
|e contributor
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1 |
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|a Gras, Slawomir
|e contributor
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1 |
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|a Kwee, Patrick
|e contributor
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1 |
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|a MacInnis, Myron E
|e contributor
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1 |
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|a Mason, Kenneth R
|e contributor
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1 |
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|a Matichard, Fabrice
|e contributor
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|a Mavalvala, Nergis
|e contributor
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|a Miller, John
|e contributor
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|a Mittleman, Richard K
|e contributor
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|a Shoemaker, David H
|e contributor
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|a Stein, Andrew J
|e contributor
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|a Waldman, Samuel J.
|e contributor
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|a Weiss, Rainer
|e contributor
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|a Yu, Hang
|e contributor
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|a Zucker, Michael E
|e contributor
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|a Hall, E. D.
|e author
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|a Abbott, B. P.
|e author
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|a Abbott, R.
|e author
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|a Abbott, T. D.
|e author
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|a Adams, C.
|e author
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|a Adhikari, R. X.
|e author
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|a Anderson, R. A.
|e author
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|a Anderson, S. B.
|e author
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|a Arai, K.
|e author
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|a Arain, M. A.
|e author
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|a Aston, S. M.
|e author
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|a Austin, L.
|e author
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|a Ballmer, S. W.
|e author
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|a Barbet, M.
|e author
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|a Barker, D.
|e author
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|a Barr, B.
|e author
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|a Bartlett, J.
|e author
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|a Barton, M. A.
|e author
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|a Bartos, I.
|e author
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|a Batch, J. C.
|e author
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|a Bell, A. S.
|e author
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|a Belopolski, I.
|e author
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|a Bergman, J.
|e author
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|a Betzwieser, J.
|e author
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|a Billingsley, G.
|e author
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|a Birch, J.
|e author
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|a Biwer, C.
|e author
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|a Black, E.
|e author
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|a Blair, C. D.
|e author
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|a Bogan, C.
|e author
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|a Bork, R.
|e author
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|a Bridges, D. O.
|e author
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|a Brooks, A. F.
|e author
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|a Celerier, C.
|e author
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|a Ciani, G.
|e author
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|a Clara, F.
|e author
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|a Cook, D.
|e author
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|a Countryman, S. T.
|e author
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|a Cowart, M. J.
|e author
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|a Coyne, D. C.
|e author
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|a Cumming, A.
|e author
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|a Cunningham, L.
|e author
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|a Damjanic, M.
|e author
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|a Dannenberg, R.
|e author
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|a Danzmann, K.
|e author
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|a Costa, C. F. Da Silva
|e author
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|a Daw, E. J.
|e author
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|a DeBra, D.
|e author
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|a DeRosa, R. T.
|e author
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|a DeSalvo, R.
|e author
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|a Dooley, K. L.
|e author
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|a Doravari, S.
|e author
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|a Driggers, J. C.
|e author
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|a Dwyer, S. E.
|e author
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|a Effler, A.
|e author
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|a Etzel, T.
|e author
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|a Evans, T. M.
|e author
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|a Factourovich, M.
|e author
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|a Fair, H.
|e author
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|a Feldbaum, D.
|e author
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|a Fisher, R. P.
|e author
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|a Frede, M.
|e author
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|a Frolov, V. V.
|e author
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|a Fulda, P.
|e author
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|a Fyffe, M.
|e author
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|a Galdi, V.
|e author
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|a Giaime, J. A.
|e author
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|a Giardina, K. D.
|e author
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|a Gleason, J. R.
|e author
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|a Goetz, R.
|e author
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|a Gray, C.
|e author
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|a Greenhalgh, R. J. S.
|e author
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|a Grote, H.
|e author
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|a Guido, C. J.
|e author
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|a Gushwa, K. E.
|e author
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|a Gustafson, E. K.
|e author
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|a Gustafson, R.
|e author
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|a Hammond, G.
|e author
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|a Hanks, J.
|e author
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|a Hanson, J.
|e author
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|a Hardwick, T.
|e author
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|a Harry, G. M.
|e author
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|a Heefner, J.
|e author
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|a Heintze, M. C.
|e author
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|a Heptonstall, A. W.
|e author
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|a Hoak, D.
|e author
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|a Hough, J.
|e author
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|a Ivanov, A.
|e author
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|a Izumi, K.
|e author
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|a Jacobson, M.
|e author
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|a James, E.
|e author
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|a Jones, R.
|e author
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|a Kandhasamy, S.
|e author
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|a Karki, S.
|e author
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|a Kasprzack, M.
|e author
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|a Kaufer, S.
|e author
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|a Kawabe, K.
|e author
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|a Kells, W.
|e author
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|a Kijbunchoo, N.
|e author
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|a King, E. J.
|e author
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|a King, P. J.
|e author
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|a Kinzel, D. L.
|e author
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|a Kissel, J. S.
|e author
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|a Kokeyama, K.
|e author
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|a Korth, W. Z.
|e author
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|a Kuehn, G.
|e author
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|a Landry, M.
|e author
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|a Lantz, B.
|e author
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|a Le Roux, A.
|e author
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|a Levine, B. M.
|e author
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|a Lewis, J. B.
|e author
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|a Lhuillier, V.
|e author
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|a Lockerbie, N. A.
|e author
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|a Lormand, M.
|e author
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|a Lubinski, M. J.
|e author
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|a Lundgren, A. P.
|e author
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|a MacDonald, T.
|e author
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|a Macleod, D. M.
|e author
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|a Mageswaran, M.
|e author
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|a Mailand, K.
|e author
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|a Márka, S.
|e author
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|a Márka, Z.
|e author
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|a Markosyan, A. S.
|e author
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|a Maros, E.
|e author
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|a Martin, I. W.
|e author
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|a Martin, R. M.
|e author
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|a Marx, J. N.
|e author
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|a Massinger, T. J.
|e author
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|a McCarthy, R.
|e author
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|a McClelland, D. E.
|e author
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|a McCormick, S.
|e author
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|a McIntyre, G.
|e author
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|a McIver, J.
|e author
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|a Merilh, E. L.
|e author
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|a Meyer, M. S.
|e author
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|a Meyers, P. M.
|e author
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|a Moreno, G.
|e author
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|a Mueller, C. L.
|e author
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|a Mueller, G.
|e author
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|a Mullavey, A.
|e author
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|a Munch, J.
|e author
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|a Nuttall, L. K.
|e author
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|a Oberling, J.
|e author
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|a O'Dell, J.
|e author
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|a Oppermann, P.
|e author
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|a Oram, Richard J.
|e author
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|a O'Reilly, B.
|e author
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|a Osthelder, C.
|e author
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|a Ottaway, D. J.
|e author
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|a Overmier, H.
|e author
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|a Palamos, J. R.
|e author
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|a Paris, H. R.
|e author
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|a Parker, W.
|e author
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|a Patrick, Z.
|e author
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|a Pele, A.
|e author
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|a Penn, S.
|e author
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|a Phelps, M.
|e author
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|a Pickenpack, M.
|e author
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|a Pierro, V.
|e author
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|a Pinto, I.
|e author
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|a Poeld, J.
|e author
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|a Principe, M.
|e author
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|a Prokhorov, L.
|e author
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|a Puncken, O.
|e author
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|a Quetschke, V.
|e author
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|a Quintero, E. A.
|e author
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|a Raab, F. J.
|e author
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|a Radkins, H.
|e author
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|a Raffai, P.
|e author
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|a Ramet, C. R.
|e author
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|a Reed, C. M.
|e author
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|a Reid, S.
|e author
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|a Reitze, D. H.
|e author
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|a Robertson, N. A.
|e author
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|a Rollins, J. G.
|e author
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|a Roma, V. J.
|e author
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|a Romie, J. H.
|e author
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|a Rowan, S.
|e author
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|a Ryan, K.
|e author
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|a Sadecki, T.
|e author
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|a Sanchez, E. J.
|e author
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|a Sandberg, V.
|e author
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|a Sannibale, V.
|e author
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|a Savage, R. L.
|e author
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|a Schofield, R. M. S.
|e author
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|a Schultz, B.
|e author
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|a Schwinberg, P.
|e author
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|a Sellers, D.
|e author
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|a Sevigny, A.
|e author
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|a Shaddock, D. A.
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|a Shao, Z.
|e author
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|a Shapiro, B.
|e author
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|a Shawhan, P.
|e author
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|a Sigg, D.
|e author
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|a Slagmolen, B. J. J.
|e author
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|a Smith, J. R.
|e author
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|a Smith, M. R.
|e author
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|a Smith-Lefebvre, N. D.
|e author
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|a Sorazu, B.
|e author
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|a Staley, A.
|e author
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|a Stochino, A.
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|a Strain, K. A.
|e author
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|a Taylor, R.
|e author
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|a Thomas, M.
|e author
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|a Thomas, P.
|e author
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|a Thorne, K. A.
|e author
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|a Thrane, E.
|e author
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|a Torrie, C. I.
|e author
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|a Traylor, G.
|e author
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|a Vajente, G.
|e author
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|a Valdes, G.
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|a van Veggel, A. A.
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|a Vargas, M.
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|a Vecchio, A.
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|a Veitch, P. J.
|e author
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|a Venkateswara, K.
|e author
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|a Vo, T.
|e author
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|a Vorvick, C.
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|a Walker, M.
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|a Ward, R. L.
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|a Warner, J.
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|a Weaver, B.
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|a Welborn, T.
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|a Weßels, P.
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|a Wilkinson, C.
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|a Willems, P. A.
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|a Williams, L.
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|a Willke, B.
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|a Winkelmann, L.
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|a Wipf, C. C.
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|a Worden, J.
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|a Wu, G.
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|a Yamamoto, H.
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|a Yancey, C. C.
|e author
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|a Zhang, L.
|e author
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|a Zweizig, J.
|e author
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|a Barsotti, Lisa
|e author
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|a Biscans, Sebastien
|e author
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|a Evans, Matthew J
|e author
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|a Foley, Stephany
|e author
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|a Fritschel, Peter K
|e author
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1 |
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|a Gras, Slawomir
|e author
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700 |
1 |
0 |
|a Kwee, Patrick
|e author
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1 |
0 |
|a MacInnis, Myron E
|e author
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1 |
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|a Mason, Kenneth R
|e author
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|a Matichard, Fabrice
|e author
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|a Mavalvala, Nergis
|e author
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|a Miller, John
|e author
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|a Mittleman, Richard K
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|a Shoemaker, David H
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|a Waldman, Samuel J.
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|a Weiss, Rainer
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|a Yu, Hang
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|a Zucker, Michael E
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|a Stein, Andrew J.
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|a Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy
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|b American Physical Society,
|c 2017-07-11T19:33:29Z.
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|z Get fulltext
|u http://hdl.handle.net/1721.1/110647
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|a The Laser Interferometer Gravitational Wave Observatory (LIGO) consists of two widely separated 4 km laser interferometers designed to detect gravitational waves from distant astrophysical sources in the frequency range from 10 Hz to 10 kHz. The first observation run of the Advanced LIGO detectors started in September 2015 and ended in January 2016. A strain sensitivity of better than 10⁻²³/√Hz was achieved around 100 Hz. Understanding both the fundamental and the technical noise sources was critical for increasing the astrophysical strain sensitivity. The average distance at which coalescing binary black hole systems with individual masses of 30 M[subscript ⊙] could be detected above a signal-to-noise ratio (SNR) of 8 was 1.3 Gpc, and the range for binary neutron star inspirals was about 75 Mpc. With respect to the initial detectors, the observable volume of the Universe increased by a factor 69 and 43, respectively. These improvements helped Advanced LIGO to detect the gravitational wave signal from the binary black hole coalescence, known as GW150914.
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|a en
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|a Article
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|t Physical Review D
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