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dc.contributor.authorAggarwal, Nancy
dc.contributor.authorBarsotti, Lisa
dc.contributor.authorBiscans, Sebastien
dc.contributor.authorBlackburn, Lindy L.
dc.contributor.authorBodiya, Timothy P.
dc.contributor.authorBuikema, Aaron
dc.contributor.authorChatterji, Shourov K.
dc.contributor.authorDonovan, Frederick J
dc.contributor.authorEssick, Reed Clasey
dc.contributor.authorEvans, M.
dc.contributor.authorFritschel, Peter K
dc.contributor.authorGras, Slawomir
dc.contributor.authorIsogai, Tomoki
dc.contributor.authorKatsavounidis, Erotokritos
dc.contributor.authorKontos, Antonios
dc.contributor.authorLibson, Adam A.
dc.contributor.authorLynch, Ryan Christopher
dc.contributor.authorMacInnis, Myron E
dc.contributor.authorMason, Kenneth R
dc.contributor.authorMatichard, Fabrice
dc.contributor.authorMavalvala, Nergis
dc.contributor.authorMiller, John
dc.contributor.authorMittleman, Richard K
dc.contributor.authorRay Pitambar Mohapatra, Satyanarayan
dc.contributor.authorOelker, Eric Glenn
dc.contributor.authorShoemaker, David H
dc.contributor.authorTse, Maggie
dc.contributor.authorVaulin, Ruslan
dc.contributor.authorVitale, Salvatore
dc.contributor.authorWeiss, Rainer
dc.contributor.authorYam, William
dc.contributor.authorYu, H.
dc.contributor.authorZhang, F.
dc.contributor.authorZucker, Michael E
dc.contributor.authorLIGO Collaboration
dc.contributor.authorVirgo Collaboration
dc.contributor.authorBrown N. M.
dc.date.accessioned2019-11-05T15:05:50Z
dc.date.available2019-11-05T15:05:50Z
dc.date.issued2016-06
dc.date.submitted2016-02
dc.identifier.issn0264-9381
dc.identifier.issn1361-6382
dc.identifier.urihttps://hdl.handle.net/1721.1/122773
dc.description.abstractOn 14 September 2015, a gravitational wave signal from a coalescing black hole binary system was observed by the Advanced LIGO detectors. This paper describes the transient noise backgrounds used to determine the significance of the event (designated GW150914) and presents the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around the time of the event. The detectors were operating nominally at the time of GW150914. We have ruled out environmental influences and non-Gaussian instrument noise at either LIGO detector as the cause of the observed gravitational wave signal. Keywords: gravitational waves; detector characterization; GW150914en_US
dc.publisherIOP Publishingen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0264-9381/33/13/134001en_US
dc.rightsCreative Commons Attribution 3.0 unported licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/en_US
dc.sourceIOP Publishingen_US
dc.titleCharacterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914en_US
dc.typeArticleen_US
dc.identifier.citationAbbott, B P et al. “Characterization of Transient Noise in Advanced LIGO Relevant to Gravitational Wave Signal GW150914.” Classical and Quantum Gravity 33, 13 (June 2016): 134001 © 2016 IOP Publishing Ltden_US
dc.contributor.departmentMassachusetts Institute of Technology. Center for Theoretical Physicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentLincoln Laboratoryen_US
dc.contributor.departmentLIGO (Observatory : Massachusetts Institute of Technology)en_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.relation.journalClassical and Quantum Gravityen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2019-03-19T18:42:07Z
dspace.orderedauthorsAbbott, B P; Abbott, R; Abbott, T D; Abernathy, M R; Acernese, F; Ackley, K; Adamo, M; Adams, C; Adams, T; Addesso, P; Adhikari, R X; Adya, V B; Affeldt, C; Agathos, M; Agatsuma, K; Aggarwal, N; Aguiar, O D; Aiello, L; Ain, A; Ajith, P; Allen, B; Allocca, A; Altin, P A; Anderson, S B; Anderson, W G; Arai, K; Araya, M C; Arceneaux, C C; Areeda, J S; Arnaud, N; Arun, K G; Ascenzi, S; Ashton, G; Ast, M; Aston, S M; Astone, P; Aufmuth, P; Aulbert, C; 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; Behnke, B; Bejger, M; Bell, A S; Bell, C J; Berger, B K; Bergman, J; Bergmann, G; Berry, C P L; Bersanetti, D; Bertolini, A; Betzwieser, J; Bhagwat, S; Bhandare, R; Bilenko, I A; Billingsley, G; Birch, J; Birney, R; Biscans, S; Bisht, A; Bitossi, M; Biwer, C; Bizouard, M A; Blackburn, J K; Blackburn, L; Blair, C D; Blair, D G; Blair, R M; Bloemen, S; Bock, O; Bodiya, T P; Boer, M; Bogaert, G; Bogan, C; Bohe, A; Bojtos, P; Bond, C; Bondu, F; Bonnand, R; Boom, B A; Bork, R; Boschi, V; Bose, S; Bouffanais, Y; Bozzi, A; Bradaschia, C; Brady, P R; Braginsky, V B; Branchesi, M; Brau, J E; Briant, T; Brillet, A; Brinkmann, M; Brisson, V; Brockill, P; Brooks, A F; Brown, D A; Brown, D D; Brown, N M; Buchanan, C C; Buikema, A; Bulik, T; Bulten, H J; Buonanno, A; Buskulic, D; Buy, C; Byer, R L; Cadonati, L; Cagnoli, G; Cahillane, C; Bustillo, J Calderón; Callister, T; Calloni, E; Camp, J B; Cannon, K C; Cao, J; Capano, C D; Capocasa, E; Carbognani, F; Caride, S; Diaz, J Casanueva; Casentini, C; Caudill, S; Cavaglià, M; Cavalier, F; Cavalieri, R; Cella, G; Cepeda, C B; Baiardi, L Cerboni; Cerretani, G; Cesarini, E; Chakraborty, R; Chalermsongsak, T; Chamberlin, S J; Chan, M; Chao, S; Charlton, P; Chassande-Mottin, E; Chatterji, S; Chen, H Y; Chen, Y; Cheng, C; Chincarini, A; Chiummo, A; Cho, H S; Cho, M; Chow, J H; Christensen, N; Chu, Q; Chua, S; Chung, S; Ciani, G; Clara, F; Clark, J A; Cleva, F; Coccia, E; Cohadon, P-F; Colla, A; Collette, C G; Cominsky, L; Conte, A; Conti, L; Cook, D; Corbitt, T R; Cornish, N; Corsi, A; Cortese, S; Costa, C A; Coughlin, M W; Coughlin, S B; Coulon, J-P; Countryman, S T; Couvares, P; Cowan, E E; Coward, D M; Cowart, M J; Coyne, D C; Coyne, R; Craig, K; Creighton, J D E; Cripe, J; Crowder, S G; Cumming, A; Cunningham, L; Cuoco, E; Canton, T Dal; Danilishin, S L; D’Antonio, S; Danzmann, K; Darman, N S; Dattilo, V; Dave, I; Daveloza, H P; Davier, M; Davies, G S; Daw, E J; Day, R; DeBra, D; Debreczeni, G; Degallaix, J; Laurentis, M De; Deléglise, S; Pozzo, W Del; Denker, T; Dent, T; Dereli, H; Dergachev, V; DeRosa, R T; Rosa, R De; DeSalvo, R; Dhurandhar, S; Díaz, M C; Fiore, L Di; Giovanni, M Di; Lieto, A Di; Pace, S Di; Palma, I Di; Virgilio, A Di; Dojcinoski, G; Dolique, V; Donovan, F; 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dspace.embargo.termsNen_US
dspace.date.submission2019-04-04T10:30:23Z
mit.journal.volume33en_US
mit.journal.issue13en_US
mit.licensePUBLISHER_CCen_US


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