{"id":"W2158293236","doi":"10.1088/0264-9381/32/11/115012","title":"Characterization of the LIGO detectors during their sixth science run","year":2015,"lang":"en","type":"article","venue":"Classical and Quantum Gravity","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1317,"is_retracted":false,"has_abstract":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Division of Physics; Ministero dello Sviluppo Economico; Australian Research Council; National Research Foundation of Korea; Ministerio de Economía y Competitividad; Centre National de la Recherche Scientifique; Industry Canada; Govern de les Illes Balears; Fundacja na rzecz Nauki Polskiej; National Science Foundation; Royal Society; Scottish Funding Council; Scottish Universities Physics Alliance; Istituto Nazionale di Fisica Nucleare; David and Lucile Packard Foundation; Hungarian Scientific Research Fund; Leverhulme Trust; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Council of Scientific and Industrial Research, India; Science and Technology Facilities Council; National Research Foundation; Alfred P. Sloan Foundation; National Aeronautics and Space Administration","keywords":"LIGO; Physics; Gravitational wave; Interferometry; Detector; Noise (video); Astronomy; Astrophysics; Sensitivity (control systems); Gravitational-wave astronomy; Optics; Electronic engineering; Computer science","routes":{"ca_aff":true,"ca_fund":true,"ca_venue":false,"about_ca":false,"invisible_to_affiliation_only":false},"retraction":null,"screen":null,"machine_scores":{"provisional":true,"baseline":true,"maturity_gate_passed":false,"score_opus":0.01968918980061782,"score_gpt":0.2889964154050896,"score_spread":0.2693072256044717,"validation_status":"score_only:v0-immature-baseline","note":"Baseline scores from an immature model (maturity gate not passed). Scores rank; they never assert a category."}}