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@Article{CovasEGMNOPRSAABCCCCCCDEHKLLMMMMOPPPRRSSSSTTTTAAAAAAAAAABBBBBBBBBBBBBBBBBBCCCCCCCCCCCDCDDDDDDDEEEEFFGFFFFFFFFGGGGGGGGGGGHHHHHHHHHIIJKKKKKKKKKKKKLLLLLLMMMMMMMMMMMMMMMMMMMMMMMMMMMMMNNNOOOOOOOPPPPPPPPPPPQQRRRRRRRRRRRRSSSSSSSSSSSSSSSSSSTTTTTTTTTTVVVVVVVVWWWWWWWWWWWYYYYZZZZ:2018:IdMiNa,
               author = "Covas, P. B. and Effler, A. and Goetz, E. and Meyers, P. M. and 
                         Neunzert, A. and Oliver, M. and Pearlstone, B. L. and Roma, V. J. 
                         and Schofield, R. M. S. and Adya, V. B. and Astone, P. and 
                         Biscoveanu, S. and Callister, T. A. and Christensen, N. and Colla, 
                         A. and Coughlin, E. and Coughlin, M. W. and Crowder, S. G. and 
                         Dwyer, S. E. and Eggenstein, H. -B. and Hourihane, S. and 
                         Kandhasamy, S. and Liu, W. and Lundgren, A. P. and Matas, A. and 
                         McCarthy, R. and McIver, J. and Mendell, G. and Ormiston, R. and 
                         Palomba, C. and Papa, M. A. and Piccinni, O. J. and Rao, K. and 
                         Riles, K. and Sammut, L. and Schlassa, S. and Sigg, D. and 
                         Strauss, N. and Tao, D. and Thorne, K. A. and Thrane, E. and 
                         Trembath-Reichert, S. and Abbott, B. P. and Abbott, R. and Abbott, 
                         T. D. and Adams, C. and Adhikari, R. X. and Ananyeva, A. and 
                         Appert, S. and Arai, K. and Aston, S. M. and Austin, C. and 
                         Ballmer, S. W. and Barker, D. and Barr, B. and Barsotti, L. and 
                         Bartlett, J. and Bartos, I. and Batch, J. C. and Bejger, M. and 
                         Bell, A. S. and Betzwieser, J. and Billingsley, G. and Birch, J. 
                         and Biscans, S. and Biwer, C. and Blair, C. D. and Blair, R. M. 
                         and Bork, R. and Brooks, A. F. and Cao, H. and Ciani, G. and 
                         Clara, F. and Clearwater, P. and Cooper, S. J. and Corban, P. and 
                         Countryman, S. T. and Cowart, M. J. and Coyne, D. C. and Cumming, 
                         A. and Cunningham, L. and Danzmann, K. and Costa, C. F. Da Silva 
                         and Daw, E. J. and DeBra, D. and DeRosa, R. T. and DeSalvo, R. and 
                         Dooley, K. L. and Doravari, S. and Driggers, J. C. and Edo, T. B. 
                         and Etzel, T. and Evans, M. and Evans, T. M. and Factourovich, M. 
                         and Fair, H. and Galiana, A. Fern{\'a}ndez and Ferreira, 
                         {\'E}lvis Camilo and Fisher, R. P. and Fong, H. and Frey, R. and 
                         Fritschel, P. and Frolov, V. V. and Fulda, P. and Fyffe, M. and 
                         Gateley, B. and Giaime, J. A. and Giardina, K. D. and Goetz, R. 
                         and Goncharov, B. and Gras, 10 S. and Gray, C. and Grote, H. and 
                         Gushwa, K. E. and Gustafson, E. K. and Gustafson, R. and Hall, E. 
                         D. and Hammond, G. and Hanks, J. and Hanson, J. and Hardwick, T. 
                         and Harry, G. M. and Heintze, M. C. and Heptonstall, A. W. and 
                         Hough, J. and Inta, R. and Izumi, K. and Jones, R. and Karki, S. 
                         and Kasprzack, M. and Kaufer, S. and Kawabe, K. and Kennedy, R. 
                         and Kijbunchoo, N. and Kim, W. and King, E. J. and King, P. J. and 
                         Kissel, J. S. and Korth, W. Z. and Kuehn, G. and Landry, M. and 
                         Lantz, B. and Laxen, M. and Liu, J. and Lockerbie, N. A. and 
                         Lormand, M. and MacInnis, M. and Macleod, D. M. and M{\'a}rka, S. 
                         and M{\'a}rka, Z. and Markosyan, A. S. and Maros, E. and Marsh, 
                         P. and Martin, I. W. and Martynov, D. V. and Mason, K. and 
                         Massinger, T. J. and Matichard, F. and Mavalvala, N. and 
                         McClelland, D. E. and McCormick, S. and McCuller, L. and McIntyre, 
                         G. and McRae, T. and Merilh, E. L. and Miller, J. and Mittleman, 
                         R. and Mo, G. and Mogushi, K. and Moraru, D. and Moreno, G. and 
                         Mueller, G. and Mukund, N. and Mullavey, A. and Munch, J. and 
                         Nelson, T. J. N. and Nguyen, P. and Nuttall, L. K. and Oberling, 
                         J. and Oktavia, O. and Oppermann, P. and Oram, Richard J. and 
                         O’Reilly, B. and Ottaway, D. J. and Overmier, H. and Palamos, J. 
                         R. and Parker, W. and Pele, A. and Penn, S. and Perez, C. J. and 
                         Phelps, M. and Pierro, V. and Pinto, I. and Principe, M. and 
                         Prokhorov, L. G. and Puncken, O. and Quetschke, V. and Quintero, 
                         E. A. and Radkins, H. and Raffai, P. and Ramirez, K. E. and Reid, 
                         S. and Reitze, D. H. and Robertson, N. A. and Rollins, J. G. and 
                         Romel, C. L. and Romie, J. H. and Ross, M. P. and Rowan, S. and 
                         Ryan, K. and Sadecki, T. and Sanchez, E. J. and Sanchez, L. E. and 
                         Sandberg, V. and Savage, R. L. and Sellers, D. and Shaddock, D. A. 
                         and Shaffer, T. J. and Shapiro, B. and Shoemaker, D. H. and 
                         Slagmolen, B. J. J. and Smith, B. and Smith, J. R. and Sorazu, B. 
                         and Spencer, A. P. and Staley, A. and Strain, K. A. and Sun, L. 
                         and Tanner, D. B. and Tasson, J. D. and Taylor, R. and Thomas, M. 
                         and Thomas, P. and Toland, K. and Torrie, C. I. and Traylor, G. 
                         and Tse, M. and Tuyenbayev, D. and Vajente, G. and Valdes, G. and 
                         Veggel, A. A. van and Vecchio, A. and Veitch, P. J. and 
                         Venkateswara, K. and Vo, T. and Vorvick, C. and Wade, M. and 
                         Walker, M. and Ward, R. L. and Warner, J. and Weaver, B. and 
                         Weiss, R. and Weßels, P. and Willke, B. and Wipf, C. C. and 
                         Wofford, J. and Worden, J. and Yamamoto, H. and Yancey, C. C. and 
                         Yu, Hang and Yu, Haocun and Zhang, L. and Zhu, S. and Zucker, M. 
                         E. and Zweizig, J.",
          affiliation = "{Universitat de les Illes Balears} and {Universitat de les Illes 
                         Balear} and {LIGO Livingston Observatory} and {Max Planck 
                         Institute for Gravitational Physics} and {University of Minnesota} 
                         and {University of Michigan} and {Universitat de les Illes 
                         Balears} and SUPA, University of Glasgow and {University of 
                         Oregon} and {University of Oregon} and {Max Planck Institute for 
                         Gravitational Physics} and INFN, Sezione di Roma and {Monash 
                         University} and LIGO, California Institute of Technology and 
                         Universit{\'e} C{\^o}te d’Azur, Observatoire C{\^o}te d’Azur 
                         and INFN, Sezione di Roma and Carleton College, Northfield and 
                         LIGO, California Institute of Technology and {Bellevue College} 
                         and {LIGO Hanford Observatory} and {Max Planck Institute for 
                         Gravitational Physics (Albert Einstein Institute)} and {University 
                         of Michigan} and {LIGO Livingston Observatory} and {University of 
                         Michigan} and {Max Planck Institute for Gravitational Physics} and 
                         {University of Minnesota} and {LIGO Hanford Observatory} and LIGO, 
                         California Institute of Technology and {LIGO Hanford Observatory} 
                         and {University of Minnesota} and INFN, Sezione di Roma and {Max 
                         Planck Institute for Gravitational Physics} and INFN, Sezione di 
                         Roma and {University of Michigan} and {University of Michigan} and 
                         {Monash University} and {Carleton College} and {LIGO Hanford 
                         Observatory} and {Carleton College} and {Carleton College} and 
                         {LIGO Livingston Observatory} and {Monash University} and 
                         {University of Michigan} and LIGO, California Institute of 
                         Technology and LIGO, California Institute of Technology and {} and 
                         {} and {} and {} and {} and {} and {} and {} and {} and {} and {} 
                         and {} and {} and {} and {} and {} and {} and {} and {} and {} and 
                         {} and {} and {} and {} and {} and {} and {} and {} and {} and {} 
                         and {} and {} and {} and {} and {} and {} and {} and {} and {} and 
                         {} and {} and {} and {} and {} and {} and {} and {} and {} and {} 
                         and {} and {} and {} and {Instituto Nacional de Pesquisas 
                         Espaciais (INPE)}",
                title = "Identification and mitigation of narrow spectral artifacts that 
                         degrade searches for persistent gravitational waves in the first 
                         two observing runs of Advanced LIGO",
              journal = "Physical Review D",
                 year = "2018",
               volume = "97",
               number = "8",
                pages = "e082002",
                month = "Apr.",
             abstract = "Searches are under way in Advanced LIGO and Virgo data for 
                         persistent gravitational waves from continuous sources, e.g. 
                         rapidly rotating galactic neutron stars, and stochastic sources, 
                         e.g. relic gravitational waves from the Big Bang or superposition 
                         of distant astrophysical events such as mergers of black holes or 
                         neutron stars. These searches can be degraded by the presence of 
                         narrow spectral artifacts (lines) due to instrumental or 
                         environmental disturbances. We describe a variety of methods used 
                         for finding, identifying and mitigating these artifacts, 
                         illustrated with particular examples. Results are provided in the 
                         form of lists of line artifacts that can safely be treated as 
                         non-astrophysical. Such lists are used to improve the efficiencies 
                         and sensitivities of continuous and stochastic gravitational wave 
                         searches by allowing vetoes of false outliers and permitting data 
                         cleaning.",
                  doi = "10.1103/PhysRevD.97.082002",
                  url = "http://dx.doi.org/10.1103/PhysRevD.97.082002",
                 issn = "1550-2368 and 1550-7998",
             language = "en",
           targetfile = "covas_identification.pdf",
        urlaccessdate = "24 nov. 2020"
}


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