Effects of transients in LIGO suspensions on searches for gravitational waves
Creators: name: Walker, M.
name: Abbott, T. D.
name: Aston, S. M.
name: González, G.
name: Macleod, D. M.
name: McIver, J.
name: Abbott, B. P.
name: Abbott, R.
name: Adams, C.
name: Adhikari, R. X.
name: Anderson, S. B.
name: Ananyeva, A.
name: Appert, S.
name: Arai, K.
name: Ballmer, S. W.
name: Barker, D.
name: Barr, B.
name: Barsotti, L.
name: Bartlett, J.
name: Bartos, I.
name: Batch, J. C.
name: Bell, A. S.
name: Betzwieser, J.
name: Billingsley, G.
name: Birch, J.
name: Biscans, S.
name: Biwer, C.
name: Blair, C. D.
name: Bork, R.
name: Brooks, A. F.
name: Ciani, G.
name: Clara, F.
name: Countryman, S. T.
name: Cowart, M. J.
name: Coyne, D. C.
name: Cumming, A.
name: Cunningham, L.
name: Danzmann, K.
name: Costa, C. F. Da Silva
name: Daw, E. J.
name: DeBra, D.
name: DeRosa, R. T.
name: DeSalvo, R.
name: Dooley, K. L.
name: Doravari, S.
name: Driggers, J. C.
name: Dwyer, S. E.
name: Effler, A.
name: Etzel, T.
name: Evans, M.
name: Evans, T. M.
name: Factourovich, M.
name: Fair, H.
name: Galiana, A. Fernández
name: Fisher, R. P.
name: Fritschel, P.
name: Frolov, V. V.
name: Fulda, P.
name: Fyffe, M.
name: Giaime, J. A.
name: Giardina, K. D.
name: Goetz, E.
name: Goetz, R.
name: Gras, S.
name: Gray, C.
name: Grote, H.
name: Gushwa, K. E.
name: Gustafson, E. K.
name: Gustafson, R.
name: Hall, E. D.
name: Hammond, G.
name: Hanks, J.
name: Hanson, J.
name: Hardwick, T.
name: Harry, G. M.
name: Heintze, M. C.
name: Heptonstall, A. W.
name: Hough, J.
name: Izumi, K.
name: Jones, R.
name: Kandhasamy, S.
name: Karki, S.
name: Kasprzack, M.
name: Kaufer, S.
name: Kawabe, K.
name: Kijbunchoo, N.
name: King, E. J.
name: King, P. J.
name: Kissel, J. S.
name: Korth, W. Z.
name: Kuehn, G.
name: Landry, M.
name: Lantz, B.
name: Lockerbie, N. A.
name: Lormand, M.
name: Lundgren, A. P.
name: MacInnis, M.
name: Márka, S.
name: Márka, Z.
name: Markosyan, A. S.
name: Maros, E.
name: Martin, I. W.
name: Martynov, D. V.
name: Mason, K.
name: Massinger, T. J.
name: Matichard, F.
name: Mavalvala, N.
name: McCarthy, R.
name: McClelland, D. E.
name: McCormick, S.
name: McIntyre, G.
name: Mendell, G.
name: Merilh, E. L.
name: Meyers, P. M.
name: Miller, J.
name: Mittleman, R.
name: Moreno, G.
name: Mueller, G.
name: Mullavey, A.
name: Munch, J.
name: Nuttall, L. K.
name: Oberling, J.
name: Oliver, M.
name: Oppermann, P.
name: Oram, Richard J.
name: O'Reilly, B.
name: Ottaway, D. J.
name: Overmier, H.
name: Palamos, J. R.
name: Paris, H. R.
name: Parker, W.
name: Pele, A.
name: Penn, S.
name: Phelps, M.
name: Pierro, V.
name: Pinto, I.
name: Principe, M.
name: Prokhorov, L. G.
name: Puncken, O.
name: Quetschke, V.
name: Quintero, E. A.
name: Raab, F. J.
name: Radkins, H.
name: Raffai, P.
name: Reid, S.
name: Reitze, D. H.
name: Robertson, N. A.
name: Rollins, J. G.
name: Roma, V. J.
name: Romie, J. H.
name: Rowan, S.
name: Ryan, K.
name: Sadecki, T.
name: Sanchez, E. J.
name: Sandberg, V.
name: Savage, R. L.
name: Schofield, R. M. S.
name: Sellers, D.
name: Shaddock, D. A.
name: Share, T. J.
name: Shapiro, B.
name: Shawhan, P.
name: Shoemaker, D. H.
name: Sigg, D.
name: Slagmolen, B. J. J.
name: Smith, B.
name: Smith, J. R.
name: Sorazu, B.
name: Staley, A.
name: Strain, K. A.
name: Tanner, D. B.
name: Taylor, R.
name: Thomas, M.
name: Thomas, P.
name: Thorne, K. A.
name: Thrane, E.
name: Torrie, C. I.
name: Traylor, G.
name: Tuyenbayev, D.
name: Vajente, G.
name: Valdes, G.
name: van Veggel, A. A.
name: Vecchio, A.
name: Veitch, P. J.
name: Venkateswara, K.
name: Vo, T.
name: Vorvick, C.
name: Ward, R. L.
name: Warner, J.
name: Weaver, B.
name: Weiss, R.
name: Weßels, P.
name: Willke, B.
name: Wipf, C. C.
name: Worden, J.
name: Wu, G.
name: Yamamoto, H.
name: Yancey, C. C.
name: Yu, Hang
name: Yu, Haocun
name: Zhang, L.
name: Zucker, M. E.
name: Zweizig, J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: This paper presents an analysis of the transient behavior of the Advanced LIGO suspensions used to seismically isolate the optics. We have characterized the transients in the longitudinal motion of the quadruple suspensions during Advanced LIGO's first observing run. Propagation of transients between stages is consistent with modelled transfer functions, such that transient motion originating at the top of the suspension chain is significantly reduced in amplitude at the test mass. We find that there are transients seen by the longitudinal motion monitors of quadruple suspensions, but they are not significantly correlated with transient motion above the noise floor in the gravitational wave strain data, and therefore do not present a dominant source of background noise in the searches for transient gravitational wave signals.