Authors

P. Nguyen, University of Oregon
R. M.S. Schofield, University of Oregon
A. Effler, LIGO Livingston
C. Austin, Louisiana State University
V. Adya, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
M. Ball, University of Oregon
S. Banagiri, University of Minnesota Twin Cities
K. Banowetz, California Institute of Technology
C. Billman, University of Florida
C. D. Blair, LIGO Livingston
A. Buikema, LIGO Livingston
C. Cahillane, California Institute of Technology
F. Clara, LIGO Hanford
P. B. Covas, Universitat de les Illes Balears
G. Dalya, Eötvös Loránd Tudományegyetem
C. Daniel, California Institute of Technology
B. Dawes, California Institute of Technology
R. Derosa, LIGO Livingston
S. E. Dwyer, LIGO Hanford
R. Frey, University of Oregon
V. V. Frolov, LIGO Livingston
D. Ghirado, California Institute of Technology
E. Goetz, Louisiana State University
T. Hardwick, Louisiana State University
A. F. Helmling-Cornell, University of Oregon
I. J. Hollows, The University of Sheffield
N. Kijbunchoo, The Australian National University
J. Kruk, California Institute of Technology
M. Laxen, LIGO Livingston
E. Maaske, California Institute of Technology
G. L. Mansell, LIGO, Massachusetts Institute of Technology
R. McCarthy, LIGO Hanford
K. Merfeld, University of Oregon
A. Neunzert, University of Michigan-Ann Arbor
J. R. Palamos, University of Oregon
W. Parker, LIGO Livingston Observatory
B. Pearlstone, University of Glasgow
A. Pele, LIGO Livingston Observatory
H. Radkins, LIGO Hanford Observatory
V. Roma, University of Oregon
R. L. Savage, LIGO Hanford Observatory
P. Schale, University of Oregon
D. Shoemaker, Massachusetts Institute of Technology
T. Shoemaker, California Institute of Technology
S. Soni, Louisiana State University at Baton Rouge
D. Talukder, University of Oregon
M. Tse, Massachusetts Institute of Technology
G. Valdes, Louisiana State University at Baton Rouge
M. Vidreo, California Institute of Technology
C. Vorvick, LIGO Hanford Observatory
R. Abbott, California Institute of Technology
C. Adams, LIGO Livingston Observatory
R. X. Adhikari, California Institute of Technology
A. Ananyeva, California Institute of Technology
S. Appert, California Institute of Technology
K. Arai, California Institute of Technology
J. S. Areeda, California State University, Fullerton
Y. Asali, Columbia University
S. M. Aston, LIGO Livingston Observatory
A. M. Baer, Christopher Newport University
S. W. Ballmer, Syracuse University
D. Barker, LIGO Hanford Observatory
L. Barsotti, Massachusetts Institute of Technology
J. Bartlett, LIGO Hanford Observatory
B. K. Berger, Stanford University
J. Betzwieser, LIGO Livingston Observatory
D. Bhattacharjee, Missouri University of Science and Technology
G. Billingsley, California Institute of Technology
S. Biscans, Massachusetts Institute of Technology
R. M. Blair, LIGO Hanford Observatory
N. Bode, Max Planck Institute for Gravitational Physics
P. Booker, Max Planck Institute for Gravitational Physics
R. Bork, California Institute of Technology
A. Bramley, LIGO Livingston Observatory
A. F. Brooks, California Institute of Technology
D. D. Brown, University of Adelaide
K. C. Cannon, University of Tokyo
X. Chen, University of Western Australia
A. A. Ciobanu, University of Adelaide
S. J. Cooper, University of Birmingham
C. M. Compton, LIGO Hanford Observatory
K. R. Corley, Columbia University
S. T. Countryman, Columbia University
D. C. Coyne, California Institute of Technology
L. E. H. Datrier, University of Glasgow
D. Davis, Syracuse University
C. Di Fronzo, University of Birmingham
K. L. Dooley, Cardiff University
J. C. Driggers, LIGO Hanford Observatory
P. Dupej, University of Glasgow
T. Etzel, California Institute of Technology
M. Evans, Massachusetts Institute of Technology
T. M. Evans, LIGO Livingston Observatory
J. Feicht, California Institute of Technology
A. Fernandez-Galiana, Massachusetts Institute of Technology
P. Fritschel, Massachusetts Institute of Technology
P. Fulda, University of Florida
M. Fyffe, LIGO Livingston Observatory
J. A. Giaime, Louisiana State University at Baton Rouge
K. D. Giardina, LIGO Livingston Observatory
P. Godwin, The Pennsylvania State University
S. Gras, Massachusetts Institute of Technology
C. Gray, LIGO Hanford Observatory
R. Gray, University of Glasgow
A. C. Green, California Institute of Technology
E. K. Gustafson, California Institute of Technology
R. Gustafson, University of Michigan-Ann Arbor
J. Hanks, LIGO Hanford Observatory
J. Hanson, LIGO Livingston Observatory
R. H. Hasskew, LIGO Livingston Observatory
M. C. Heintze, LIGO Livingston Observatory
N. A. Holland, Australian National University
J. D. Jones, LIGO Hanford Observatory
S. Kandhasamy, Inter-University Centre for Astronomy and Astrophysics
S. Karki, University of Oregon
M. Kasparzack, California Institute of Technology
K. Kawabe, LIGO Hanford Observatory
P. J. King, LIGO Hanford Observatory
J. S. Kissel, LIGO Hanford Observatory
R. Kumar, LIGO Hanford Observatory
M. Landry, LIGO Hanford Observatory
B. B. Lane, Massachusetts Institute of Technology
B. Lantz, Stanford University
Y. K. Lecoeuche, LIGO Hanford Observatory
J. Leviton, University of Michigan-Ann Arbor
J. Liu, Max Planck Institute for Gravitational Physics
M. Lormand, LIGO Livingston Observatory
A. P. Lundgren, University of Portsmouth
R. Macas, Cardiff University
M. MacInnis, Massachusetts Institute of Technology
D. M. Macleod, Cardiff University
S. Marka, Columbia University
Z. Marka, Columbia University
D. V. Martynov, University of Birmingham
K. Mason, Massachusetts Institute of Technology
T. J. Massinger, Massachusetts Institute of Technology
F. Matichard, California Institute of Technology
N. Mavalvala, Massachusetts Institute of Technology
D. E. McClelland, Australian National University
S. McCormick, LIGO Livingston Observatory
L. McCuller, Massachusetts Institute of Technology
J. McIver, California Institute of Technology
T. McRae, Australian National University
G. Mendell, LIGO Hanford Observatory
E. L. Merilh, LIGO Hanford Observatory
F. Meylahn, Max Planck Institute for Gravitational Physics
P. M. Meyers, University of Melbourne
T. Mistry, The University of Sheffield
R. Mitteman, Massachusetts Institute of Technology
G. Moreno, LIGO Hanford Observatory
C. M. Mow-Lowry, University of Birmingham
S. Mozzon, University of Portsmouth
A. Mullavey, LIGO Livingston Observatory
T. J. N. Nelson, LIGO Livingston Observatory
L. K. Nuttall, University of Portsmouth
J. Oberling, LIGO Hanford Observatory
R. J. Oram, LIGO Livingston Observatory
C. Osthelder, California Institute of Technology
D. J. Ottaway, University of Adelaide
H. Overmier, LIGO Livingston Observatory
E. Payne, Monash University, Australia
R. Penhorwood, University of Michigan-Ann Arbor
C. J. Perez, LIGO Hanford Observatory
M. Pirello, LIGO Hanford Observatory
K. E. Ramirez, The University of Texas Rio Grande Valley
J. W. Richardson, California Institute of Technology
K. Riles, University of Michigan-Ann Arbor
N. A. Robertson, California Institute of Technology
J. G. Rollins, California Institute of Technology
C. L. Romel, LIGO Hanford Observatory
J. H. Romie, LIGO Livingston Observatory
M. P. Ross, University of Washington
K. Ryan, LIGO Hanford Observatory
T. Sadecki, LIGO Hanford Observatory
E. J. Sanchez, California Institute of Technology
L. E. Sanchez, California Institute of Technology
T. R. Saravanan, Inter-University Centre for Astronomy and Astrophysics
D. Schaetzl, California Institute for Gravitational Physics
R. Schnabel, Universitat Hamburg
E. Schwartz, LIGO Livingston Observatory
D. Sellers, LIGO Livingston Observatory
T. Shaffer, LIGO Hanford Observatory
D. Sigg, LIGO Hanford Observatory
B. J. J. Slagmolen, Australian National University
J. R. Smith, California State University Fullerton
B. Sorazu, University of Glasgow
A. P. Spencer, University of Glasgow
K. A. Strain, University of Glasgow
L. Sun, California Institute of Technology
M. J. Szczepanczyk, University of Florida
M. Thomas, LIGO Livingston Observatory
P. Thomas, LIGO Hanford Observatory
K. A. Thorne, LIGO Livingston Observatory
K. Toland, University of Glasgow
C. I. Torrie, California Institute of Technology
G. Traylor, LIGO Livingston Observatory
A. L. Urban, Louisiana State University at Baton Rouge
G. Vajente, California Institute of Technology
D. C. Bander-Hyde, Syracuse University
P. J. Veitch, University of Adelaide
K. Venkateswara, University of Washington - Seattle Campus
G. Venugopalan, California Institute of Technology
A. D. Viets, Concordia University - Wisconsin
T. Vo, Syracuse University
M. Wade, Kenyon College
R. L. Ward, Australian National University
J. Warner, LIGO Hanford Observatory
B. Weaver, LIGO Hanford Observatory
R. Weiss, Massachusetts Institute of Technology
C. Whittle, Massachusetts Institute of Technology
B. Willke, Leibniz University Hannover
C. C. Wipf, California Institute of Technology
L. Xiao, California Institute of Technology
H. Yamamoto, California Institute of Technology
H. Yu, Massachusetts Institute of Technology
L. Zhang, California Institute of Technology
M. E. Zucker, Massachusetts Institute of Technology
J. Zweizig, California Institute of Technology

Document Type

Article

Publication Date

7-1-2021

Abstract

The sensitivity of the advanced LIGO detectors to gravitational waves can be affected by environmental disturbances external to the detectors themselves. Since the transition from the former initial LIGO phase, many improvements have been made to the equipment and techniques used to investigate these environmental effects. These methods have aided in tracking down and mitigating noise sources throughout the first three observing runs of the advanced detector era, keeping the ambient contribution of environmental noise below the background noise levels of the detectors. In this paper we describe the methods used and how they have led to the mitigation of noise sources, the role that environmental monitoring has played in the validation of gravitational wave events, and plans for future observing runs.

Publication Source (Journal or Book title)

Classical and Quantum Gravity

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