Measurement and subtraction of Schumann resonances at gravitational-wave interferometers

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An upper limit on the stochastic gravitational-wave background of cosmological origin

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Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600–1000 Hz

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Correlated magnetic noise in global networks of gravitational-wave detectors: Observations and implications

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Correlated noise in networks of gravitational-wave detectors: Subtraction and mitigation

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Improved Upper Limits on the Stochastic Gravitational-Wave Background from 2009-2010 LIGO and Virgo Data

Aasi, J. et al · 2014

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Extremely low frequency electromagnetic field measurements at the Hylaty station and methodology of signal analysis

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Knee model: Comparison between heuristic and rigorous solutions for the Schumann resonance problem

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GW150914: Implications for the Stochastic Gravitational-Wave Background from Binary Black Holes

B. P. et al. Abbott · 2016

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Subtraction of correlated noise in global networks of gravitational-wave interferometers

Michael W Coughlin, Nelson L Christensen, Rosario De Rosa, Irene Fiori, Mark Gołkowski, Melissa Guidry, Jan Harms, Jerzy Kubisz, Andrzej Kulak, Janusz Mlynarczyk, Federico Paoletti, and Eric Thrane · 2016

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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott, R. Abbott, T. D. Abbott, F. Acernese, K. Ackley, C. Adams, T. Adams, P. Addesso, and et al · 2017

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Globally coherent short duration magnetic field transients and their effect on ground based gravitational-wave detectors