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The dissertation addresses the technological challenges of gravitational-wave detection from space, focusing on the LISA mission, which aims to launch in the late 2030s. It involves modeling, estimation, and calibration of tilt-to-length coupling noise to meet the precision needed for detecting gravitational waves from various cosmic sources.
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Tilt-to-Length Noise Estimation and Reduction Algorithms for Spaceborne Gravitational-Wave Observatories, Niklas Houba
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- 2023
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