Tilt-to-length coupling noise can be fitted and subtracted from simulated LISA data without being confused by, or damaging, gravitational wave signals from several source types.
Non- geometric tilt-to-length coupling in space interferometry: mechanisms and analytical descriptions
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Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals
Tilt-to-length coupling noise can be fitted and subtracted from simulated LISA data without being confused by, or damaging, gravitational wave signals from several source types.