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.
The static arm lengths given are those assumed in [7]
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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.