activity
20242026
collaborators

6 papers

astro-ph.IM2026

LISA Non-Linear Dynamics and Tilt-To-Length Coupling

Lavinia Heisenberg, Henri Inchauspé, Sarah Paczkowski +1

For the LISA mission, Tilt-To-Length (TTL) coupling is expected to be one of the dominant instrumental noise contributions after laser frequency noise is suppressed based, on assum…

astro-ph.IM2025

Post-processing subtraction of tilt-to-length noise in LISA in the presence of gravitational wave signals

Marie-Sophie Hartig, Sarah Paczkowski, Martin Hewitson +2

The Laser Interferometer Space Antenna (LISA) will be the first space-based gravitational wave (GW) observatory. It will measure gravitational wave signals in the frequency regime…

astro-ph.IM2025

Tilt-To-Length Coupling in LISA -- Uncertainty and Biases

Marie-Sophie Hartig, Joshua Marmor, Daniel George +2

The coupling of the angular jitter of the spacecraft and their sub-assemblies with the optical bench and the telescope into the interferometric length readout will be a major noise…

gr-qc2024

Design of Dedicated Tilt-to-Length Calibration Maneuvers for LISA

Henry Wegener, Sarah Paczkowski, Marie-Sophie Hartig +3

Tilts of certain elements within a laser interferometer can undesirably couple into measurements as a form of noise, known as tilt-to-length (TTL) coupling. This TTL coupling is an…

astro-ph.IM2024

Precision measurements of the magnetic parameters of LISA Pathfinder test masses

M Armano, H Audley, J Baird +76

A precise characterization of the magnetic properties of LISA Pathfinder free falling test-masses is of special interest for future gravitational wave observatory in space. Magneti…

astro-ph.IM2024

Magnetic-induced force noise in LISA Pathfinder free-falling test masses

M Armano, H Audley, J Baird +76

LISA Pathfinder was a mission designed to test key technologies required for gravitational wave detection in space. Magnetically driven forces play a key role in the instrument sen…