Objects sensed by laser interferometers are usually not stable in position or orientation. This angular instability can lead to a coupling of angular tilt to apparent longitudinal displacement -- tilt-to-length coupling (TTL). In LISA this is a potential noise source for both the test mass interferometer and the long-arm interferometer. We have experimentally investigated TTL coupling in a setup representative for the LISA test mass interferometer and used this system to characterise two different imaging systems (a two-lens design and a four-lens design) both designed to minimise TTL coupling. We show that both imaging systems meet the LISA requirement of +-25 um/rad for interfering beams with relative angles of up to +-300 urad. Furthermo...
This paper is the second in a set of two investigating tilt-to-length (TTL) coupling. TTL describes ...
Tilt-to-length coupling was the limiting noise source in LISA Pathfinder between 20 and 200 mHz befo...
A coupling between angular jitter of satellite and length readout, called tilt-to-length coupling, i...
Objects sensed by laser interferometers are usually not stable in position or orientation. This angu...
Objects sensed by laser interferometers are usually not stable in position or orientation. This angu...
Objects sensed by laser interferometers are usually not stable in position or orientation. This angu...
The arm length and the isolation in space enable LISA to probe for signals unattainable on ground, o...
The laser interferometer space antenna (LISA) is a future space-based interferometric gravitational-...
The Laser Interferometer Space Antenna (LISA) is a future space-based interferometric gravitational-...
The laser interferometer space antenna (LISA) is a future space-based interferometric gravitational-...
Angular misalignment of one of the interfering beams in laser interferometers can couple into the in...
Angular misalignment of one of the interfering beams in laser interferometers can couple into the in...
Angular misalignment of one of the interfering beams in laser interferometers can couple into the in...
In the mid-2030s, the laser interferometer space antenna (LISA) is planned to be launched and will b...
The laser interferometer space antenna (LISA) is a future space-based interferometric gravitational-...
This paper is the second in a set of two investigating tilt-to-length (TTL) coupling. TTL describes ...
Tilt-to-length coupling was the limiting noise source in LISA Pathfinder between 20 and 200 mHz befo...
A coupling between angular jitter of satellite and length readout, called tilt-to-length coupling, i...
Objects sensed by laser interferometers are usually not stable in position or orientation. This angu...
Objects sensed by laser interferometers are usually not stable in position or orientation. This angu...
Objects sensed by laser interferometers are usually not stable in position or orientation. This angu...
The arm length and the isolation in space enable LISA to probe for signals unattainable on ground, o...
The laser interferometer space antenna (LISA) is a future space-based interferometric gravitational-...
The Laser Interferometer Space Antenna (LISA) is a future space-based interferometric gravitational-...
The laser interferometer space antenna (LISA) is a future space-based interferometric gravitational-...
Angular misalignment of one of the interfering beams in laser interferometers can couple into the in...
Angular misalignment of one of the interfering beams in laser interferometers can couple into the in...
Angular misalignment of one of the interfering beams in laser interferometers can couple into the in...
In the mid-2030s, the laser interferometer space antenna (LISA) is planned to be launched and will b...
The laser interferometer space antenna (LISA) is a future space-based interferometric gravitational-...
This paper is the second in a set of two investigating tilt-to-length (TTL) coupling. TTL describes ...
Tilt-to-length coupling was the limiting noise source in LISA Pathfinder between 20 and 200 mHz befo...
A coupling between angular jitter of satellite and length readout, called tilt-to-length coupling, i...