The Laser Interferometer Space Antenna (LISA) is required to reduce two important noise sources by post-processing on the ground using time-delay interferometry (TDI): phase noise of the on-board reference clocks and laser frequency noise. To achieve the desired suppression, the TDI algorithm needs measurements of the differential clock noise between any two spacecraft and inter-spacecraft ranging measurements with at least 1 m accuracy, which is beyond the precision of ground-based measurements for deep space missions. Therefore, we need on-board measurements by transmitting clock noise and ranging information between the spacecraft as auxiliary functions of the laser link. This paper reports our current experimental results in clock noise...
International audienceThe LISA mission is the future space-based gravitational wave (GW) observatory...
LISA is an upcoming ESA mission that will detect gravitational waves in space by interferometrically...
The LISA phase measurement system (PMS) will provide interferometric phase readout of the primary he...
The Laser Interferometer Space Antenna (LISA) is required to reduce two important noise sources by p...
International audienceThe Laser Interferometry Space Antenna (LISA) mission is the future space-base...
We report on the first demonstration of time-delay interferometry (TDI) for LISA, the Laser Interfer...
The relative motion of the LISA spacecraft will Doppler shift the laser frequencies by around 15 MHz...
Laser phase noise is the dominant noise source in the on-board measurements of the space-based gravi...
Auxiliary functions of the LISA laser link: ranging, clock noise transfer and data communication Thi...
International audienceTime-delay interferometry (TDI) is a crucial step in the on-ground data proces...
We discuss the baseline optical configuration for the Laser Interferometer Space Antenna (LISA) miss...
International audienceTime-delay interferometry (TDI) is a data processing technique for LISA design...
International audienceTime delay interferometry (TDI) is a postprocessing technique used in the Lase...
International audienceThe Laser Interferometer Space Antenna (LISA) is a European Space Agency missi...
International audienceThe LISA mission is the future space-based gravitational wave (GW) observatory...
LISA is an upcoming ESA mission that will detect gravitational waves in space by interferometrically...
The LISA phase measurement system (PMS) will provide interferometric phase readout of the primary he...
The Laser Interferometer Space Antenna (LISA) is required to reduce two important noise sources by p...
International audienceThe Laser Interferometry Space Antenna (LISA) mission is the future space-base...
We report on the first demonstration of time-delay interferometry (TDI) for LISA, the Laser Interfer...
The relative motion of the LISA spacecraft will Doppler shift the laser frequencies by around 15 MHz...
Laser phase noise is the dominant noise source in the on-board measurements of the space-based gravi...
Auxiliary functions of the LISA laser link: ranging, clock noise transfer and data communication Thi...
International audienceTime-delay interferometry (TDI) is a crucial step in the on-ground data proces...
We discuss the baseline optical configuration for the Laser Interferometer Space Antenna (LISA) miss...
International audienceTime-delay interferometry (TDI) is a data processing technique for LISA design...
International audienceTime delay interferometry (TDI) is a postprocessing technique used in the Lase...
International audienceThe Laser Interferometer Space Antenna (LISA) is a European Space Agency missi...
International audienceThe LISA mission is the future space-based gravitational wave (GW) observatory...
LISA is an upcoming ESA mission that will detect gravitational waves in space by interferometrically...
The LISA phase measurement system (PMS) will provide interferometric phase readout of the primary he...