B. Kaune

TL;DR: The first results of the LISA Pathfinder in-flight experiment demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational wave observatory like LISA, can be put in free fall with a relative acceleration noise with a square root of the power spectral density.

TL;DR: This performance provides an experimental benchmark demonstrating the ability to realize the low-frequency science potential of the LISA mission, recently selected by the European Space Agency.

TL;DR: In this paper, the authors report on the temperature measurements throughout mission operations, characterize the thermal environment, estimate transfer functions between different locations, and report temperature stability (and its time evolution) at frequencies as low as 10'|$\mu$|Hz, where typically values around 1'K'Hz^−1'1/2 were measured.

TL;DR: In this paper, the authors report on the magnetic measurements throughout LISA Pathfinder (LPF) operations and characterize the magnetic environment within the spacecraft, study the time evolution of the magnetic field and its stability down to 20μHz.

TL;DR: The LISA Pathfinder satellite was launched on 3 December 2015 toward the Sun Earth first Lagrangian point (L1) where the LISA Technology Package (LTP), which is the main science payload, will be tested.