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Gaia-like astrometry and gravitational waves
DOI: 10.1088/1361-6382/aa9f57 Bibcode: 2018CQGra..35d5005K

Klioner, Sergei A.

This paper discusses the effects of gravitational waves on high-accuracy astrometric observations such as those delivered by Gaia. Depending on the frequency of gravitational waves, two regimes for the influence of gravitational waves on astrometric data are identified: the regime when the effects of gravitational waves directly influence the deri…

2018 Classical and Quantum Gravity
Gaia 43
Light propagation in 2PN approximation in the field of one moving monopole I. Initial value problem
DOI: 10.1088/1361-6382/aa9976 Bibcode: 2018CQGra..35e5013Z

Zschocke, Sven

In this investigation the light propagation in the gravitational field of one arbitrarily moving body with monopole structure is considered in the second post-Newtonian approximation. It is found that the light trajectory depends on the acceleration of the body. Some of these acceleration terms are important in order to get well-defined logarithmi…

2018 Classical and Quantum Gravity
Gaia 10
Measuring fN force variations in the presence of constant nN forces: a torsion pendulum ground test of the LISA Pathfinder free-fall mode
DOI: 10.1088/1361-6382/aaa00f Bibcode: 2018CQGra..35c5017R

Russano, G.; Cavalleri, A.; Cesarini, A. +11 more

LISA Pathfinder is a differential accelerometer with the main goal being to demonstrate the near perfect free-fall of reference test masses, as is needed for an orbiting gravitational wave observatory, with a target sensitivity of 30 fm s-2 Hz-1/2 at 1 mHz. Any lasting background differential acceleration between the two test…

2018 Classical and Quantum Gravity
LISAPathfinder 10