Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …

This report summarises progress made in estimating the local density of dark matter (ρ
DM,⊙), a quantity that is especially important for dark matter direct detection experiments …

We use the data from Gaia Early Data Release 3 (EDR3) to study the kinematic properties of
Milky Way globular clusters. We measure the mean parallaxes and proper motions (PM) for …

We assemble a catalogue of candidate Sagittarius stream members with 5D and 6D phase-
space information, using astrometric data from Gaia DR2, distances estimated from RR …

Gravitational interactions between the Large Magellanic Cloud (LMC) and the stellar and
dark matter halo of the Milky Way are expected to give rise to disequilibrium phenomena in …

Aims. We perform a comprehensive determination of the systemic proper motions of 74
dwarf galaxies and dwarf galaxy candidates in the Local Group based on Gaia early data …

We review the recent theoretical and observational developments concerning the interaction
of the Large Magellanic Cloud (LMC) with the Milky Way and its neighbourhood. An …

Indications of disequilibrium throughout the Milky Way (MW) highlight the need for compact,
flexible, non-parametric descriptions of phase–space distributions of galaxies. We present a …

The Gaia mission has revolutionized our view of the Milky Way and its satellite citizens. The
field of Galactic Archaeology has been piecing together the formation and evolution of the …

We propose a scenario in which the Large Magellanic Cloud (LMC) is on its second
passage around the Milky Way. Using a series of tailored N-body simulations, we …