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 …

Abstract The Milky Way halo was predominantly formed by the merging of numerous
progenitor galaxies. However, our knowledge of this process is still incomplete, especially in …

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 present the discovery of DELVE 6, an ultra-faint stellar system identified in the second
data release of the DECam Local Volume Exploration (DELVE) survey. Based on a …

Stellar streams are excellent probes of the underlying gravitational potential in which they
evolve. In this work, we fit dynamical models to five streams in the Southern Galactic …

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 …

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 …