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 field of dark matter detection is a highly visible and highly competitive one. In this paper,
we propose recommendations for presenting dark matter direct detection results particularly …

The growing trove of precision astrometric observations from the Gaia space telescope and
other surveys is revealing the structure and dynamics of the Milky Way in ever more …

Abstract The Large Magellanic Cloud is the most massive satellite galaxy of the Milky Way,
with an estimated mass exceeding a tenth of the mass of the Milky Way,,,–. Just past its …

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 …

Data from the Gaia satellite show that the solar neighborhood of the Milky Way's stellar halo
is imprinted with substructure from several accretion events. Evidence of these events is …

Now that conventional weakly interacting massive particle (WIMP) dark matter searches are
approaching the neutrino floor, there has been a resurgence of interest in detectors with …

We study the effect of the Large Magellanic Cloud (LMC) on the dark matter (DM) distribution
in the Solar neighborhood, utilizing the Auriga magneto-hydrodynamical simulations of Milky …

Recent observations of high-energy neutrinos from active galactic nuclei (AGN), NGC 1068
and TXS 0506+ 056, suggest that cosmic rays (CRs) are accelerated in the vicinity of the …

If dark matter has mass lower than around 1 GeV, it will not impart enough energy to cause
detectable nuclear recoils in many direct-detection experiments. However, if dark matter is …