Ultra-faint dwarf galaxies (UFDs) are commonly found in close proximity to the Milky Way
and other massive spiral galaxies. As such, their projected stellar ellipticity and extended …

Observational studies are finding stars believed to be relics of the earliest stages of
hierarchical mass assembly of the Milky Way (ie proto-galaxy). In this work, we contextualize …

Understanding the evolution of satellite galaxies of the Milky Way (MW) and M31 requires
modelling their orbital histories across cosmic time. Many works that model satellite orbits …

We present an update to Via Machinae, an automated stellar stream-finding algorithm based
on the deep learning anomaly detector ANODE. Via Machinae identifies stellar streams …

The Hercules ultrafaint dwarf galaxy (UFD) has long been hypothesized to be tidally
disrupting, yet no conclusive evidence has been found for tidal disruption owing partly to …

The third data release (DR3) of Gaia has provided a fivefold increase in the number of radial
velocity measurements of stars, as well as a stark improvement in parallax and proper …

For the first time, systematic studies of dwarf galaxies are being conducted throughout the
Local Volume, including the dwarf satellites of the nearby giant elliptical galaxy Centaurus A …

We present several machine learning (ML) models developed to efficiently separate stars
formed in-situ in Milky Way-type galaxies from those that were formed externally and later …

ABSTRACT The Dark Energy Spectroscopic Instrument Milky Way Survey (DESI MWS) will
explore the assembly history of the Milky Way by characterizing remnants of ancient dwarf …

We analyze the photometric data in the Wide layer of the Hyper Suprime-Cam Subaru
Strategic Program (HSC-SSP) over∼ 1200 deg2 to uncover new halo substructures beyond …