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 …

We use GRUMPY, a simple regulator-type model for dwarf galaxy formation and evolution,
to forward model the dwarf galaxy satellite population of the Milky Way (MW) using the …

The orbits of satellite galaxies encode rich information about their histories. We investigate
the orbital dynamics and histories of satellite galaxies around Milky Way (MW)-mass host …

Understanding quenching mechanisms in low-mass galaxies is essential for understanding
galaxy evolution overall. In particular, isolated galaxies are important tools to help …

So far, numerical simulations of ultra-faint dwarf galaxies (UFDs) have failed to properly
reproduce the observed size–luminosity relation. In particular, no hydrodynamical simulation …

We use the APOSTLE cosmological simulations to examine the role of the cosmic UV
background in regulating star formation (SF) in low-mass Lambda cold dark matter (ΛCDM) …

We use the APOSTLE Local Group (LG) cosmological hydrosimulations to examine the
properties of 'backsplash'galaxies, ie dwarfs that were within the virial boundaries of the …

We study the relative fractions of quenched and star-forming satellite galaxies in the
Satellites Around Galactic Analogs (SAGA) survey and Exploration of Local VolumE …

Abstract Interpretation of data from faint dwarf galaxies is made challenging by observations
limited to only the brightest stars. We present a major improvement to tackle this challenge …

We present the first comprehensive census of the satellite population around a Large
Magellanic Cloud stellar-mass galaxy, as part of the Magellanic Analog Dwarf Companions …