The tip of the red giant branch has been used to measure distances to 500 nearby galaxies
with the Hubble Space Telescope (HST) which are available in the Color–Magnitude …

We report the discovery of Tucana B, an isolated ultra-faint dwarf galaxy at a distance of D=
1.4 Mpc. Tucana B was found during a search for ultra-faint satellite companions to the …

We show how the interplay between feedback and mass-growth histories introduces scatter
in the relationship between stellar and neutral gas properties of field faint dwarf galaxies () …

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 results from an optical search for Local Group dwarf galaxy candidates
associated with the Ultra-Compact High Velocity Clouds (UCHVCs) discovered by the …

Mergers play a complex role in galaxy formation and evolution. Continuing to improve our
understanding of these systems requires ever larger samples, which can be difficult (even …

Low-mass dwarf galaxies are expected to reside within dark matter haloes that have a
pristine,'cuspy'density profile within their stellar half-light radii. This is because they form too …

We report the discovery of three faint and ultrafaint dwarf galaxies—Sculptor A, Sculptor B,
and Sculptor C—in the direction of NGC 300 (D= 2.0 Mpc), a Large Magellanic Cloud–mass …

We report the discovery of Corvus A, a low-mass, gas-rich galaxy at a distance of
approximately 3.5 Mpc, identified in DR10 of the Dark Energy Camera Legacy Imaging …

We use panoramic optical spectroscopy obtained with the Very Large Telescope/MUSE to
investigate the nature of five candidate extremely isolated low-mass star-forming regions …