Within the Local Universe galaxies can be studied in great detail star by star, and here we
review the results of quantitative studies in nearby dwarf galaxies. The color-magnitude …

Positional, structural, and dynamical parameters for all dwarf galaxies in and around the
Local Group are presented, and various aspects of our observational understanding of this …

We present spectroscopic metallicities of individual stars in seven gas-rich dwarf irregular
galaxies (dIrrs), and we show that dIrrs obey the same mass–metallicity relation as the dwarf …

We present uniformly measured star formation histories (SFHs) of 40 Local Group (LG) dwarf
galaxies based on color–magnitude diagram (CMD) analysis from archival Hubble Space …

We use high-resolution simulations of isolated dwarf galaxies to study the physics of dark
matter cusp-core transformations at the edge of galaxy formation: M 200= 107–109 M⊙. We …

Galaxy morphology is a product of how galaxies formed, how they interacted with their
environment, how they were influenced by internal perturbations, AGN, and dark matter, and …

We present a suite of 15 cosmological zoom-in simulations of isolated dark matter haloes, all
with masses of M halo≈ 1010 M⊙ at z= 0, in order to understand the relationship among …

We present MMT spectroscopic observations of H ii regions in 42 low luminosity galaxies in
the Spitzer Local Volume Legacy survey. For 31 of the 42 galaxies in our sample, we were …

We present uniformly measured star formation histories (SFHs) of 60 nearby (D≲ 4 Mpc)
dwarf galaxies based on color–magnitude diagrams of resolved stellar populations from …

We study star formation histories (SFHs) of 500 dwarf galaxies (stellar mass) from FIRE-2
cosmological zoom-in simulations. We compare dwarfs around individual Milky Way (MW) …