The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical
property of the system, including the star-formation history, metal content, abundance …

Inference of the physical properties of stellar populations from observed photometry and
spectroscopy is a key goal in the study of galaxy evolution. In recent years, the quality and …

Feedback to the interstellar medium from ionizing radiation, stellar winds and supernovae is
central to regulating star formation in galaxies. Owing to their low mass (< 109 solar …

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 present an all-sky catalog of 869 nearby galaxies having individual distance estimates
within 11 Mpc or corrected radial velocities V LG< 600 km s− 1. The catalog is a renewed …

We examine the effects of stellar feedback and bursty star formation on low-mass galaxies
(M star= 2× 10 6− 5× 10 10 M⊙) using the Feedback in Realistic Environments (FIRE) …

We demonstrate that dwarf galaxies (10 7< M stellar< 10 9 M☉,− 12> M r>− 18) with no
active star formation are extremely rare (< 0.06%) in the field. Our sample is based on the …

Abstract We introduce the Making Galaxies In a Cosmological Context (MAGICC)
programme of smoothed particle hydrodynamics simulations. We describe a parameter …