We review progress over the past decade in observations of large-scale star formation, with
a focus on the interface between extragalactic and Galactic studies. Methods of measuring …

The Binary Population and Spectral Synthesis suite of binary stellar evolution models and
synthetic stellar populations provides a framework for the physically motivated analysis of …

We present Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …

We use the chemical evolution predictions of cosmological hydrodynamic simulations with
our latest theoretical stellar population synthesis, photoionization, and shock models to …

Aims. Photometric data of galaxies covering the rest-frame wavelength range from far-UV to
far-IR make it possible to derive galaxy properties with a high reliability by fitting the …

We investigate the effect of metallicity calibrations, AGN classification, and aperture covering
fraction on the local mass-metallicity (MZ) relation using 27,730 star-forming galaxies from …

We combine Hα emission-line and infrared (IR) continuum measurements of two samples of
nearby galaxies to derive dust attenuation-corrected star formation rates (SFRs). We use a …

Galactic winds are a prime suspect for the metal enrichment of the intergalactic medium
(IGM) and may have a strong influence on the chemical evolution of galaxies and the nature …

We present results from our on-going MusE GAs FLOw and Wind (MEGAFLOW) survey,
which consists of 22 quasar lines of sight, each observed with the integral field unit MUSE …

We characterize the mass-dependent evolution of more than 8000 galaxies using
spectroscopic redshifts from the DEEP2 Galaxy Redshift Survey in the range 0.4< z< 1.4 and …