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 …

▪ Abstract Observations of star formation rates (SFRs) in galaxies provide vital clues to the
physical nature of the Hubble sequence and are key probes of the evolutionary histories of …

The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ∼
5 - IOPscience This site uses cookies. By continuing to use this site you agree to our use of …

Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …

We present a comprehensive study of the physical properties of∼ 105 galaxies with
measurable star formation in the Sloan Digital Sky Survey (SDSS). By comparing physical …

The formation of the first stars and quasars marks the transformation of the universe from its
smooth initial state to its clumpy current state. In popular cosmological models, the first …

The Lyman decrement associated with the cumulative effect of H i in QSO absorption
systems along the line of sight provides a distinctive feature for identifying galaxies at z≳ 2.5 …

The transformations that take place in late‐type galaxies in the environment of rich clusters
of galaxies at z= 0 are reviewed. From the handful of late‐type galaxies that inhabit local …

We investigate the 21 cm signature that may arise from the intergalactic medium (IGM) prior
to the epoch of full reionization (z> 5). In scenarios in which the IGM is reionized by discrete …

We develop a method for interpreting faint galaxy data which focuses on the integrated light
radiated from the galaxy population as a whole. The emission history of the universe at …