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 …

Star formation lies at the center of a web of processes that drive cosmic evolution:
generation of radiant energy, synthesis of elements, formation of planets, and development …

Abstract The Widefield ASKAP L-band Legacy All-sky Blind surveY (wallaby) is a next-
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …

ABSTRACT We use CANUCS JWST/NIRCam imaging of galaxies behind the gravitationally-
lensing cluster MACS J0417. 5-1154 to investigate star formation burstiness in low-mass …

We present results on the dust attenuation curve of z∼ 2 galaxies using early observations
from the MOSFIRE Deep Evolution Field survey. Our sample consists of 224 star-forming …

The observation of quasars at very high redshift such as Pōniuā'ena is a challenge for
models of supermassive black hole (SMBH) formation. This work presents a study of SMBH …

In the companion Paper XV of this series, we derive accurate total mass-to-light ratios within
a sphere of radius centred on the galaxy, as well as stellar (M/L) stars (with the dark matter …

We investigate the burstiness of star formation and the ionizing efficiency of a large sample
of galaxies at 0.7< z< 1.5 using HST grism spectroscopy and deep ultraviolet (UV) imaging …

We present new calibrations of far-ultraviolet (FUV) attenuation as derived from the total
infrared to FUV luminosity ratio (IRX) and the FUV–near-UV (NUV) color. We find that the …

Whether the stellar initial mass function (IMF) is universal or is instead sensitive to
environmental conditions is of critical importance: The IMF influences most observable …