The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

We study the abundance of substructure in the matter density near galaxies using ALMA
Science Verification observations of the strong lensing system SDP. 81. We present a …

We present a self-consistent cross-calibration of the three main molecular gas mass tracers
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …

Abstract The South Pole Telescope (SPT) has systematically identified 81 high-redshift,
strongly gravitationally lensed, dusty star-forming galaxies (DSFGs) in a 2500 square …

THE EVOLUTION OF INTERSTELLAR MEDIUM MASS PROBED BY DUST EMISSION: ALMA
OBSERVATIONS AT z = 0.3–2 - IOPscience Skip to content IOP Science home Accessibility …

Dusty star-forming galaxies at high redshift (1< z< 3) represent the most intense star-forming
regions in the universe. Key aspects to these processes are the gas heating and cooling …

A critical challenge to the cold dark matter (CDM) paradigm is that there are fewer satellites
observed around the Milky Way than found in simulations of dark matter substructure. We …

We show how LIGO is expected to detect coalescing binary black holes at z> 1 that are
lensed by the intervening galaxy population. Gravitational magnification, μ, strengthens …

We present the IRAM-30 m observations of multiple-J CO (J up mostly from 3 up to 8) and
[CI](3 P 2→ 3 P 1)([CI](2–1) hereafter) line emission in a sample of redshift~ 2–4 …