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 …

ISM MASSES AND THE STAR FORMATION LAW AT Z = 1 TO 6: ALMA OBSERVATIONS
OF DUST CONTINUUM IN 145 GALAXIES IN THE COSMOS SURVEY FIELD - IOPscience …

Aims. We present a 69 arcmin 2 ALMA survey at 1.1 mm, GOODS-ALMA, matching the
deepest HST-WFC3 H-band part of the GOODS-South field. Methods. We tapered the 0 ″24 …

Three billion years after the big bang (at redshift z= 2), half of the most massive galaxies
were already old, quiescent systems with little to no residual star formation and extremely …

We aim to measure the average dust and molecular gas content of massive star-forming
galaxies (> 3× 10 10 M⊙) up to z= 4 in the COSMOS field to determine if the intense star …

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 …

Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large
Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally …

Massive galaxy clusters have been found that date to times as early as three billion years
after the Big Bang, containing stars that formed at even earlier epochs,–. The high-redshift …