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

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 …

SPT0311-58 is the most massive infrared luminous system discovered so far during the
Epoch of Reionization (EoR). In this paper, we present a detailed analysis of the molecular …

Exploiting the sensitivity of the IRAM NOrthern Extended Millimeter Array (NOEMA) and its
ability to process large instantaneous bandwidths, we have studied the morphology and …

By using data from the Atacama Large Millimeter/submillimeter Array and near-infrared
(NIR) integral field spectrographs, including both Spectrograph for INtegral Field …

Aims. We present and study spatially resolved imaging obtained with the Atacama Large
Millimeter/submillimeter Array (ALMA) of multiple 12 CO (J= 6− 5, 8− 7, and 9− 8) and two H …

High-redshift dusty star-forming galaxies with very high star formation rates (500− 3000 M⊙
yr− 1) are key to understanding the formation of the most extreme galaxies in the early …

We report the discovery of a high-redshift, massive molecular outflow in the starburst galaxy
SPT 0346-52 (z= 5.656) via the detected absorption of high-excitation water transitions (H 2 …

Abstract Water (H 2 O), one of the most ubiquitous molecules in the universe, has bright
millimeter-wave emission lines that are easily observed at high redshift with the current …

The molecular gas content of high-redshift galaxies is a highly sought-after property.
However, H2 is not directly observable in most environments, so its mass is probed through …