Over the past decade, observations of the cool interstellar medium (ISM) in distant galaxies
via molecular and atomic fine structure line (FSL) emission have gone from a curious look …

▪ Abstract The Early Universe Molecular Emission Line Galaxies (EMGs) are a population of
galaxies with only 36 examples that hold great promise for the study of galaxy formation and …

We investigate the CO excitation and interstellar medium (ISM) conditions in a cold gas
mass-selected sample of 22 star-forming galaxies at z= 0.46–3.60, observed as part of the …

The Properties of the Interstellar Medium of Galaxies across Time as Traced by the Neutral
Atomic Carbon [C i] - IOPscience This site uses cookies. By continuing to use this site you …

The growth of galaxies in the early Universe is driven by accretion of circum-and
intergalactic gas. Simulations have predicted that steady streams of cold gas penetrate the …

Abstract We used the Atacama Large Millimeter/Submillimeter Array (ALMA) to map the CO
(3–2) and [C i](1–0) lines, as well as their underlying continuum emission, from the central∼ …

We analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies
between redshifts 1.4 and 4.6 detected by the Atacama Large Millimeter/submillimeter Array …

Abstract We present Atacama Large Millimeter Array [C i](1− 0)(rest frequency 492 GHz)
observations for a sample of 13 strongly lensed dusty star-forming galaxies (DSFGs) …

We present a high sensitivity, ground-based spectral line survey of low-J carbon monoxide
(CO (J up→ J up− 1) with J up= 1, 2, 3) and neutral carbon [CI] 3 P 1− 3 P 0 ([CI](1–0)) in 36 …

We examine the fine structure lines 3 P 1→ 3 P 0 (492 GHz) and 3 P 2→ 3 P 1 (809 GHz) of
neutral atomic carbon as bulk molecular gas mass tracers and find that they can be good …