Line-intensity mapping (LIM) is an emerging approach to survey the Universe, using
relatively low-aperture instruments to scan large portions of the sky and collect the total …

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 …

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 …

All measurements of cosmic star formation must assume an initial distribution of stellar
masses—the stellar initial mass function—in order to extrapolate from the star-formation rate …

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 …

Context. Sources at the brightest end of the quasi-stellar object (QSO) luminosity function,
during the peak epoch in the history of star formation and black hole accretion (z∼ 2− 4 …

We have used ALMA and NOEMA to study the molecular gas reservoirs in 61 ALMA-
identified submillimetre galaxies (SMGs) in the COSMOS, UDS, and ECDFS fields. We …

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 …

We present a multiline survey of the interstellar medium (ISM) in two z> 6 quasar host
galaxies, PJ231− 20 (z= 6.59) and PJ308− 21 (z= 6.23), and their two companion galaxies …

The intensity mapping of the [CII] 158-μm line redshifted to the submillimeter window is a
promising probe of the z> 4 star formation and its spatial distribution into large-scale …