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 …

Line intensity mapping (LIM) is rapidly emerging as a powerful technique to study galaxy
formation and cosmology in the high-redshift Universe. We present LIM estimates of select …

We present a detailed overview of the science goals and predictions for the Prime-Cam
direct-detection camera–spectrometer being constructed by the CCAT-prime collaboration …

Abstract The CO Mapping Array Project (COMAP) aims to use line-intensity mapping of
carbon monoxide (CO) to trace the distribution and global properties of galaxies over cosmic …

We present a detection of molecular gas emission at z∼ 1–5 using the technique of line
intensity mapping. We make use of a pair of 3 mm interferometric data sets, the first from the …

We present the current state of models for the z∼ 3 carbon monoxide (CO) line intensity
signal targeted by the CO Mapping Array Project (COMAP) Pathfinder in the context of its …

Line intensity mapping (LIM) is a rapidly emerging technique for constraining cosmology
and galaxy formation using multi-frequency, low angular resolution maps. Many LIM …

Submillimeter emission lines produced by the interstellar medium (ISM) are strong tracers of
star formation and are some of the main targets of line intensity mapping (LIM) surveys. In …

Line intensity mapping (LIM) is an emerging technique with a unique potential to probe a
wide range of scales and redshifts. Realizing the full potential of LIM, however, relies on …

Submillimeter emission lines are important tracers of the cold gas and ionized environments
of galaxies and the targets for future line intensity mapping surveys. Physics-based …