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 …

We present the IRAM-30 m observations of multiple-J CO (J up mostly from 3 up to 8) and
[CI](3 P 2→ 3 P 1)([CI](2–1) hereafter) line emission in a sample of redshift~ 2–4 …

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 …

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 …

We report the detection of CO (J= 2→ 1) emission from three massive dusty starburst
galaxies at z> 5 through molecular line scans in the NSF's Karl G. Jansky Very Large Array …

Using NOEMA and ALMA 3mm line scans, we measured spectroscopic redshifts of six new
dusty galaxies at 3.5< z< 4.2 by solidly detecting [CI](1-0) and CO transitions. The sample …

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 …

Following the first two annual intensity mapping workshops at Stanford in March 2016 and
Johns Hopkins in June 2017, we report on the recent advances in theory, instrumentation …